What is going on guys today? I am back with another destiny video and today I'm gonna give you guys what in my opinion is the best PVP pulse rifle in this game And I'm gonna tell you guys how you can get it quite easily to be honest Scavenging them fucking tags on his weapon just Tears Before we get into the video guys, if you want to be with a chance of winning this resurrectionist emblem seen on screen now Simply drop a like and leave a comment details are on screen with that emblem Chips and Okay, so the pulse rifle I am talking about is none other than the serious PDX 421 now I am banner is a is around now surround for the next three or four days and Actually three or four. Yeah about five days, whatever And it means I'm playing a lot more PVP now because I like to do I am better. I like to get that loot Guns a monster. Oh, it's such a beast sidearms even trying to get rewards I haven't got and So it's time to pull out a weapon. I'm nose decent and this is it right here Don't put your luck out. Oh you noob Now I've used it in about 20 games on two characters and absolutely destroyed With it. I really have Based though actually have one two three of these I got another one waiting And that's exactly how you get these you get them from the gunsmith Simply go there of a Wednesday Pick up the serious PDX 41 package and wait until next Wednesday until he brings a decent Well, he may not bring a decent role the first week But if he brings three roles every week as you may know with gunsmith weapons And there's a chance he may bring a great role for you now show you guys my three Start enough with this one right here on this. I've got perfect balance counterbalance and injection mold Stability all day every day doesn't bounce at all on this one. I have Appended mag or hammer forged full auto and hand-laid stuck or lightweight Which is a monster because obviously I keep tapping the trigger Which I sometimes puts me off and because I've got full auto on that one It's actually quite decent this one here, which is my favorite. This thing just is it's a headshot machine On this we've got a pending appended mag We've got perfect balance. We've got a counter balance and we've got a rifle would barrel now this one is It's just the beast. I mean look at that range. Look at the range Have you ever seen anything like that on a Porsche rifle so you can imagine how accurate this thing is? Crust and map it doesn't matter where you are.  You're going nowhere other pulse rifles that are Could be as good. I mean, I just don't give them a chance I know I like you guys in the comment section will be saying well this weapons just as good or that weapons just as good Oh, this is my go to pulse rifle, which is fair enough This is just my opinion on my video on my channel as you guys would probably notice you're watching it here But yeah, hop scotch program one that drops On a regular basis to be honest I'm my one here. I've got I got a red dot OES, which is a decent sight I've got head seeker perfect balance hand-laid stock or small ball with full auto as you can imagine These things are based it really is I still prefer this stuff and this one. I haven't leveled this up yet I've got this recently actually And this I got there red dot or EES I got counterbalance a light weight brash frame and Glass half full shame brash frame takes and well affects magazine size I think it takes it down to about 26 24 something like that so yeah And this one which is a classic which I've just kept forever because it was one of the first of this Archetype pulse rifles I had it's a no wins mercy on this one. I got the red dot OES I've got outlaw perfect balance brash frame which affects mag size But then to be honest look at the difference between the two stability wise I may as well keep on perfect balance and keep my extra like what eight bullets or so and this one about injection mode Which affects range. So yeah, and then we have third eye now I am all up for using anything to PvP which allows me to Keep red on screen when I'm aiming down sight because that helps me a lot It really does I can be aiming down so I don't know if someone's coming around me. So yes But yes guys, this is the sewers pdx 41 Definitely my opinion the best PvP pulse rifle in the game, especially legendary wise anyway It really is and you know how to get it So go get it try it out and let me know what you think down below in that comment section Hope you guys enjoyed the video though, and I will as always see you on that next one Sun strike and he's teabagging me I think I did pretty good then I'm done at four times Life's the part What do I do? What's my KD? 6.5 KD by 44 score Da haaaang


Chris Pratt and Catherine Schwarzenegger, who are best known as the Avengers star actor and renowned author receptively, have finally chosen a mega mansion in the Pacific Palisades. The two have been married since 2019, so it was only fitting that they would snag a place together with their new daughter Lila. We'll take a look at the massive $15.6 million mansion Chris, Catherine, and their new family will be calling home in Hollywood, which is under the radar purchased back in 2017. In these videos, we do not reveal any real addresses, so please do not show up at any private residences because it's not safe for anyone. The Avengers star has accumulated a net worth of $60 million in first roles to fame playing Andy Dwyer on NBC's Parks and Recreation, which aired from 2009 to 2015. After Pratt starred in Guardians of the Galaxy in 2014 and Jurassic World in 2015, he became known as one of the most bankable actors in Hollywood. These films crushed it at the box office and went on to earn more than $700 million and $1.6 billion respectively at the box office. This led Chris into stardom in between June 2016 and June 2017. Chris earned $18 million from his various acting roles. However, it was his role in Jurassic World Fallen Kingdom where Chris broke bank. He went on to earn a career high $10 million. Catherine Schwarzenegger is an American author and has accumulated a net worth of $3 million. She's the eldest child of broadcast journalist Maria Shriver, and you guessed it, the actor and former governor of California Arnold Schwarzenegger. Over her writing career, she has written a number of renowned books including Rock What You've Got, Secrets to Loving Your Inner and Outer Beauty from Someone Who's Been There and Back. Schwarzenegger uses the book to describe her personal journey and encourage other women to achieve confidence and a positive self-image. What a sweetheart. What's going on guys? It's your boy Marlon Palmer and today we're bringing you another house tour here for you on Famous Entertainment. I noticed 95% of you watching aren't subscribed so please be sure to hit that subscribe button because we post new videos daily. We previously reported on the homes of Jason Statham and Keith Urban. If you like these videos, ring that bell for notifications. Make sure you guys follow me on Instagram at that new McFly so we can chat and let me know who's house tour is next in these comments down below. Let's get into the video. Chris Pratt was formally married to star Anna Faris and the former spouses finally sold their secluded and long ago vacated Hollywood Hills residence. The house was originally listed just a tad shy of $5 million but managed to be sold for $4.75 million. Hey, in this economy $200,000 less is a win for me and it was still a substantial raise from the $3.3 million they paid in 2014 for the property. This gated nearly two-thirds of an acre estate, boasts extreme privacy and resort style living just moments away from the heart of Hollywood. With how busy the two actors are it would make sense to have a home so close to their work. The palace was hidden by high hedges and towering poms. The exterior has a Mediterranean design with an alabaster stucco walls and terracotta tiled roof. The inside is a tad more than 4,700 square foot home and contains four bedrooms, 3.5 bathrooms that gives off a cozy laminated and snug modern farmhouse ambience. The entrance contains double glass doors which is tucked into a deep porch and open to a foyer. The archways lead to formal living and dining rooms. The living room features a carved wood fireplace and wood clad vaulted ceiling and contains a family room that is complete with painted oak paneling and another wooden clad vaulted ceiling plus a wet bar. Recently installed since it was first listed the high end mostly all-white kitchen contains snow white shaker style cabinets, gray marble subway tile, backsplashes and a large center island. The French doors in the breakfast area lead out to a poolside covered patio that's heated in the winter by luxurious fixed ceiling heaters in addition to a main floor guest bedroom slash office with direct backyard access. The abode boasts two more guest bedrooms upstairs along with the large primary bedroom that comprises a sitting area, fireplace and a private balcony with backyard view. The main bathroom comes with a jetted tub and multi-person steam shower but may be in need of an update. The terrace outside the kitchen leads to a sunsplash swimming pool and spa set that is against the towering hedge hidden from the main house by a high hedge and chain link fence. 25,000 square foot plus lot is a lighted tennis court and includes an elevated end pavilion that is decked out with a massage table and gym equipment. The lot comes complete with a built-in barbecue and outdoor fireplace, an impressive motor court and three-car garage. Now we all know that Chris Pratt and Anna Faris had split and they both moved on however after Chris split with Anna Faris he upgraded in a major way snagging an unfinished property in the Pacific Palisades for 15.6 million. Pratt made this purchase completely under the radar because he wanted to keep everything private. But let me tell you it is prime real estate and the property boasts spectacular views of the Pacific Ocean and Catalina Island. This breathtaking ocean view villa estate is located behind the exclusive gates of Bella Oceana Vista. After entering through the roomy atrium courtyard guests will be transported through the hills of Tuscany. Elevated ceilings and a perfect indoor-outdoor floor plan create a vibe of both style and grace. All main-level rooms are king-size and offer charming views, the upstairs master suite and adjoining office sitting area is its own luxury. The large grassy backyard has plenty of additional room for pools, spa and any outdoor entertainment that you may desire. This magnificent European estate is perfect for both living and entertaining. It is unclear when construction will be complete but the dwelling will reportedly span an impressive 10,000 square feet with five bedrooms and six bathrooms. It is located in a family-friendly gated community with five other homes, none of which is owned by celebrities. Equally important is that Pratt's new dig is located less than five miles away from Anna Ferris as they had their divorce agreement that they must live within five miles of each other for the sake of their young son Jack. The hillside lot originally housed an 8,000 square foot Mediterranean style home built in 1995 but that was before it was expanded into the planned 10,000 square foot abode with a more traditional style feel. Along with the newly installed infinity edge swimming pool and spa, other amenities will include a home gym, a wine cellar and a pool house as well as a magnificently sized garage capable of holding multiple luxury vehicles. Photos of the property show that it stands three stories tall. In addition to their mansion in the Pacific Palisades, Pratt has been known to leak photos of himself and his farmhouse. However, Pratt gave a glimpse inside this and Catherine's new home. The Instagram post features cute photos of Catherine posing as a measuring stick to measure the abode. The dwelling features hardwood paneling on the walls and floors with high ceilings and a balcony with beautiful countryside views. Now while Chris didn't reveal where the new home is, the couple have been spending a lot of time on the farm he owns on the San Juan Islands in Washington so it may well be nearby. The actor has also welcomed some new additions to the farm including a 160 sheep, 30 pigs and 60 chickens on his San Juan Island farm off the coast of Washington State. Chris has previously said that he would like to spend more time at the farm in the years to come and plans to spend less time working. Alright so I think I'll bring this house tour to an end. We got to take a look at Chris Pratt's former home with Anna Ferris in the Hollywood Hills and his new extravagant mansion in the Pacific Palisades with his new wife, Catherine Schwarzenegger. After seeing that $15.6 million abode he snagged, what do you guys think? Was it better or worse than his former home with Anna Ferris? Personally, I think I would rather live at the farm out of Chris Pratt's home which was your fave. You guys can go ahead and rate them in the comments down below. Also love it if you guys subscribe to my personal channel, DaddoomitFly. I don't post often but you know I might, I might. Thank you guys so much for watching and I'll catch you guys next video.


