Mark, you started your career off in Tennessee, spent a little time in Vegas, and now you're here in Atlanta. Michael 10, Michael to the 5, he'll move the pocket to the left, has an alley, turns the corner and hits the pylon, touchdown Atlanta. Tell me about the last couple months and what that journey has been like. Yeah, really for a couple years it was a good reset. When I left Tennessee I was pretty beat up, kind of mentally and physically. I'm excited to be here now, and I'm excited to be part of this team, this young team. Coach Smith, I think he's getting everybody going in the right direction, and I just can't wait for the season. Snap to Mariota, looks left, gonna throw in... 11 of the days that Keyes on a streak on the back line of the end zone, holes in the touchdown. Your coaches, you mentioned Coach Smith, you talk about changing the culture around here, and I know culture is big everywhere around the league, but in this culture, in this locker room, what do y'all want that culture to look like? A winning attitude, man. It takes it one day at a time, really. I think some people get so caught up in what's going on in the future, and maybe what they've done in the past. Art always talks about staying present, being in the moment. If we can do that and build one day after another, I think we're where we're at. You got some pretty big targets in the season. You got Cowpicks, Drake London, the new addition, the new rookie that you're going to take up under your wing. How does it feel to have those big targets, and how do you plan on using them? It makes my life easy. You know it, right? You get big targets like that, you don't got to be perfect. And I think as I'm watching these guys grow, I think it's pretty cool because they're learning to create separation. And with their frames, with their athletic ability, they can do a lot of things with the ball. They can do a lot of things, you can do a lot of things, being a dual-thread quarterback. Who are you going to use that ability to the best of your ability? How do you plan to attack defenses this year along with the passing game and the run game? Just creating advantages, like you said. I think it starts with being efficient as the quarterback, completing the ball, being the point guard. And then from there, sometimes you got to take it to the whole yourself. And I'm excited about that. I think we've got a good plan. And wherever I can be, whatever I can do to make this team work and make this offense run, I'm going to do. You're probably one of the fastest guys on the field when you step out there. Do you see this transition taking on the life of his own, and do you embrace being a dual-thread? Yeah, absolutely. And I think it creates advantages for you as an offense. It used to be where, you know, in the center, it's 10 on 11, really, because the quarterback's handing the ball off, you're not really doing much. But now you get an opportunity to play true 11 on 11 with the guy that can run. It makes it tough on defenses. For me, it's been fun to be a part of it.  And, you know, it's just cool to kind of see the evolution. Yeah, my coaches always say, when they play man coverage, they can cover everybody, but they can't cover everybody. Exactly, no doubt. Always remember that. I look around the locker room, I look at the practice, and I don't see a lot of familiar faces. And I look at some of the guys who've been here for a while, but you are among the leaders on this team now. It's not a plan. You have to embrace that role. And what is that going to look like for you? Do I feel good? Do you feel comfortable in that role now? Absolutely. And it comes on just being yourself. Right. You know, I think guys can relate to you a little bit better. I think people can catch on to kind of a fake, a fraud type of deal. So I just try to be myself, lead where I can. I do, I love communicating with the receivers, making sure they're all on the same page. And then just setting the standard. I think if you're out there and you're putting the extra work, you're doing the extra time, I think those guys kind of buy into that. I don't know why they might meet up. I'm not very good content. Hey, this is what it's about. Atlanta, the city of Atlanta has great culture.  What's some of your favorite places you done visited so far? Some of your favorite restaurants you done ate at? Yeah, we've been to Frankie's Steakhouse, which has been dope. We took the receivers there a few months back. Went down to Umi Sushi, a thing was called. That was great. Pretty good. You know how long you lie? I don't lie, being from an island in the middle of the Pacific. And then you come to a state that's pretty landlocked. That fish was solid. You wanted to be fresh. Yeah. It was fresh. But those two spots were good. At the end of this 2022 season, and you look back on it, what did you want the message to read, you know, from Marcus Mario on down on that roster? I think it comes down to you're going to find a group of guys that not only believe in each other, but got a winning attitude, man, that believe in what's being built here. There's going to be ups and downs. We know that. But it's being able to withstand those storms and dust yourself off and get ready for the next one. Because I think as a young team, you know, it can be pretty special. I'm glad you're here where you at now, bro. And I'm so excited to watch you this year. And I'm glad you're getting a second shot at it because I know what that really means. To have another chance to do it again and have a team that you call your own. So embrace it and I'll be rooting. I appreciate it. Thanks, man.