When I was in grade school, I'd often be looking out the window studying the clouds instead of studying the text in front of me. I was always interested in astronomy. I mean, since I was a baby, it was just fascinating to me. Thinking of things that were so far away, in just philosophical terms, like, wow, the Earth is such a minor, small part of the entire universe. I brought home rocks and bugs and things at the youngest age I could imagine, wondering why spiders have been webs or why there are some large insects and small ones. Well, when I was a child I was playing around. I was just interested. I wanted to know how to do stuff and how to think about stuff, and I wanted to see the stars with my telescope. I was always interested in problems or projects where you have something to do, maybe you don't know how to do it, but you need to have something done at the end. It was a very gradual process from just going out and observing nature on my own and becoming a professional at it. We're all curious, and when we're curious about the natural world, the natural universe, the stuff around us where we live, breathe, our planet lives and breathes, and that's the first start of science. It seems to me, if you want to be a scientist, then you just have to start and put your heart into it and immerse yourself in it as much as you can. Don't postpone doing what you want to do. Do it right now and go as deeply into it right now as you can. We don't legislate physics or chemistry or biology. The natural world does, and that's what's so fun. It's a puzzle. To me, it seems sciences are among the most exciting things we could be thinking about these days. Scientists are discovering so many fascinating things, partly because we have new tools and we can be participants in it. That's just so rewarding to be discovering the secrets of the universe.


Everybody forced here ripping There's my stuff here. Yeah, uh, six bucks number six of 2023 luminance football hobby pick your team style Just waiting for the names to load up here Come on now Shopify Erin E Steelers Alvin S Falcons Andrew M Niners Anthony G With the Rams Austin B Bears Brad M has the Giants Brandon S bucks Carl C Cardinals Dain B Vikings Jisuke Saints Dave a Browns David H Broncos Derek B Seahawks Don G Lyons Edward P Eagles Chiefs Eric W Ravens Jeremy P with the Jets Jerry B with the Raiders Jonathan B Patriots Josh C with the Colts Matthew G Titans Michael J. Dolphins Mike Y with the Jags Nathan Q Bengals Patrick H Packers Richard L Bills and Panthers Shawna has the Cowboys and Texans Towel in Chargers Terry R with Washington. He just a sec to get started here Hey guys teams on sale. Let's get them filled up Usually we do PYT's at first when releases drop. Yeah, usually PYT's first Ijan got Olave Saints to 250 250 points and Savage of Mike Evans Yeah, just your ones are in pro jersey and it's not all of them. It's only some of them Craft rice mingo. You've got a baker to 50 for the Bucks Cowboys Deuce Vaughn you're one rookie on a card on it and engaged Aaron Donald. So when he runs out I would I might it's for comedic effects, but no You've got I'm on rada 150 for the Lions Saints on the Kendra Miller rookie red year one auto and DeMar Hamlin, that's pretty cool. That's pretty sick Unforgettable DeMar Hamlin that is fire actually might be the coolest card in the whole and the whole product right there Jasmine Ritter Jersey card for the foul for the Falcons there rookie to 75 Sam La Porta Lions Deuce Vaughn rookie to 175 Cowboys and Russ to 50 vestige God Strange Scott Butte rookie to 150 Marvin Mims for Denver Orange points now random to everybody at the end Engaged Nick Bosa, not Nick Bosa. Sorry, Nick Bolton the chiefs Nick Bolton Saw Nick B saw someone get tackled. I just wanted the autopilot People guys getting tackled all of them man. They're all getting tackled All right guys teams on sale just five to go on the next one So Richardson rookie for the Colts Bryce young the Panthers there Joe mixing out of 250 Bengals They Cowboys Deuce Vaughn you're one rookie on a card auto fusion of Chase Bijan Robinson and Christian Gonzalez Clayton Tune Dorian Thompson Robinson rookie to 200 for the Browns They Brown Cedric Tillman rookie auto to 100 Savage of Etienne there Mingo Evan Neal Jalen Hyatt Dual Giants jerseys here is Daniel Jones and Eli Manning player worn Miles Murphy rookie for uh sin C to 75 Got Ty J Spears the 175 rookie Titans and a dynamic Jameer Gibbs ox three It's a bargain. It's going well It's going on Derek All right guys carnells ravens bills bucks and Titans Got rogers here out of 250 for the Packers 250 points random at the end everybody unforgettable jamar chase Spears mayor Tucker rookie chase brown Bengals out of 200 A loose schoonmacher rookie year one auto Cowboys doing really well here And dynamic CJ Stroud for the Texans Let me see a big-time Stroud now That'd be cool and then Hooker about a conda dante banks Daniel Jones out of 150 Giants Packers rookie auto to 25 Tucker Kraft Bonte Adams Will Leviss base there Damian Pierce jersey card for the Texans Bright beginnings That is rookie to 35 Devon Ashane for the Dolphins. It's a nice one Mack Jones pats to 100 Plus unforgettable Chandler Jones for the Raiders to 100 Brutal ravenge just sold carnells just sold down to Bill's bucks Titans, so just three to go now And there are teams on sale for NT football as well a lot of teams mark down All right, let's keep it rolling the Maryland love mayor Wilson Ashane Mix in number to 250 for the Bengals another points card here 250 random at the end fusion Jefferson less points more autos I think we literally matched what we though came out of the case when we came out of the other half Yeah Branch there is Anthony Richardson to 175 Colts rookie Roshan Johnson rookie auto to 350 for the Bears And a gara wilson There is a Bennett Eric gray rookie numbered to 200 for the Giants Hardy and Nickerson on the bear on the on the box auto here eight of 10 shutter signatures And Cooper cup unforgettable ed reed ravens jersey card player Warren rushy rice rookie out of 25 for the chiefs Terry McLauren out of 150 for the commanders And josh Allen vestige to 50 for the uh bills Biggest hit today probably the Trevor Lawrence auto to three that we pulled Even over that Richardson just because it's super low numbered Gala march accent at 250 for the ravens pulled the Richardson purple auto jamir gibbs rookie year one auto there you go lions forgettable mike evans Hit a joe borough animation. We hit a dual auto jamir gibbs v. John robinson pulling heat and hooker auto to five Van ness rookie for the Packers to 200 Because van ness Tyler Scott rookie auto out of 50 for the Bears Like a Parsons engaged Herbert out of 150 for the Chargers Followed by a Cedric Tillman Brown's rookie auto year one on card And nick bose of vestige Because everybody up to today everybody working. We have like almost 200 viewers, which is crazy for a wednesday daytime Flowers josh allen bills jersey card beacons with Texans rookie will Anderson to 150 Lamar Jackson out of 100 for the ravens As well as an engaged 100 seahawks to mall atoms Just marked NT teams down some more everybody looking for some NT During the day here, but the next break is at three to go bills bucks and Titans all on sale You sure to like the streaming for watching on youtube give us a follow if you're on twitch Make sure you subscribe if you're on youtube Will Anderson wicks murphy. We've got a Watson out of 100 for the Packers God rookie auto jamir gibbs year one on card again two of them last two boxes It's a lot Shane smith and jigba rookie Kenny Macintosh to 150 seattle Rashi rice rookie auto chiefs the 350 fusion jesson jefferson Addison Bonsai Adams out of 250 for the Raiders Chase brown bangles rookie red year one auto and last pack. Thanks for filling this up everybody It is much appreciated Okay, Bijan Dallas you got Dak Jersey here Beacon Jersey Dak Prescott Bryce young to 175 rookie for the Panthers. There we go There's a Levis the 200 for the Titans as well nice And unforgettable Cooper cup. All right four points guards here top four in the random top spot gets 400 spots two three and four each get 200 Good luck Eight times six and two Gonna be top four gonna get points here One two three and four Bills get the 400 Then it goes rams vikings patreons All right relics we had Dak Josh Allen ed reed Damian pierce daniel jones elie manning Desperator autos of cedric tilman jamir gibbs twice on the year one on card Luke schoonmacher duce vaughn duce vaughn A lot of your ones man a red chase brown and a red kendre miller autos of rashi rice roshan johnson Cedric tilman hardy nickerson 20 to 50 was a tyler scott and to 25 was a tucker craft. Thanks everybody Okay, eight times. I'm sorry that is those. Yeah, it was eight times. We got to keep roll. We're gonna keep randomizing Thank you for calling that out a little too fast right here We got to go four more times. So I'm just gonna copy those results and we're just gonna randomize it Four more times here. Sorry about that. Those were not where the points go So again, I just copied this That was what we had we'll go four more times with that one two three and four Broncos get the 400 then it's panthers rams and eagles Broncos panthers rams and eagles Sorry about that guys moving on


Today, I have the pleasure of speaking with Michael Schuster. How are you today, Michael? Pretty good. Pretty good. Nice to be back in Toronto. Michael, the last time, I think we met initially during the Rare Earth Boom in 2010. 2010, yeah. It seems like yesterday, doesn't it? And it was a PDAC. Was it not? PDAC, and you were hosting a party for another company. Of course, now we're trying to get some of the cannabis investors excited about diversifying their portfolio. And, of course, you have all the energy metals, or a lot of the top ones. Well, I've been doing the Rare Earth, which is really part of the energy story, too. So I've been doing all those specialty metals for probably about 25 years. So it's not something we jump on the bandwagon and off, we're always into the specialty metals. All right. So, Michael, we know you're here in the game to stay, but can you tell us what your number one priority is presently? Right now, we've got a project in New Brunswick, it was a former Noranda project. It had exceptional cobalt numbers. I've looked at thousands of cobalt projects all over the world. When I saw this, the numbers were so good, I thought we go PPMs to PPBs. I thought for sure this is PPBs, which is a smaller number, because the numbers were so high. So when I confirmed it with the ex-Noranda guys, looked at all the old data, I said I've got to get this. So we have cobalt, we have nickel, nickel and copper. And copper, which of course is one of the top technology metals. Yeah, nobody knows that, I think, but it is. So of course, everybody knows you for reputation. You've taken this company, changed its name, what's different? Well part of it is, I think the market is really into the energy materials now, much more than say, you know, we look back at 2010 rares, we're kind of new. Everybody knows that story that the materials are there. So I thought we were just ready to relaunch and rebrand and go with it. The market, in our opinion, has never been more competitive. You're one of the many companies out there. Of course, you have a great deal of knowledge and expertise, an amazing management team, Michael. Great team you've built here. Can you tell me what your biggest competitive advantages are? Well I think we've got one of the best cobalt projects out there. And it's also copper nickel, which is not bad commodity space either. Sorry, why is it one of the best projects in the world? I want to know, Michael. Because of the geophysics that was previously done by Noranda. We have a very world-class target on the geophysics. We've done a brand new survey using expert geophysics, the best guys in the world. I had Kit Campbell, probably the best geophysicist in the world. Kit watches this, he'll like that. I think he is. And he came up with some pretty convincing targets.  Geophysics, tell us what that really means for all of us cannabis investors that are straight out of high school. Well number one, in the mining journey or mining space, you want something huge. And the geophysics tell you if you've got something huge. So we do have something big, a big target. We put a couple drill holes in it. We will look like a marijuana stock once we get some results. We will look like a marijuana stock. I love it. How should we anticipate this spring? I think that the stock price will creep up as everybody knows we're getting closer to the drill program. We're fully funded so we don't have to raise money. We're a very well-structured company so that if we get some good news, the stock can really move. And I've got some really influential investors, sophisticated mining investors and probably some of the best guys in Vancouver are backing the project on the pure science of it. Okay. For the pure science of it, love it. Thank you so much for joining us today, Michael. Okay, thank you.


So there are notes, at least for the first two lectures, they're putting it on the web page. So hopefully by tomorrow or Tuesday, you'll have the second two lectures. OK, so there's a new ingredient that I'll describe today, so I've given already, I guess, three sets of lectures at ICTP on pure spinor formalism. But there's a new ingredient now that I think is better understood, which is where the formalism comes from. So I'll spend today, today I have two lectures. So I'll spend most of today's lectures discussing these new ingredients. So let me start with motivation. And then to simplify things, I will discuss first the super particle. So the super particle is, of course, the massless degree of freedom in the string. And most of the issues that come up in the string already come up in the particle or in the super particle. So I'll discuss this in three different languages. So first with green Schwartz, then with pure spinner. And then finally, I'll give this twister-like description, which will generalize to the string. And in some sense, unlike these two formalism, this will be completely gauge invariant. These two descriptions can be understood as gauge-fixed versions of this. OK, then we'll go to the string. So these things I will try to cover today. Then we'll discuss, of course, the super string, which is the main focus. And first, we'll discuss vertex operators and tree amplitudes. So this will probably be done tomorrow. And then finally, we'll discuss multi-loop amplitudes. To do this, we'll have to introduce some new degrees of freedom that I'll describe, non-minimal. And this will require a construction of something called a b-ghost. And with this, we'll be able to compute multi-loop amplitudes. OK, so what I won't have time to discuss in these lectures are curved backgrounds. But if you're interested, you can look at previous lectures on that. So let me give you some references. OK, so as I already mentioned, there'll be notes on the web page. But you can look at earlier lectures I gave, for example. So these are some lectures I gave here. And there's some lectures at GGI. And there's a new paper that's discussing these twister results. So there's no review of that, but hopefully this paper is readable. And the multi-loop amplitudes, the most recent results, are by Humberto Gomez and Carlos Mafa. So this is their three-loop paper, which is OK. So if you can't see something I wrote from writing too small, just please stop me and tell me to write bigger. So is everything OK up to now? Any questions? OK, so motivation. So as you will hear, certainly from Ashok, the usual description of the super string uses the RNS formulas, Ramon Nevers-Schwarz. So Ramon Nevers-Schwarz's formalism has the advantage that it's a very simple idea. You extend the bosonic string variables to spinning string variables by extending the conformal invariance, or the reparameterization invariance, to worldsheet super conformal invariance, or worldsheet super reparameterization invariance by introducing these grassman coordinates, which I'll call cap and capobar. So this is, of course, a super field. And if you expand it out, you get, of course, bosonic and fermionic degrees of freedom. So these are commuting, and these are anti-commuting. So I'll always use fermionic to mean anti-commuting. Some people use fermionic to mean spinorial. I don't use that language. So this is, of course, a spacetime vector. So although it's anti-commuting, it's a fermion to spacetime vector. This is an auxiliary field, which the equation of motion is that it's 0. So maybe you're not used to seeing that. So psi m is a worldsheet spinner. So this has spin plus a half. This has spin minus a half. So it has half-integer spin as a worldsheet variable. So psi m psi bar. But they're, of course, spacetime vectors. Now, if you think about spin statistics, it's natural to have spinorial. So that's fine. It's a worldsheet spinner. It has the normal statistics as a worldsheet variable. But it has the opposite spin statistics for a spacetime variable. So what this means is the worldsheet properties act very simply. They just act by worldsheet supersymmetry. They mix x and psi. But under spacetime supersymmetry, it transforms in a complicated way. So the spacetime, I'm not going to go into detail, although I should probably will go into some detail about the spacetime supersymmetry generator. If he doesn't, I'll do it later. You have to bosonize these fields. So it acts in a nonlinear way, just sketching how it looks. You have to bosonize the beta-gamma ghosts, which are the worldsheet ghosts for this worldsheet supersymmetry. And you also have to bosonize the psi. So this is some kind of spin field. It transforms as a spacetime spinner. That's why I've given this alpha index. So m equals 0 to 9 is a vector index. And alpha equals 1 to 16 is a spinner index. So this would be a Majorana vile spinner, depending on the choices of plus and minuses here. Now the algebra here is not quite the supersymmetry algebra. This turns out to be related to the translation generator by picture changing. So it's times some other operator. Let's call it y. Picture-lowering operator. Now I'm not going to go into detail on this, but you can see that the spacetime supersymmetry transformations are complicated. What this means is that it's complicated, for example, to compute scattering amplitudes involving external fermions or external states which carry spacetime spinner indices. So anything that carries spacetime vector indices is easy to describe. But anything which carries spacetime spinner indices is going to be complicated to describe. So for example, using this formalism up to now, what has been computed is 4.2-loop amplitudes. So this is Do-Kun-Fong. But only with external, never short, or only with external bosons. The technology for computing with external fermions, well, I'm not sure if it's a technical problem or a conceptual problem. It hasn't been worked out yet. Furthermore, it's unknown how to describe Ramon-Ramon backgrounds. Now, it might be possible tomorrow that somebody will figure out how to do this, but up to now it's unknown. And these are, of course, crucial for ADS-CFT. And the problem is essentially that the Ramon states are complicated in the same way as the spacetime supersymmetry generator is complicated. Furthermore, it's difficult to verify finite-ness properties or non-renormalization theorems. And the reason is simple. It's because one needs to sum over spin structures. So before summing over spin structures, the amplitudes are not spacetime supersymmetric. And, of course, these finite-ness properties depend crucially on spacetime supersymmetry. Finally, there's a question which is, if you want to compute the amplitude, not just the momentum dependence of the amplitude, but the overall factor multiplying the amplitude, it's unknown in the RNS how to compute the overall factor. So for a genus greater than one. Now this coefficient is important if you want to test certain duality conjectures. The reason in RNS it's unknown how to compute this is because when you work in the RNS formalism, you have BC, you have beta-gamma goats, you have these size, they all have different conformal weights. And what happens is the determinants that you get from doing the partition function over these fields of different conformal weights, they, of course, enter into the partition function. And it's not clear how to compare them. Essentially, you need different regularizations for each determinant and it's not known how to compute that overall coefficient in the RNS form. Okay, so these are, of course, the main advantage of RNS is this world-sheet supersymmetry. We can describe many different kinds of backgrounds. But the difficult features, as I said, because as soon as you describe things with spacetime spinner indices, the amplitude become, the formalism becomes complicated to deal with. Can people see down here if I write here? Yes? After I did it. Yes? So far not. So yes, but if you, so if you can use uniterity, of course, to try to fix this. So Doquin-Fong showed how to do this for two loop. It's not obvious how to do that for the three loop, for example. At least nobody has shown how to get that coefficient from uniterity. But in any case, in using pure spinner form, of course, uniterity is not manifest in any of these formalisms. Uniterity is only manifest in light cone gate. Now in the pure spinner form, you can directly compute it. So you can just check the two loop. Of course, if it, a two loop, if it gave the wrong answer, it means that uniterity is somehow violating. The formalism is wrong. But actually Marfa and Gomez computed the three loop and showed that it's consistent with duality. So, sorry, you can't see down there, is that right? Okay, so let me, okay. So the summary for our NS is that if we're looking at, for example, the open string, there are four different sectors of the super string. We have the sector called GSO plus, which contains, for example, the vector. Let's do the open string. So we have open string, we have the tachyon, we have the masses vector. And then we also have the Ramon states of different chiralities and also all the masses states. So the GSO plus sector is the one containing, for example, the masses vector. The GSO minus sector is the one containing the tachyon. Then we also have the Niver-Schwarz and the Ramon sector. So we have four different sectors for the, for the super string in the open string case. If we do a closed string, we get four times four, 16. Okay, so here's the vector, here's the tachyon. Of course, what one can also have, so this is the vector, this is the tachyon here. They're in the Niver-Schwarz sector. In the Ramon sector, we can have GSO plus, which would be like Majorana vial, and here would be Majorana antiviral. So just these are some examples of states in these different sectors. The Ramon formula, the RNS formula is good for describing things in this Niver-Schwarz sector, either GSO plus or GSO minus. It's good for describing tachons, it's good for describing vectors. Good means it's simple. I don't mean, of course, it's good in the sense that tachyons are objects you want to get rid of. I just mean that in the RNS formula, it's easy to handle them. Whereas in the Ramon sector, either GSO plus or GSO minus, RNS is not the way to go, okay? It's messy. Now what we'll see is that there's another description of the string using either Green-Schwarz or pure spinner formalism, in which, so if RNS is blue and Green-Schwarz is green, RNS is good in the Niver-Schwarz GSO plus and GSO minus. Green-Schwarz is good in the GSO plus Niver-Schwarz and also GSO plus Ramon, okay? Whereas it's not good in this GSO minus either