Hello, I'm Anne-Marie Burkle, Acting Chairman of the Consumer Product Safety Commission. Did you know that the two weeks ahead of the Super Bowl is one of the most popular times of the year to buy a new television? With so many new TVs, families need to know about a hidden home danger. Televisions can tip over and cause serious injuries and death. Here are the facts. About 60% of child tip-over deaths involve children ages two to five. In the time it takes to watch the Super Bowl, eight children will be rushed to the emergency room from a television or a furniture tip-over incident. And the force of a falling TV on a child is 10 times stronger than two NFL football players colliding at full speed. Think about that. The good news is that tip-over incidents can be prevented. Anchor TVs to the wall or to their stand using anti-tip devices. Brackets, braces and wall straps are inexpensive and easy to install, usually in just about five minutes. Recycle your older unused TVs and place TVs on a sturdy low base and push them back as far as possible, especially if anchoring is not possible. Avoid putting items that might tempt kids to climb, such as toys and remote controls on top of the TV. Remember, anchor it to keep your family safe.


Studying Romeo and Juliet. Here's how you can analyse Act 1, Scene 1. The discussion between two servants from the House of Capulet in Act 1, Scene 1, establishes a theme of hate. Here, the metaphor where Samson is talking about the House of Montague highlights the hatred that exists between the two families. This imperative sentence shows that the hatred between the Montagues and Capulets runs deep. The servants are about to pick a fight with the servants from the House of Montague. The servants from both houses begin to fight. However, Benvolio from the House of Montague stops the fight. The Caesura hair in part falls as well as this exclamatory sentence establishes Benvolio as a peacekeeper. Yet, Tybalt from the House of Capulet enters and we can see from this hyperbole that Tybalt is not a peacekeeper. Also, the repetition of the words hate foreshadows how Tybalt will disrupt the peace. A great fight then breaks out and the Ascendant's hair shows that the Prince of Verona is stopping this fight. The Prince is fed up of the fighting and hair that I am the pentameter in what he says heightens the dramatic tension. He says that they're not allowed to fight again.


really sorry because at 12.10 I have to go for something urgent we're gonna have an extra makeup class tomorrow at 11.30 in the mathematics seminar room okay so just for those who came late I'm today's gonna be very short class like half an hour class because I have to go for something urgent at 12.10 I'm sorry about this okay so but we're having a makeup class tomorrow in the mathematics seminar room okay so now let's let's move quickly okay so in the last class we derived Einstein's equations and this class we want to start using Einstein's equations okay so we want to start using Einstein's equations but before we start using it indeed these equations in detail which will be much of this class the first thing we're going to try to do is try to understand them the non-relativistic or the Newtonian limit of the Einstein equations okay so you remember that in the previous class we had checked that provided g00 is equal one plus two phi okay provided g00 is one plus two phi test particles in a background metric will in the appropriate limit test particles in a background metric will in the appropriate limit behave as if they are subjected to Newtonian potential phi okay and the appropriate limit was let me say it was of course that g is equal to one plus plus epsilon and h some degree of smallness in epsilon and we had also that velocities velocity squares were like one plus excellent so velocity squares were of the same order of smallness okay so velocity is like a measure of x distance by time distance okay so velocity squares was of the same order of smallness as the deviation of the metric from flat space and the way to see that those had to be of the same order was to note that in the Newtonian theory phi and v squared are often exchanged in ordinary motion so a planet that has only phi ball up here that has only phi at the top has v squared at the bottom but v squared and phi of the same order right so v squared and phi were of the same order this was the the Newtonian limit under under consideration okay so what we're interested now is in looking at what Einstein's equations become in this limit so we look at the limit in which g squared is one plus epsilon of epsilon times h and these squares are small now how do we precise the statement these squares okay the kind of thing that we want to say is that now v this is sort of like delta x by delta t the whole thing squared is okay so what what we're saying is that in the configurations that we're looking at time derivatives one of the things we're saying is that time derivatives are of order square root epsilon times space derivatives because d by dx is like one over a spatial distance d by dt is like one over a time distance so this will give us delta x by delta t is over epsilon squared it we get this okay so we're interested in the limit in which things are varying much faster in right but a derivative is one over delta x okay so this is one by delta t is over the square root epsilon times one by delta x so delta x by delta t whole thing squared is of order square root epsilon okay so basically this tells us the time derivatives are much smaller than space derivatives by a factor of square root epsilon and we want to examine Einstein's equations in this limit okay really clear what we want to see is that Newton's law has come out of Einstein's equations okay now as we've seen and in order to get Newton's laws all that's important is that g 0 0 takes the form 1 plus 2 phi where phi is the Newtonian potential we got agreement with behave with motion in a Newtonian potential provided that all g's were 1 plus order epsilon and g 0 0 was of this form it didn't matter to us what g i j was do you remember that okay so we have to demonstrate is that g 0 0 when written as 1 plus something is that that something becomes a Newtonian potential the g i j's can be whatever they want it doesn't affect the Newtonian limit the strict Newtonian limit so what we want to do is to find an equation for g 0 0 sorry what we want to do is to find an equation for the the deviation from g 0 0 so we write g 0 0 is equal to 1 plus h 0 0 and try to find one of Einstein's equations that in this limit of smallness gives us an autonomous equation just for h 0 0 so the equation we look at is this one the equation we look at is that okay now there's something else that I should have said this the something else that I should have said is so far we've been looking at Einstein's equations to the answer Einstein part of the equations but there's also the matter but we're looking at the non-relativistic limit in matter so imagine that the matter has made up of a bunch of non-relativistic objects moving around okay in this limit the rest energy the stress tensor of this this this system is dominated by the rest energy of the system right so t 0 0 is going to be much much larger than okay it's going to be of order t 0 i will be of order v i times t 0 0 is this clear and and t i j will be will be down even even smaller t i j will have a v i v j in it would be of order v square compared to t 0 0 so the dominant term on the right hand side is t 0 0 and t 0 0 is larger than t 0 i by a factor of square root epsilon and t 0 i is factor by as larger than t i j by another factor of square root epsilon okay so that's the other thing that we're going to use because the matter itself is assumed to be non-relativistic so given all these assumptions we want to check that we get back newtons equations okay so now let's look at this in this equation r 0 0 what was Einstein's equations Einstein's equation was that r mu nu is equal to 8 pi k we're dropping the C's t mu nu minus half delta mu nu t so keeping things just to leading order on the right hand side okay what we're going to do is to reduce everything here just to the to the t 0 0 parts but this should be an r you think okay good so that's something that I forgot to tell you about last time let's let's let's move back to our so our mu nu we had our mu nu minus half r by 2 delta mu nu is equal to how was it 8 pi k tends to be okay now there's another way of writing this equation that we can get by just taking the trace of both sides of this equation so if I take the trace on both sides of this equation what I get I get r by 2 wait so let me be careful here the trace of this guy is just r the trace of this guy is 4 times r but there's a by 2 here so that's a minus 2 times r so this is minus r okay is equal to 8 pi k times t let me plug this in here so now what do I get I get our mu nu plus 4 pi k times t delta mu nu is equal to 8 pi k mu nu which implies that our mu nu is equal to 8 pi k in a T mu nu minus half minus t by 2 delta mu nu so this is an equivalent way of writing Einstein's equations this and this are the same equation this is the form that I'm going to find more convenient for whatever don't know is this clear okay so the next thing I'm going to do is to try to understand I'm going to take this equation so I'm sorry I'm extra chaotic today we're going okay but I'm going to write here so now what I'm going to do is now take the indices mu and nu to be 0 and 0 so we get the equation r 0 0 is equal to 8 pi k then there's a t 0 0 okay and we get minus delta 0 0 so that's 1 times half of t since we're only keeping leading a leaving on on the right-hand side we can replace that what was t t was t 0 0 plus t 1 1 plus t 2 2 plus t 3 3 1 index lower 1 index higher 1 they suffer and doubt and we're only going to keep the leading order term so this was half of t 0 0 keeping just the leading order okay so we've got all 0 0 is equal to 4 pi k times t 0 0 in the approximation of which we're keeping things this is what one of Einstein's equations being because okay now to further process this this so remember I'll keep this on the board because this is we want to we're going to write g 0 0 0 1 plus 2 phi and find an equation for phi okay but