Niver-Schwarz or Ramon sector. Okay, so this is the difference between the two formalisms. Essentially, the formalism is supposed to be equivalent, of course. The amplitude is supposed to agree for anything you compute. But the computations are much simpler using Green-Schwarz or pure spinners. In these two sectors, whereas RNS is better for these. So for example, we can describe curved backgrounds easily in RNS with vectors or tachyons. In Green-Schwarz or pure spinner, we can describe curved backgrounds easily in GSO plus Niver-Schwarz or Ramon backgrounds. Okay, so this is an important difference to remember. And of course, if we want to describe space-time supersymmetric theories, Green-Schwarz, pure spinner is much better because we want to describe these sectors. In general, we want to avoid the GSO minus sector. So, okay, so that's the main difference between the RNS and the space-time supersymmetric. Yes, but it's just as messy as describing Ramon sector in, so you have anti-periodic theaters, then you have to have spin fields in order to construct the GSO minus sector. Okay, are there any other questions? Okay, so the next thing I'm going to discuss is the motivation for doing this pure spinner or Green-Schwarz. So everything I write down here should be in the notes. So you don't have to copy, but at least try to ask questions. Okay, unlike the RNS formalism, Green-Schwarz or pure spinner formalism, so I'll use PS for pure spinner, space-time supersymmetry has now manifest. The way to do that is that instead of starting with a world-sheet superfield, now you introduce XM and fermionic space-time spinner variables. And these transform in the usual way under space-time supersymmetry, so. Okay, so now is a good time to introduce notation. So my gamma matrices, M is always zero to nine, alpha's one to 16. These matrices here will be symmetric in alpha and beta. And they're related to the 32 by 32 matrices in this way. So alpha and beta can either be down or up. So if something has an index up like theta alpha, it's called Myron vial, or more precisely vial. Whereas if it has a down index, so let's, this would be called the antivial. So you can see gamma matrix with two up indices, it takes something antivial to vial, and something with two down indices takes vial to antivial. So of course the gamma matrices change the chirality, and this would be a 32 by 32 gamma matrix. So in four-dimensional notation, this would be what was usually called the gamma matrices, and these would be the Pauli matrices. So this is of course in a certain representation. I'm only going to use this representation. So of course the usual gamma matrix relation, gamma M, gamma N equals two A to MN. This translates into this language here, gamma M alpha beta, gamma N beta gamma. If you symmetrize in M and N, it gives you two delta alpha gamma, okay? So you always, you can, there's no metric which raises in lower indices because these are different representations of SO91, yes? Say it louder please. Delta of X is minus one half epsilon. Delta theta is epsilon? No. So supersymmetry, so in four dimensions, if you remember Wesson-Bagger, so the supersymmetry transformation is of this type. D d theta alpha plus, I guess minus one half gamma M theta alpha d dx M. So this is just the action of epsilon alpha q alpha. So epsilon is the Grassmann parameter associated with the spacetime supersymmetry in this direction. Okay, so just to say, what you're probably thinking of is the RNS, World Sheet Supersymmetry Transformation. So in RNS, the supersymmetry transformation of World Sheet is delta X M. In this case, epsilon is a spacetime scalar. So it's just epsilon psi M plus epsilon psi bar M. And delta psi is equal epsilon d dz of XM. So here, yes, psi transforms into X. But this is the World Sheet Supersymmetry. This is not spacetime supersymmetry. Okay, it's a good question because these are the best kinds of questions because this is a question that probably half of you have but somebody has to ask it, okay? So are there any other questions? Okay, so this is the spacetime supersymmetry generator and as you can see q alpha with q beta using the anti-commutations of theta and d d theta. It's easy to see this is equal to minus 1 half d dx of gamma M. Sorry, minus, yeah, I guess that's right. So this is the, no, there's no one. Because you get it twice. Okay, so this is the usual anti-commutator two spacetime supersymmetries gives you a translation. Okay, so this is the gamma matrix relation. There's another identity which is useful to know. These are the things you know just by reading about it. It's not easy to prove, but okay. Of course, by writing explicit representations of these gamma matrices, you can prove this. If you symmetrize in any three indices here in 10 dimensions, this turns out to be zero. So this is just for d equals 10. For those that are interested, this is related to division algebras. So this is true in three, four, six, in 10 dimensions which is related to the real complex quaternionic octonionic division algebras. Okay, so these are identities which will be useful to know. Yes, thank you. Okay, so there any questions about this? For those that don't know, of course you can do fields. You can decompose any form constructed from vector indices in terms of these gamma matrices. So gamma MNP turns out to be anti-symmetric and alpha beta. So any object which is anti-symmetric in the spinner indices can be decomposed in terms of a three form. And any object which is symmetric in its spinner indices or by spinner can be decomposed in terms of a one form. And a five form. This five form is self-dual. Okay, so this is a notation which we'll use throughout the lectures. Any questions on the notation? Okay, so this is the spacetime supersymmetry. Of course, the action will be manifesting variant under this. It turns out that the Green-Schwarz formalism, although it's much older than the pure spinner formalism, it has only been quantized in Lycone gauge which makes life complicated if you want to compute scattering amplitude. So Lorentz covariance has not manifest. And of course, it also makes it difficult to describe curved backgrounds. So up to now, this has only been used to compute tree level and one loop five point ampoule. So Green and Schwarz computed the tree level four point and one loop four point and I don't remember but it's been extended for the tree level five point and one loop five point. Now of course, you can do these five point amplitudes for any external states. You're not restricted to external bosons. The amplitudes treat the bosons in fermions the same way. In pure spinner formulas, which we'll see later, you can quantize covariantly. So all the symmetries are manifest which has made it useful for computing multi-loop amplitude. Of course, both of these formulas can be used to describe Ramon backgrounds. In pure spinner, you can covariantly quantize these backgrounds, so that's an advantage. Finite properties are easy to verify essentially because you don't have to do the sum of spin structures, the space-time supersymmetry is manifest. And furthermore, one can explicitly compute for example, this overall coefficient essentially because all the determinants cancel. It's something like a topological string in that sense. So as I already mentioned, Mafer and Gomez, Gomez and Mafer, computed the three-loop four point of course for any external states, any external massless states and checked the estuality conjecture. So there's an estuality conjecture for this amplitude. It's a D to the sixth star to the fourth term and they computed this coefficient. That coefficient is related to the tree amplitude coefficient of that term by estuality. Okay, so that's an impressive computation. Now up to now, where these formalisms come from has been a bit of a mystery. Of course, Green-Schwarz just presented this, first they presented the formalism in light-cone gauge. Light-cone gauge is a very simple formalism, we'll see that later. Coverently, it's a bit more complicated. It's non-linear even in a flat background, but they showed that you can gauge fixed to light-cone gauge so they convinced everybody the formalism was correct. But as I already mentioned, people haven't been able to covertly quantize it and we'll see a bit later why. The pure spin of formalism can be quantized covertly but it's only written down in conformal gauge, at least up to now. So it involves a BRST operator in conformal gauge which is good enough to compute the amplitudes. But the question is where does this BRST operator come from? So what is the symmetry that this BRST operator is gauge fixing? So that's what we'll see in the following. It will turn out that it's gauge fixing a twister-like symmetry. So the generator of this symmetry is going to be something like P slash lambda equals zero. This is a twister constraint. I'll explain later why. And it will turn out that the fermionic variables here which are world sheet, they're space-time spinners. So this is of course, as you want, because it's fermionic, but it's a world sheet scalar which is surprising. Just like in the INS, it was surprising it was a space-time vector. Now we'll turn out that when you start with this approach here, this twister constraint, it will turn out that the thetas is the Fadea Popov ghosts for these constraints. So the fact that it's a world sheet scalar is now explained from the fact that it's from the world sheet point of view, it's a ghost. It's not a matter variable. So that's a new interpretation of this Green-Schwarz formula. And what I'll show next, well, after I describe these super particles, I'll show how to get these formalisms as two different gauge-fixed versions of this formalism with the twister-like constraint. Okay, so that's the motivation. So any questions before I start with the formalism? So as I said, the whole point of this is to interact. So please ask questions, otherwise, yes. Good, okay, good question. Thank you. Yeah, so the question is why we only have forms here of odd dimension. We don't have any forms of even dimension. So as I mentioned here, a gamma matrix, which is a one form, it either raises indices or lower indices. So indices of, so objects which have indices of the same chirality, they will only involve, obviously, because gamma matrices have either up or down an odd number of these. So it can be either be gamma m, gamma mnp, gamma mnpqr, or you could go on to seven forms, but the seven form is dual to this, et cetera. Now if we have something with an up index and a down index, then it can be expressed in terms of things with even indices. So for example, this can be expressed in terms of delta alpha beta, something with two indices, which would have one up and one down. Or something with four indices. So if you want to write a form with an even number of indices, or a by spinner, which would be a by spinner with one up and one down. So this is in 10 dimensions, of course, in different dimensions, things are different, but in 10 dimensions, this is how it works. Okay, these are excellent questions. Any other questions? Okay, so the next thing I'm going to do is give you an introduction to first, the green shorts, super particle, and the pure spinner super particle. So obviously there's no point in doing the string if you don't understand the particles. So let me start with the green shorts. So this is going to describe the mass of states of the open string, which is, of course, 10 dimensional super Yang-Mills. One can ask what happens if you work in lower dimensions, and I don't want to go into details, but the answer is not so clear. If there are questions, I can, of course, go into detail. So the action is, of course, going to be invariant under the spacetime supersymmetry, the one that I just erased. And it's, because it's a super particle, it's just an integral over tau.  So E would impose, this is the, you could think of this as the one-dimensional virbine, or just the Lagrange multiplier, which imposes the constraint that it's a massless. Of course, if you want it too massive, you just put in a minus M squared, but we're going to do the massless case.  No, I think that's right. If mass is zero, of course, it doesn't make sense. So since we're only considering the massless case, we're going to use the first-order form. And now this is not spacetime supersymmetric, because if you remember, spacetime supersymmetric transformations are delta theta equals epsilon L. So epsilon is a global parameter, does not depend on tau. Now to make this spacetime supersymmetric, it's easy just to add this term. So of course, dot just means g d tau, okay? It's easy to show that this combination is invariant under this transformation if epsilon is constant. And as I showed to you earlier, this transformation, if you anticommuniculate itself, it generates a translation. So q alpha is d d theta alpha. Now there's an additional symmetry of this action which was called kappa symmetry. It was first found by Warren Siegel, which is a local symmetry. So it's a gauge symmetry, but it's fermionic and it has the following form. So you introduce a fermionic parameter kappa, which depends on tau. Sorry, this should be another thing. And you'd find delta xm. So delta theta is just this thing here. Now if you do this transformation, it's easy to see that this term here, let's call this term pi m. So this object is spacetime supersymmetric. It's easy to see that delta pi m is equal to, I have to do the computation, sorry. So it's going to be equal to kappa p slash, I did it correct, let's see. I will do it on the other side. So you might think there's a d d tau acting on kappa, but that cancels from the d d tau acting on x. What that means is that because p squared, p slash p slash is of course equal to p squared, that you have to shift delta e in order to cancel the contribution. So the shift to delta e is just equal to two. Okay, so this is a local symmetry which is called kappa symmetry, any question? So of course local symmetries are implied that you have some generator, first class constraints. And to find the first class constraint, let's look at the canonical momentum to theta. So this is defined in the usual way by taking the derivative of the Lagrangian with respect to theta dot. So let's call that small p. So capital P is of course the canonical momentum for x. So the canonical momentum for theta, if we do this computation is going to be equal to minus one half p m. So it's not independent of theta, which means there's a constraint. So if we define d alpha to be equal to p alpha plus, this is a constraint. So in Dirac's language, one needs to impose this constraint on the wave function. Now of course one has to figure out if this constraint is first class or second class. And if you use the canonical commutation relations that p alpha with theta beta is equal to delta alpha beta, then it's easy to compute that d alpha with d beta is equal to gamma m alpha beta p m just because of the anti commutator here. p m is not a constraint, which means that d alpha is part second class. However p squared equals zero is a constraint. So although p m is not a constraint, part of p m is. Now when you do the computation, you find that d alpha, it splits up into eight first class constraints and eight second class constraints. In order to covariantly quantize, one has to figure out what to do with these second class constraints. Second class constraints, usually you don't know how to quantize using BRST method. But what you can do is quantize in light cone gauge. So covariant quantization is a problem. Of course, if you don't know how to covariant quantize, you don't know what the goals are. But one can't quantize in light cone gauge. So that's what I'll describe. So in light cone gauge, which is actually more properly called semi light cone gauge, you use this Kappa symmetry. This is a local symmetry to gauge fix half of the theta is to zero. So you can do that because you have these eight first class constraints. So you have eight local symmetries. So you gauge gamma plus theta, which has eight independent components. Gamma plus is of course equal to, gamma minus is equal to gamma zero plus or minus gamma nine. Furthermore, it's convenient to break SO8 down to U4. You don't have to do this, but it makes it easier to analyze the structure. So what happens is theta alpha has 16 components.  So gamma, this one we're going to set to zero. This one we're going to split up further into U4. So under U4, this SO8 spinner splits up into a four and four bar. So I'll call it theta J and theta J bar equals one to four. So broken SO9 one all the way down to U4. And now we're going to rescale theta J bar. We're going to define this to be one over P plus eta. When you do that, this action, so of course we still have this term here, but this term is going to only contribute when this P is in the plus direction.  That's the only contribution just because you gauge these theta's away. This is equal to theta plus A dot theta A dot, which now I can write in terms of these J and J bar and absorbing the P plus into the eta. This is equal to theta J bar theta J. So this part is of course the same as before. Okay, so this part I'm going to replace by this. Okay, so now it's easy to quantize because we just have these three fields. So the wave function of course has to satisfy P squared equals zero from this constraint. So the wave function is going to depend on X and it will depend on, the theta's and eta's are of course conjugate. So it either depends on theta's or eta's, but not both. Just like here, it either depends on X's and P's, but not both. So if we're working in the theta space, it's a function of theta J. And now you can of course expand it just because these are fermionic variables. So it has a single component here, then it has a term proportional to one theta, then it has a term proportional to two theta's, has a term with three theta's, and a term with fourth theta. So it has 16 terms, eta bosonic and eta fermionic. And these A plus, A J K, A minus, are just the usual eight components of the on-shell components of the gluon in Lycone gauge. So this is a six because it's anti-symmetric in J and K. And of course the C J and C J bar are the two components of the gluino. Okay, so this is the quantization of the Green-Schwarz super particle in Lycone gauge. Of course it's not covariant. I've broken it down to U4. Okay, any questions? Yes, please. One second, please. Here, eight, eight. Okay, very good. Okay, so p squared equals zero implies that, let's choose a reference frame just to simplify my notation. So let's suppose the momentum is in the p plus direction. Okay, so the algebra here is d with d here is equal to p. So if p is only non-zero in the p plus direction, then you have d alpha with d beta is equal to gamma plus alpha beta p plus. So I have to tell you what this gamma matrix is. This gamma matrix, let me just finish this. The gamma matrix turns out to be, it has 16, it's a 16 by 16 matrix, but it turns out that half of these components, it only has a non-zero component in this component here. So it's gamma plus a dot b dot. So all of these other corners are zero. This is an eight by eight matrix. So that's why there are only eight second class constraints. Now, of course, this was assumed that p plus was the only non-zero component. Of course, if I do a Lorentz transformation, that doesn't change the rank of the matrix. Okay, there was another question? Same question. Okay, any other questions? Yes? So Kennaut is too strong. So this was, of course, developed in the 80s and the covariant green Schwartz action was written in the early 90s. So for about 10 years, people struggled with how to write this, how to covariantly quantize this. Okay, so the main exercise was to convert these second class constraints into first class constraints. So once you can convert these second class into first class, if you can write the first class theory in a covariant way, then you can use your usual BRST method. So there were many attempts for the super particle, a few that succeeded, but none of these methods for the super particle extended for the string. So of course, for the string, there's a similar situation. You have eight first and eight second class, but the variables here are more complicated. So none of the methods which were successfully used for the super particle involving a different set of ghosts for ghosts or various methods, I shouldn't say there was one method which was generalized to the string using a different set of ghosts for ghosts by Siegel and Lee, Lee and Siegel. But it was so complicated that they couldn't compute. They computed some amplitude, but not many. So I can't say there are no methods to covariantly quantize, but I think it's fair to say there are no good methods to covariantly quantize. Okay, so that's right. So we're doing the super particle. So the super particle, of course, if it's described just at the free level, so free just means that it's not interacting, then it just describes super Maxwell. So it's just U1, so these are just linearized fields. If you want, you can introduce champatin factors and have it start to interact. Okay, now for the string, it's completely natural to do that, and the champatin factors you put at the end of the string and open string, of course, we can describe any gauge. Up to anomalies, we can describe any gauge group. And there are anomalies, I shouldn't say any. There are conditions on the gauge group in string theory. For the super particle, you can put in champatin factors, but describing interacting super particle is another story that I don't want to get into. So at the moment, just consider it to be super Maxwell. But when we do the string, of course it will generalize to super angles. But there are no conditions for the super particle. In principle, if I'm looking at the linearized theory, of course super Maxwell and super Yang-Mills are completely the same. You just add multiple copies of super Maxwell and you get super Yang-Mills. Other questions? Okay, so the pure spinner form is, so let me just spend, I'll just write down Lagrangian and then I'll stop. So the Lagrangian for the pure spinner is going to be start out similar, P and X. But instead of writing down in action just in terms of P, X and theta, we're going to introduce a conjugate momentum for theta just like we have for X. So P alpha will be an independent degree of freedom. So you go first to order a form. And then we're going to introduce some ghosts. So we're not going to try to write down the world line reparameterization invariant action. We'll do that later today. We're just going to write down what we call the gauge fixed action. So you introduce an additional variable, lambda w. And the idea is that this action is supposed to describe super Yang-Mills in a covariant way. In order to do that, you need a BRST operator. So I'm just going to save in two minutes and then this afternoon I'll explain this in more detail. So this is of course equal to D alpha, the same D alpha that we had before. But now D alpha is not zero because P alpha is an independent variable. Doesn't satisfy direct constraint. So in some sense, this is what you might try to construct if somebody gave you green schwarz. It's constraint times ghost. That's the BRST operator. But of course the constraint is not first class. So what you find is a Q squared instead of being zero is equal to lambda gamma M lambda times Pm, right? Because I'm using this constraint, this relation here. In order to make Q squared zero, this variable here has to be constrained. So the constraint will be lambda gamma lambda equals zero. And this is what carton called a pure spinner in D. Okay, so this is the answer. And this afternoon I'll explain where this answer comes from. Okay, so I'll stop there for questions.