let's go there slowly so we've got we've got this equation now and I want to process this r 0 0 so firstly let's remember what let's remember the formula for r a b cd okay so the formula for r a b cd was what it was gamma a b we had c comma d minus gamma a b d comma c plus terms that are quadratic in gamma now if we write g as 1 plus order epsilon the Christopher symbols are obviously for the epsilon because they involve derivatives of the metric and one has no derivative so Christopher symbol square is obviously for the epsilon square and we're gonna only good only going to be keeping this equation to order epsilon the minus sign is wrong the first one is a minus sign the second ones plus thank you okay thank you okay good now that's right. That's it thank you thank you, thank you thank you thank you. Thank you thank you thank you, think let me write it as plus okay good yes and thank you yes okay so we only need to keep these two terms okay more over every term that we are keeping has at least one factor of the small metric as we said so this automatically of order epsilon so any further smallness is we kill it what does that mean that means that all derivatives that we are taking should be spaced derivatives okay so now let's actually let's process the formula for our so firstly now what was our we want to contract the first and third indices together so we get a so gamma a a and now we want okay and then of course we this is going to give us our zero zero with both indices lower but the difference between upper and lower is a factor of the inverse which differs from delta and one higher order of smallness so we ignore that so r zero zero with both uppers is the same as r zero zero with both lowest because we're using the signature no minus sign because we're using the signature plus minus minus minus okay so to the same order what we're interested in is okay let me be more systematic r zero zero which is the same as r zero zero to the order which we're working is equal to gamma a a zero zero minus gamma first and third first and third first and third sorry first and third a and c gamma a a zero zero minus gamma a a zero zero now we decided that because all these are already order epsilon any further smallnesses for instance by differentiating with respect to zero should be ignored so we ignore the stuff is this clear so all that remains is this guy so we've got gamma a zero zero comma a now this a runs over all values but we'll only allow it to run over space because we don't want a time derivative so gamma i zero zero i so now all we need to do is to compute this gamma i zero zero zero i but we know how to compute that that is equal to minus half g zero zero comma i plus terms that it will involve time derivatives which we're going to throw we've concluded from here that this equation in the in the Newtonian limit that we're considering simply boils down to minus half g zero zero comma i is equal to eight pi four pi k t zero zero okay now we substitute g zero zero this is basically we've met our objective we've got an equation that autonomously determines g zero zero forgetting about all the others okay and now we just now we just oh sorry and there was another eye so this is del square spatial del square okay so now we substitute g zero zero is this so we get minus del square phi is equal to four pi k now this we can call mass density energy density it doesn't matter because we're setting c equals one we work it non relativistic limit okay and this is of course Newton's equation once you identify well in some convention once you identify the gravitational constant Newton's constant as how yeah case G but without four pies okay I think this is case what yeah case G right so K is equal to G it's Newton's constant once we make this identification we've got Newton's law Newton's law of gravitation so in the appropriate limit neglecting many things that are small inappropriate circumstances these are the appropriate circumstances include motion of the sun for instance okay we've recovered Newton's equations so we see that Einstein's equations why much much much bigger than Newton's equations Newton's equations gravity much more beautiful much more complicated having much more structure reduced to it in the right limit which is of course a necessary condition for it to be the right equation of gravity since Newton's equations have been fabulously tested for instance in planetary motion okay questions or comments about this okay so now let's move on now we understand that these equations reduced to reduce to Newton's equations so that's one well this is minus sign is the minus sign minus sign is not changed so we've messed up on the minus sign but did I wait sorry I've messed up the minus sign the minus sign shouldn't be there let me let me look at that okay yeah wait and was correct oh where did this minus sorry no no no that was okay the minus sign is okay let's see let's see let's to check what is the gravitational potential of a delta function source according to this equation so according to this equation if we do the Stokes theorem kind of business I mean the Gauss theorem kind of business