Okay good morning everyone and thank you for joining us today. My name is Kimberley and I am here with my colleague Hobie. Now he is from the RTA's web services project team. Hi Hobie. Hi Kimberley, hello everyone as Kimberley said I am from the project team and I'm excited to share what we have been working on. Awesome so today's webinar is part one of our part two series all about the RTA web services for boundary funds. Today we are going to introduce you to the RTA's new boundary fund fast track process and we also will demonstrate how you'll be able to update your details online through the web services. The most exciting topic covered today is the boundary fund fast track. It is a new process designed to replicate the current process of downloading and printing your forms and getting everyone involved to sign it. Whether that be sitting around the kitchen table together or scanning and emailing it to each other for signatures. The fast track is the simple digital way for everyone to submit an agreed boundary fund and can be completed in as little as a few minutes. We will also provide you an update on existing RTA web services and other services and the best part is you will have a sneak peek of our new web services launching early December. We have allowed four question and answers at the end of this session today. Now you will notice and I have seen some questions coming through that the questions will be open during the webinar and I'll also be launching some polls throughout also. Now in terms of the questions we will endeavour to answer as many as possible today and we do get a large volume of questions. If your question isn't answered during this webinar please visit our website to have a look at our news section as you will find FAQs, webinars and other information. The RTA values the questions will be back that we receive. You can also call or email the RTA if you have specific questions on 1300 366 301. Brilliant okay I reckon we launch a poll. Toby what do you think? Let's do it. I really am interested to know which groups in the rental sector there are out there today listening in. So I've launched that poll you should see that poll up on your screen. It's always good to give us a little bit of an idea in terms of who's out there and that helps us best tailor our webinar today. Okay brilliant I'll close that poll off now. Thank you all for responding. Just looking at those figures there. It looks like the bulk of our attendees today is the property managers or agents and we also have hello out there to landlords and other members. That's right. Brilliant okay we will move on now and just provide you with a little bit of an update on the Bond Launchment web service. Now the RTA Bond Launchment web service was successfully launched in June. Toby can you tell us a little bit about what the uptake has been like? It's been really good Kimberley. Thousands of customers have transitioned to the new service with around over a third of all bonds currently being watched online through web services. Wow okay great all right well let's move into the new web service as mentioned in early December the RTA is launching web services for bond refunds, bond disputes and updating customer details. Now the suite of digital services is being released together. This is because the services are commonly used together at the end of a tenancy. Now web services will offer the 100% digital fast-track option as I mentioned for agreed bond refunds. That's right and if the bond is reduced during the tenancy for example for a rent reduction the new online refund service caters for this. I will point this out during our sneak peek. Okay now following the launch of the successful launch of digital launchments the RTA as I mentioned will be offering bond refunds through our web service. I have a video here today it's of Sam Pangelli the director of RTA customer experience talking a little bit about the development of the web services. So now we're working on refunds so we have decided for the next release that we're going to release a suite of forms together so the reason why we've done that is we're conscious that at the end of a tenancy there can be multiple touch points with the RTA. It can involve multiple processes and filling out multiple forms and we wanted to provide an experience that can be a bit more seamless and an entirely digital so 100% end-to-end strategy device. So we're releasing together the bond refund form, the bond dispute form and update your details form because that's typically what customers look to do with SMPM at the tenancy. Okay excellent now in just a moment we will demonstrate actually how to submit that digital refund and just to let you know that the video the digital refund will pick up from the RTA refund form. Looking there is screen you will see all of our web services that will be accessed from the RTA website so always going through to the RTA website to access our services. You can see there at the moment we know we have the lodger bond service and after the launch we'll have the refunder bond and update your details. So launching from our webpage you'll then be asked to read and accept the RTA's terms and conditions and once you've done that you'll be directed to the QGov website you can see that down there in the low lower right hand corner of your screen. Now this is where you'll be asked to either login or register and once you have done that you are taken through to the RTA digital form to complete. Now don't forget you can find out more on how to register with QGov on our website or call our contact centre. Also too it is important to note that you do need a unique email account to create a QGov login and to access the RTA web services. Now this is to ensure I'm assuming Hoby the security and privacy of all online transactions. That's absolutely right yes and our data from our earlier poll shows that our largest group of attendees today are managing parties. So today we will demonstrate the digital refund submission from a managing parties perspective. Okay let's play that video. So starting off here you'll have come from the QGov website and onto the RTA website here. You'll elect the bond refund option. It's something that you can go continue on from a previous form you were going with but on this one we're going to start a new form. There's a helpful hint explaining the options here. You'll select what your relationship is to the bond then next screen display some information about your QGov account. You can elect someone else if you're not the contact person for this refund and enter in their details. For this example we'll put in yourself so you can also put in a phone number. You'll continue on. Here you'll put in the details to do with the relevant bond. So you'll put in the bond number as well it'll last for the RTA ID for the bond. You can enter that in. Okay then continue on. It'll return some information about the bond you're attempting to refund. You'll confirm that also like another one. Then you'll identify which type of refund you're wanting to do. There's some information and helpful hint explaining the two options we provide. Much like our pay-per-form you'll need to put in the date for when the notice of any the tenancy has been issued. If there hasn't been a notice ending the tenancy you can select no and it'll provide a box there where you can put in when the tenant left or vacated the property. For this example we'll just use the notice continue on. Here it'll ask you if you discussed the refund with the tenant of the property. The RTA encourages parties to discuss the bond refund process. It's just some more information about that. You can select no it'll still let you on but in this example we'll say yes. Here you can select if you want to claim any of the bond. So for this example we do. Here is a list of the claims that you can make. So we have a list of all the possibilities that you can claim for and then on top of that you'll put in some claim amounts that you wish to claim from the bond. You can also add another claim reason in from the same drop-down box. You can also remove one you've previously entered and down the bottom there'll be a breakdown of the claim you're wishing to make on the bond. As well some information on how you can get paid. Once confirmed you'll continue on to the refund allocation page. This is where if it's more than one tenant you can allocate different amounts of different parties as well. If there's another party that you wish to allocate money to some more helpful hints about what a third party is you can allocate money to them. Once confirmed continue on then there's a summary page so we do suggest that you do confirm this information and just double check make sure that everything you're providing is the correct amounts. If you have made a mistake on here you can then navigate back to the previous screens by clicking on the titles on the left here. So you can confirm these details once complete come back to the summary and then you can then submit. Here it will confirm that you have submitted your bond refund request and there's some more information about the process as well. So you can print your summary or give feedback on the form or submit another form as well. Excellent thank you Hoby. Now the diagram you can see here shows where you are in the process once the form has been submitted. You may have noticed in the video that diagram and the diagram does display at each stage of the digital refund process and we also include that diagram on all of your email notifications. So this is just for ease of keeping track of where you are in the bond refund process. Hoby I noticed you accessing the information along the way there. I think you mentioned helpful hints. Yes Kimberly there are helpful hints on all of our forms to assist with completing the web services. Okay and we did see that from a managing party or an agency perspective their organization. Are there any key differences if I was a tenant submitting the form? The only differences between the forms are the wordings between the forms but the process and the path of the form is the same. Okay so more words tailored more to the tenants. Absolutely that's right yeah. Excellent okay now after the bond refund is submitted you will notice in the diagram the new fast track. We have a video of Sam speaking again further around the concept which is new to the RTA. So fast track is a process that we came up with to replicate digital agreement. I guess we had a couple of key design challenges in converting the paper form to a digital form. One of them was that two-thirds of the forms that we currently receive completely agreed. So when we receive them we can see that everyone signed that form they've talked about it and all we need to do is process that payment for them. How do we replicate that in a form that one person for this one person submits. So fast track is a solution that we've come up with that replicates everyone getting around the same table signing the paper form. So once that person submits the digital form to us we generate digital workflows to everybody else and it's their opportunity to say we've talked about this we agree you can proceed straight to payment. So we give them a small window of 48 hours to respond to that fast track. If we don't get a response or they tell us that it's the first they've heard of it they don't agree with it then the normal notice of claim process commences. Okay so Sam Pangelli they're talking about the exciting new fast track process. If you are having any difficulties hearing that video we are going to go through some more of the particulars now. As I said this is an exciting new process for the RTA. So really the process replicates where you and a tenant would have ordinarily jointly signed a refund form and have all agreed. Is that right Hobie? Yes and as Sam said that is over two-thirds of the bond refunds the RTA currently receives. Okay so the new fast track process will become the fastest and most convenient way to complete agreed refunds which is the largest portion of refunds. Yes that's right. Okay so what do we know fast track is a 100% digital end-to-end option to submit a refund agreement. There'll be no more chasing up signatures on a paper form if you choose this option and the RTA confirms the agreement. Now only one person submits the digital refund and the RTA requests the information from the other party so they'll no longer be chasing up bank account details for tenants example. That's right yes. Okay now the agreed bond refund can be processed in minutes now the fast track process is only open for 48 hours so that means if we do not receive all responses or if the refund is not agreed the usual notice of claim process will commence. Now this can be done in minutes. Can you run me through how this is possible Hobie? So the RTA notification goes out straight after the refund is submitted and if everyone accesses their emails and responds right away it's that easy. Okay all right so say for example currently managing parties and tenants all need to sign the paper refund now once they do that they can upload the signed refund. So for example if a signed refund form is uploaded on our website existing process there still needs to be time allowed for for RTA processing. Yes and if the refund form is posted there is postage timeframes plus RTA processing timeframes before the refund can be finalised. Okay so basically the existing process of an agreed refund form takes a number of days. That's right yes and and providing all of the information on the form is legible and not with missing information so this can delay the process even longer. So after the discussions are had up front about the boundary fund they decide who will submit the form and everyone else ready to receive their RTA email notification this process can be done in a matter of minutes. Okay great now we do have a video here for you on how easy it is to respond to a submitted refund. When another party submits the refund you will be notified immediately as Hobie said. Now you will receive an email now Hobie that email on my right contains a link that will take you directly to the web services page. Exactly we will show you now how easy it is to respond to the boundary fund and fast track to agreement. This video picks up from where you would have clicked the email link and have been directed to the RTA fast track web service. So you'll arrive on the RTA page here you'll enter in your organisation's RTA ID another helpful hint about that RTA ID. Your QGov details will be populated you can also add a phone number as well and here you'll have a breakdown of what the refund allocation is. You'll also be able to see the claim reasons and you'll also need to select if you wish to agree to fast track the refund. And then here's the summary page once again confirming the details like the other forms you'll be able to navigate back to previous screens if you wish to change any information. And then you'll be able to click submit if you've confirmed these details and then some information about the process will be on the screen. So then that's basically the fast track process. Excellent. Okay. Lots more helpful hints along the way I noticed. Now for all of you out there what do you need to remember if you're wanting to fast track an agreement. So you want to make sure you've had the discussion and ensure everyone agrees. Now also it is important to know your RTA ID and your bond number. Now a bit of a reminder the RTA recently emailed managing parties and tenants with their RTA ID and bond numbers. So if you haven't received a good idea just to check your junk mail or you can always find the RTA contact centre. Now it is important to decide who will submit the refund and exchange current email details. And the other is not submitting the form obviously being ready to access their RTA email notification. The faster the responses the faster the refund. Is there anything else maybe Hobie that they need to know? Remember the fast track option expires in two days. Everyone must respond and agree for the refund to be fast tracked. If a bond party chooses not to fast track the refund or does not respond the RTA will start a formal notice of claim process. That's all covered in our next webinar. The RTA will keep everyone updated along the process with email notifications. Okay so that wraps up the bond refund and the fast track. I might launch another poll now Hobie. Let's have a look here. Let's find out any other polls there. Okay it appears that poll's not working. We will would be interested to find out. We do have a survey at the end of today's webinar to find out how you found the bond refund and fast track process. And there will be an area there for you to make comments. But certainly interested to find out if you found that process easy to understand. Today obviously is an introduction and an overview of those processes. And more of those details can be found. Information can be found on our website after the launch. And we do have a trained web services help desk through our contact centre. They can actually walk you through each of the processes included including QGov. And walk you through those processes. So certainly and if you are seeking some more information on bond refunds or the fast track process that's a good idea of where to access that information. So if we assume that everybody agrees Hobie and everyone agrees they have responded to the fast track they've chosen to fast track their refund. What happens next? So the RTA automatically releases the payment when all responses are received and agreed. So tenants and less willers are prompted for their own mech account details during the fast track process. If we do not have account details the RTA will contact the individual. Pay should allow for weekends, public holidays and usual bank processing times when waiting to receive their money. Excellent. Okay so let's move on now to the other service in this suite of services we will be releasing in December updating your details. Now we know Hobie at the end of a tenancy. Our customers details are outdated especially when long-term tenancies are concerned. That's right yeah that's right. So the new digital update your details web services, streamlines processes and eliminates pay performs. And I'm assuming it proves the end of tenancy experience for everyone involved. Absolutely yeah. And as Sam mentioned earlier in the webinar it makes sense for us to couple updating your details with the release of the digital bond refunds. That's right. Now also pay performs just for you out there. Pay performs will continue to be accepted for our customers who do not have access to RTA web services. That's right. Now let's see it in action Hobie. We've got a video here. So this video is of an agent updating their details. Okay. So much like the other forms you'll arrive at the RTA page after going through QGov. You'll confirm what customer type you are. Some more helpful hints about those types. You'll identify that you're not a new organization, that you are a new one in this example.  As well for security purposes we'll ask for a bond number that you manage. So you'll enter that in. And then on to the verification code. So we'll send a verification code to the email for your organization. You'll then need to retrieve that code and put it into the box there. Once that's complete, you'll then be able to provide other information or update your details. So your email address, phone number, mobile number, address as well. You can update the physical address as well as the postal address or just one of them. And then your bank details. So you'll be able to update the bank details the RTA holds. And then you'll be able to just confirm what you've put in here. So once again we suggest that you thoroughly check these details before you do them. And if you need to update any details, go back to a previous screen and click the authorize these details being changed. That's it. Excellent. That looks fairly straightforward, Hobie. I guess it is important if you are a managing party to make sure when you're completing this service, you have access to that main agency email listed on the RTA records. Yes, that's full added security for your business to ensure that details can only be updated by those with permission. Okay, and is there anything else maybe that we need to know? So the author of the request will always be asked for an email address. You will only be asked to update the physical address if the address is different to the postal address we have on record. The new customers will use a service moving forward to before submitting a lodgement or starting to do business with us. Excellent. So certainly important checking those screens, making sure the information you have entered is great. That's right. Because our systems will be updated with that information if you submit that through. Okay, now what happens if you cannot access RTA web services or if, for example, your tenants cannot access web services? The RTA does encourage tenants, property owners, and managers to lodge rental bonds online and refunds when that is launched. As it is more secure, it is convenient and it is faster for all parties. But we do understand there are instances where our customers cannot access web services. So that might be they don't have a computer and they're unable to get assistance from family or friends or get down to a local library. Now paper forms are still available to download from the RTA website or you can order a form by phoning the RTA contact center on 1300 366311. And it is really important to note paper forms will continue to be accepted via post. That service is still available. This web services is just an added service for our customers out there who have told us that they're wanting to transact with us online. Okay, so RTA services update. So we have mentioned today the big news, RTA web services bond refunds we know is happening in December. It is important to look out for RTA information regarding this. Okay, the launch details and things like that will be coming out in the coming days. A reminder, the RTA will no longer print bulk forms and publications from the 1st of January 2020. Also too, with the launch of web services bond refunds, the bond refunds service will replace the existing upload facility for scanned paper refund forms from the 1st of February 2020. And also very exciting, there will be more web services in the pipeline next year. Now just a little bit of a summary on the web services for bond refunds. We've seen that it is today a fast, efficient and a secure way to do business with the RTA. Just a reminder out there, if you haven't registered for QGov, please do so. And we encourage you to encourage your tenants or your managing parties, landlords etc. to register also in readiness for the launch. Now it's also to remind you must have a unique email address. That's really important. And you must register for QGov to use the web services. Also web services process is run via RTA electronic notifications. So that could include your notice of claim or your notice of unresolved dispute or your acknowledgement of rental bond. So remember, some of these notifications are time sensitive. So it is really important to check your emails regularly. So that wraps up our sneak peek and add discussions around the bond refund web services and fast track. We might launch into some questions. Thank you so much for sending through your questions there. We've got a heap to cover, as I said. We will endeavour to get through these. Now if your questions haven't been answered through the webinar, don't forget to jump online. You can also watch this webinar again and view those sneak peeks again if you'd like to see those. All right. Let's take a bit of a look at these questions. Now in terms of QGov, a number of you have been asking about QGov, specifically why we're using QGov. Now it is a way to verify your signature digitally. Okay. Now it is a Queensland Government Service and it offers the opportunity to verify your signature as a substitute for your paper signature. And it also helps us keep your transactions online secure. You've also mentioned here we've had some questions around water for talent can't register for QGov. Now in terms of not being able to register for QGov, Hobie, certainly post is still an option, isn't it? Yeah, so that's a key thing we want to put here is that the post and the paper processes will still exist. We're not taking those processes away. We're just adding in new ones for those clients that wish to use those processes as well. For example, if you don't have access to QGov website, you'll be sent an email notifying you that a bond refund request has been lodged. If you are unable to access a QGov site to respond to this, you'll automatically be sent an email with an attached notice of claim form after 48 hours. So the normal process will continue. We're not changing that normal process. You can fill in this form and post it to the RTA and what we use is to process your refund. So much similar as what we currently do. And also too for international students out there, for example, registering for QGov does occur online. However, we do encourage international students to contact QGov because they may be able to submit forms of identification, not accepted online. Directly with QGov. So always contacting QGov for alternatives to that online registration process. Now, we've had some questions around printing your summary or your bond submission. I thought I did see a section there that said print my... That's right. So on all of the summary screens, after you've submitted from that summary screen, you'll be able to print a summary. So we recommend printing to PDF or saving an electronic copy of this summary rather than printing a hard copy to help reduce waste. If you're using an iOS or Apple device, we recommend using Safari as your preferred web browser, but all clients will be able to do that on that screen. Okay. A little bit more about the fast track here in terms of some of you have asked what happens if a party doesn't agree. Now that will be covered in next Thursday's webinar if you haven't registered, please do so. That's all about the dispute and notice of claim process. Now, if a party doesn't respond, for example, or the fast track period ends, hope I'm assuming situation normal. Absolutely. So it continues on to the same notice of claim process that we do. So it starts as soon as 15 minutes after the last party listed on the bond has responded. As per the legislative process, all parties have 14 days to respond to the notice of claim. Brilliant. Okay. So certainly parties disagreeing or parties who don't respond, we will not be doing anything and the notice of claim process will commence. Absolutely. That's right. Excellent. Okay. We've probably got time for one more question. Thank you so much, guys, for your questions here. And to anything else that we do get through, we will analyze and review and it will form part of our frequently asked questions section on our website. So thank you so much. Now, if you've submitted a digital form using the RTA web services and didn't receive your acknowledgement, please make sure that you check your spam or junk email box. Okay. So acknowledgements do go out once payment is received with the RTA, but certainly please check your spam or your junk email box. Or of course, give us a call on our contact center number on 1300 366311. We understand that those acknowledgements are important to you for your records and certainly we would look into this for you. Okay. All right. So thank you so much. We will need to wrap up today. Please stay on the line. Once I close the webinar, we do have a quick survey. And as I mentioned, your feedback is really important to us. So please stay on. I will close the webinar, which will then trigger a survey for yourselves before you close out. From on behalf of Poby and I, we do really appreciate your attendance today. Don't forget to register for part two webinar if you haven't already. Thank you so much again. Yeah. Thank you very much. Thanks guys. I will close the webinar now.