then integral of del phi over the surface will be equal to something negative okay so that would tell us that the gravitational potential is equal to 1 by r so that its gradient is minus r hat by r square okay not bad that's the usual answer right okay thank you okay fine okay maybe we've not messed up maybe I just was checking with Landau-Liffchitz they've got the opposite sign sorry wait I think we have messed up you know in this sorry we have messed up here because we're using this weird metric you see we have this gamma ii now I want to write this in terms of both indices lower because that's what del i squared is del x times del x okay and just to say it again that this formula that I wrote down was a formula for the gamma with all three indices lower then there was a G inverse of the upper index there was a G inverse of the upper index and in special directions G inverse in our conventions has a minus sign sorry so okay so this is what we're getting now now you've confused me into thinking this is not this should not be what we're getting what no no no I think he just just a minute and now we just have to remember Newton's laws okay how does it normally go but let's look the gravitational force should be attractive okay so the gradient of the gravitational potential should be negative so the gravitational potential should be positive and this sign gives us right one potential one by our gives us force minus our hat by our square which is correct okay so we so this is what we expect if K is equal to G no no no no no force should be attractive so one by our now differentiate forces minus gratified okay okay so the question is with this one by two five did we get T minus T minus V or T plus V in our when we looked at our square okay let's let's get the straight let's go back suppose we looked at our at the motion of a particle okay so this was square root G mu nu DX mu DX nu now this thing came with a minus M okay now in this we write minus M integral square root of 1 plus 2 phi we put a DT here so that's 1 minus DX I minus V squared squared and you're right that that what we're getting here is so the action is turning out to be MD XI by DT the whole thing squared minus M phi okay so this was our action now as you say this will give us so but when we differentiate we will get acceleration minus acceleration minus grad phi is he is equal to zero so acceleration is equal to grad phi so force as you say thank you is minus gratified correct so the force is minus gratified so minus gratified should be negative okay that's right so minus gratified negative gratifies positive therefore phi should be negative according to Landau leaf shits well you know we should be able to work consistently in writing 1 plus 2 phi we've identified it with the potential okay so now unless we flip our sign of K something is just one minute have I messed up somewhere else wait okay maybe we have got it right okay let's let's let's let's keep thinking now yeah I think it's all okay look see we wanted we wanted grad phi to be positive okay sorry about this we want to grad phi to be positive but that's consistent with del square phi is equal to this because del square phi is in integrated over volume is integral grad phi over the surface and so in grad phi is positive so that the force is negative this is actually positive so I'm saying that the solution to this will be minus 1 by r the solution to del square phi is equal to positive delta function is minus 1 by r okay sorry about this sorry about this this was embarrassing okay so okay so now we are all happy with our signs it all works we believe that Newton was correct gravity is attractive rather than repulsive as we were finding briefly and and and we're all happy okay now the next thing we want to do is to go beyond the next thing we want to do is to go beyond working this Newtonian approximation because it's great that it reproduces Newton's laws approximately but we want to see what happens exactly okay so though I'm only going to be able to teach for the next six minutes I have something urgent to do it in past 12 we'll have to continue this mainly tomorrow but let's start setting it up the thing that we want to do is to try to solve Einstein's equations in some interesting situations and the most interesting situation is like to try to understand the well and all these first thing to do is try to understand planetary motion around the sun so we want to find the grad the solution to science and equations due to the sun okay but we're going to do this in a way that is a little more general than to be so that we can use in other situations as well let us try to set up Einstein's equations let us try to set up Einstein's equations in yeah so let us try to set up Einstein's equations in in a manner that that is that you that that is correct for any spherically symmetric situation okay at the moment we won't assume that this the situation is static but we will assume spherical symmetry okay so what is spherical symmetry mean spherical symmetry means that you know things in that direction in that direction are the same around a given origin okay so the metric in our situation