This is Coach Mack, color analyst for Titans Radio. Today we're going to go beneath the surface to look at Dean Pease's defense. They're created a big turnover against the Bills. This is third and sixth. Balls on the 34 yard lines, 10-40 left in the third quarter. What Dean Pease has deployed now. He's deployed a defense using six defensive backs. He's got one defensive lineman in the ball game and he's got four linebackers. He's deployed his linebackers across the front except for Jayon Brown who's the lone linebacker in the middle of the formation. You can see Rashon Evans is lined up as an interior pass rusher. Nobody has their hand on the ground. All the front people are in a two-point stance. This makes it very hard for Josh Allen, the second-year quarterback to be able to use Cypher. What's getting ready to come? He sends his back out in motion to the defensive left to get a man-zone declaration. Once Kenny Vicaro goes out there and covers him, he still doesn't know whether it's man or zone because of the multiple defensive personnel that Dean Pease has in the game. On the snap of the football, they fake as if they're going to rush forward.  Now they're in 500 or two-deep zone. This causes the quarterback to hitch, hold the ball. The zone coverings are trying to run a switch release on the right side of the Titans defense. As you see here on the outside, Gilbert does a nice job of running an inside rush. He runs what we call an ET game with Jarell Casey. Puts pressure on the quarterback. He's having to hold the football. He's not sure of what he's seen. Once he starts to scramble, everybody plasters their receiver. They start out in zone defense, but once they start to move and the quarterback starts to scramble, zone turns to man. You start to plaster your man, staying on your side of the field. Harold Landry does a nice job of spinning off, putting pressure on the quarterback, very aware not to hit and rough the quarterback, puts a hand up, does not allow Allen to follow through, and then Kevin Byrd, the all pro safety, he passes off one receiver to the zone, breaks inside of the throw, makes a tremendous, tremendous catch. Low throw, not only a great hand-eye coordination by Kevin Byrd, but it's a really nice job of plastering his receiver, following the quarterback's eyes, big turnover from the Titans defense.


Hi everybody, Joe for jashpeascasebreaks.com coming out to a 2019, 2020 Panini Contenders Optic Basketball 2 box. Pick your team number 104 with some money being given away if you follow the instructions right here. But first, the break. Big thanks to this group right here for making it happen. Thanks for picking your teams. And the last two boxes of this case already, of this inner case, already loaded up. So if you want to run this back, we definitely can. So we drew those X's on there so we know they're from the same inner case. So we'll go 1, 2, 3 for the top row, 4, 5, 6 for the bottom row. I'm going to use that die right there, 1, 2, 3 for the top row, 4, 5, 6 for the bottom row. 6, bottom row. So this, we'll say for break 105, which is on the side right now. Alright, now let's see what we got. If you're wondering, Joe, have we seen that guy? Or the guy playing on TV right now? John Moran? No, we have not. Not even a base card. Donovan Mitchell. When we dropped those 46 points, we got Ben Simmons, Red Ice, we got Devante Graham, Silver, and DeMar DeRozan, Red. All cards shift by the way, so you're going to get all those. There's Giannis right here, Pelicans falling to the, or Bucks falling to the Celtics today. So they'll regroup for game three. And we've got, oh nice, Pascal Siakam. Ink going to Raymond in Toronto, 29 out of 125, he's pretty good. Next box, Redemption on the bottom, I think they may be expired, but I don't know, we'll find out. We'll find out. There's Trey Young, Nikola Jokic, Tobias Harris, Malik Beasley, Ben Simmons, and the Redemption, Rookie Variations, Season Ticket Blue, A, D, Admiral, Admiral Schofield. It just expired very recently, March, late March, so you may still be able to redeem this. I hear a lot of stories where people, especially if it's that close, you can still scratch that off and send that in, blah, blah, blah, blah, and I'll still go through. Corey with the Wizards, he usually signs his cards, he's got kind of a cool penmanship. All right, well hey, that's that ladies and gentlemen. So again, nothing too crazy, maybe something crazy in those last two boxes over there. I'm Joe for jaskyscasebreaks.com. Let's give away some money before we put this break to bed, so we'll get some consolation prize here. Anthony, remember you have to buy an even number of teams, half of those teams become entries. Anthony bought six teams, that's three entries, Corey got four teams, that's two entries, David got two teams, that's an entry, Logan M got six teams, that's three entries, Nick Smith bought four teams, that's two entries, Patrick got two teams, that's an entry, Raymond got two teams, that's an entry, Suman got two teams, that's an entry, Victory We've got two teams. That's an actually, Logan, David, Corey, and Anthony. I think with 15 spots here, I think everyone did their part. Everyone got an even number of teams. Thank you. All right, new dice, new list, and it's gonna be the top four. We'll get $100 of break credit each. Top four after three, two and a one, three times. Good luck, everybody. One, two, and fingers crossed. Three, top four, victory. Raymond, Patrick, and Corey, $100 each. Go on your way. I'm Joe for jaspyscasebreaks.com. I'll see you next time for the next two box contenders optic basketball break. Bye-bye.


The presidency has expressed satisfaction with the standard of work done at a state-house clinic seeing that equipment are of international standard. The chief of staff to the president writes on a family by Javier Miller who stated these after touring the 21 billionaire presidential wing of the state-house hospital said when all the eyes are dotted and the teeth crossed the country would be proud to have such a clinic of high standard. Feuding questions from journalists after inspecting the facility being the first from the President Bola Tinnable-led administration by Javier Miller highlighted the advanced medical equipment including the state-of-the-art ART CARTH lab and UNICC app. Well, first of all, like you're right, there's been a lot of talk about this clinic, not just today, even when I was in the National Assembly as Speaker. So I thought, you know, I haven't been here a few months, let's have a look at it and see exactly what is going on. I have seen, I am very impressed and I'm sure you are as well because you went around with me. Well, this is a clinic like anywhere in the world you would find. This standard is very high, the equipment of world class, from my understanding this is some equipment that you wouldn't find in too many places all over the world. So as far as clinics go, in terms of equipment, in terms of what they can do, in terms of, I mean, I've just been lectured about kidney transplant now, from one of the best. Any cath lab? There's a cath lab that's world class and so many other things, there's an equipment that you could see. CT MRI. CT MRI. No, no, no, no. The one that guides you. CR. CR. You know, this is, it gladdens my heart that at least when we're appropriating money in the house of a Brazilian speaker, I can see where the money is going to. So it's for them to dot the I's and cross the T's and we'll finish in touches and I think, I mean, we'll be proud to say that we have a clinic, an international standard clinic like this one. Chairman of clinical services at the state house, Dr. Jane Ifetrucu clarified 30 facilities current status was skeletal and awaiting approval to be fully operational. Right now, the last administration stopped. Everything is in place, but they wanted this administration to drive the process. That was the language. So we've carried our principals along, so it's for them to give us a go ahead. What we have here is skeletal, just the way we were having the villa clinic. That's what we do here. But once they do the I's, we can't take decisions on our own. They give us a go ahead and we are good to go. We actually discouraged that and I can't speak now. I'm waiting for our principals, our bosses, to do that and then the PAMC could give us a directive and then you can do that. Everything is ready. Yes, yes, yes. The moment they say go? Yes, we're good to go. Thank you very much. Everything is on PAMC. Thank you.