should have a rotational symmetry symmetry of rotational rotations around this origin point okay what does that mean that means that the metric should have a factor okay so let me write down what it means and then you tell me if you agree with us this fixes the metric to take the following form firstly first thing we have to you know when we're dealing with Einstein's equations you might ask metric in what coordinates okay working general coordinates except for the metric on the sphere you see because we've got rotational invariance then it must be it must be possible to foliate our space time into two spheres into a two-parameter set of two spheres because what does it mean to have rotational invariance you take one point okay you rotate it you go to another point which is physically equivalent to the first point okay now if you take any point in space and rotate it in all possible ways what does it generate to generate the two-spheres okay but a two-spheres just a two-dimensional object space time is four-dimensional she must it must be possible to take space time and foliate it into a two-parameter set of two-spheres to generate all four dimensions of space time so on the two-spheres on the points that are related by symmetry by rotational symmetry to any other point we're going to use standard coordinates standard polar coordinates of the two-spheres so we'll use the angle we'll use the coordinates theta and phi this by the way is something very this procedure something very general that while while in general there's no preferred coordinate system in Einstein's equations once you're looking at a situation with certain amount of symmetry that picks out a very natural set of coordinates which is always advantages to use okay because we're looking at solutions with rotational symmetry in the two-spheres we'll use coordinates that are naturally adapted to that symmetry on part of this on part of space what about the other two coordinates so far we made no assumptions they're just two other completely random coordinates let's call them are and why should they be on a sphere because you have this rotational symmetry the other two could be anything they need not be no no they completely arbitrary coordinates there will the range will in general what the two-dimensional right and then the requirement of rotational symmetry is that the metric take the form ds squared is equal to minus dT squared into some function plus dT let's say dT dr into some other function plus dr squared into some other function a function let's not all is d because it's e times a d theta squared plus sine squared theta d phi squared where a is equal to a of rt b is equal to b of rt c is equal to c of rt and so on just to be totally clear what does it mean that this metric here has spherical symmetry what does it mean as a mathematical statement okay what it means is that there is a change of coordinates this change of coordinates is generated by rotations under which so such that in the new coordinates the metric has the same expression and the metric is the same expression as a function of new coordinates as it had as a function of old that's always where a symmetry means in physics there's some change of variables such that something doesn't change form as a function of new variables compared to function of old variables the rotation here is how those rotations act on this metric well exactly the way rotations act on a two sphere in theta phi coordinates okay and it's obvious that this metric this rotation doesn't touch the t and t and r coordinate it acts only on this part of the space and from the fact that the metric of two sphere is rotationally invariant okay the rotational invariance of this full metric follows I mean pedantic you know what I'm saying is obvious don't let it confuse you but just to make sure you understand exactly what it means okay for instance phi goes to phi plus delta phi is obviously a symmetry of this metric because in the new phi prime coordinate it takes the same form as in the fight one now what what ensure there was a symmetry of the metric first that the metric of the sphere took this form but secondly that there was no phi of theta dependence in these functions had there been five dependence in these functions then five goes to phi plus delta phi would not have been an isometry of this metric okay how do we know that this is the most general rotationally invariant function on the sphere the reason is that the only okay so it's sort of clear that this part of the metric has to be the metric of the sphere but could we have had some function of theta and phi entering here that was rotationally invariant and the answer is no there's no rotationally invariant scalar function on the sphere apart from the constant this you know from your study spherical harmonics all functions can be expanded in spherical harmonics and the only spherical harmonic the spherical harmonics transform in representation of the rotation group the 0 1 2 up to infinity representation of the rotation group the only one that's rotationally invariant is the one representation of the constant okay so the only scalar function the only combination of theta and phi that can appear here is some function of your coordinates of the sphere some scalar function that is invariant at rotations and there's no such function apart from the constant so these things could not have depended on theta and phi without sacrificing rotationally invariant okay so this is the most general metric that preserves rotational invariance is this clear greatly simplified our task it's greatly simplified our task for two reasons firstly we know a lot about the structure of the metric and theta and phi and secondly all these other functions are not functions of four variables but only functions of two variables so in a sense imposing rotational invariance has made the problem of solving Einstein's equations roughly as easy as it is to solve Einstein's equations in two dimensions which is a very easy task as you will see in some problems it's okay so so so so this now is more or less a solvable problem as we will as we will indicate okay but unfortunately not today because I have to run so we'll continue tomorrow at 11 30 math mathematics seminar over sorry about this okay I'll just run immediately since I'm doing this late anyway


Welcome back everybody drone tech here, and today I have a clip from an interview between Willie Geist and Dr. Fauci on MSNBC and after some drooling sycophantic cult-like Agulation guys to actually ask some a pretty decent question about the reopening of Texas and the doom and gloom that we all Heard was gonna come from that also before we start make sure to hit that like button It really helps this channel back on the show this morning particularly talking some baseball Let me just say that I absolutely hate when these guys say things like that like oh, let's talk some baseball I want to say that I got my first shot of the vaccine yesterday. I feel great mild soreness in my arm But it feels good. I'll go back in four weeks for my second dose. Wait, it feels good. I mean come on now It's a coronavirus vaccination. It's not a shot of heroin He can't just pat himself on the back for getting the vaccination No, no, no, he has to say that it felt good My wife and I who went together yesterday up in Suffolk, New York felt nothing but gratitude For the doctors and the scientists and the public health officials like yourself who brought us to this day So I know I speak for a lot of people in this country when I say that with that.  Why don't you said you mentioned Texas in that full ballpark in Arlington yesterday? There was a lot of concern last month when Texas effectively opened up Dropped all those restrictions and said it's back to life and if you go to Texas as you know It looks like 2019 the restaurants and the bars are full and open the ballparks are full and yet We've seen cases in hospitalization since then continue to tick downward So what do you make of that as all of us look around and sort of try to consider how safe it is to get back to normal life? Yeah, you know, it's it can be confusing because you may see a lag and a delay because often You have to wait a few weeks before you you see the effect of what you're doing right now Just to point out. It's been a month. It's it's been over a couple weeks So I mean if there was gonna be an effect you would definitely see it by now You know, there are a lot of things that go into that I mean when you say that they've they've had a lot of Activity on the outside like ball games. I'm not really quite sure it could be they're doing things outdoors You know, it's very difficult to just one-on-one compare that you just have to see in the long range I hope they continue to take down. Okay. I just want to kick it back here real quick and just replay this one part One second here activity on the outside like ball games. I'm not really quite sure it could be they're doing I'm not really quite sure well Fauci isn't sure about a lot, isn't he? Let's not forget here that in early January dr. Fauci said that we had nothing to fear from this virus And then a little bit later. He said that people shouldn't be out there wearing masks He said that there's no reason to be walking around with a mask When you're in the middle of an outbreak wearing a mask might make people feel a little safer and it might even Block a droplet, but it's not providing the perfect protection that people think it is and often there are unintended Consequences people fiddling with their mask touching their face But then he changed his own mind on that despite the fact that his earlier stated facts weren't wrong I think later that he claimed that he was trying to stop a run-on masks That would limit the number that would be available to medical workers But the thing is nothing that he said before was wrong and he even stated that during a 60 minutes propaganda session that he Quote didn't regret anything he said, but if he lied about that and doesn't regret it What else has he rationalized lying about then in mid-February during an interview? He said that the flu was a bigger threat and then later changed his mind on that as well Then around mid-March during an interview with Jonathan Carl He said that normal life would be returning quote within several weeks to a few months For sure and it doesn't even stop there his numbers on the levels of vaccinations needed to achieve herd immunity Have been changing as the months pass He started at 60% then the 70% then the 75% and now it's at 85% And it'll probably change from there I don't know. Maybe this Fauci guy isn't the shimmering man god folks like Willie Geist present him as Almost like the media is lying to the American people to push a political agenda All right, folks I have a busy day with the family today So just a short one, but I do want to remind you all that I am on other platforms like odyssey bit shoot and rumble Come check me out there just in case as always Thanks for watching and make sure to check back tomorrow for a new video


Hi everyone, Joe for Jasper's CaseRakes.com with a random number block randomizer for the Grizzlies, Bucks, Pelicans, Sons, Wizards, Bulls, Cavs, and Nets. That unlocks Pick Your Team 3, which will be coming up in a different video if you're looking for that. That's how it works if you're not familiar with it. And three extra spots being given away here. So big thanks to the people who bought seven spots outright, Michael, David, and Michael L, Michael P, David, and Robert. Thank you. And we'll randomize those seven names with a different dice roll. Our first dice roll, the second dice roll, will be for the numbers. But with this, top three after six, two and a four. Good luck. One, two, three, four, five, and sixth and final time. Top three, Michael L, Robert, and David. Sorry, Michael P.  Now let's gather all these names here, paste them in there, delete that on the list. All right, now our second and main dice roll, it's going to be four and a three. Seven times are names and numbers. One, two, three, four, five, six, and seven. We've got David down to David, four and a three for the numbers. One, two, three, four, five, six, and seventh and final time. Good luck. We've got four down to zero. After seven, remember zero gets any and all redemptions for that group of teams right there, including one of one redemptions. So that's for you, David. David, you also have four, eight, and two. Robert with seven. David with three, David with, Michael P with three, David B with five, Michael L with nine, Robert with one, Michael L with six, and once again David with zero. All right, gang, so let's order these numerically and we'll see in the next video for the break itself, jaspyscasebreaks.com.


an opening play that has the purpose to change situations. No good. That's the end. With their train of ancient venerable prejudices and opinions it's equated before they can ossify and manned conditions of life. His real and dangerous highway system that points us here. People must shade material for God making. A general thank you God Sunday through Sunday useful for all occasions. Mystery God we know nothing about. It's the special God of the day the God of moms and kids who shouldn't be separated. So we sing the hymn of the day first which is blue and mages to the courage which allows moms and kids to flee to sea. In southern Arizona truck loaked and bounced over the notoriously duff rough desert roads on our way to the ranch on the outskirts of town against the backdrop of the mountain ranges that separate the U.S. from Mexico south of Tucson. Upon arrival we introduced ourselves to the travelers.  There was a mother and her daughter as well as the daughter's boyfriend all from Honduras. They were cordial but timid shuffling their feet eyes cast downward as Katarina explained that she would be taking their vitals. We were here to help friends of the church. Samaritanos. They had been on the road for over a month. They crossed the southern border of Mexico by foot before trudging through the jungles of Oaxaca and Tabasco and Chiapas walking the hills and stopping in small villages to rest. They had never been to El Norte before but it became their home for some time as they struggled to find funds to cross into the U.S. eventually hoping to be reunited with family in San Jose, California. Their desert journey had been intense and they felt unwell. The days of waiting to cross, the hot sun, the terrain, their shoes were torn and their feet covered in blisters. They had been chased by La Migra, gotten away, became lost until now. With Katarina's presence, a skilled wilderness EMT, I stepped back to watch her, taking mental notes of her observations and intuition, her precision and care. Things were going slowly. She stared down at her notes, furrowing her brow. Something was amiss. Estas embaresada, she asked the younger women. My eyes widened as my heart sank. Our younger female patient was five months pregnant. I stepped out to allow some privacy. Katarina returned outside after some time to update me. Things were complicated. She had noticed the color of the older women's skin as well as the younger ones, both jaundiced and yellow. There was likely something going on with their liver. She phoned a doctor for more advice. The doctor surmised that they both had hepatitis but with no lab to take samples, we were forced to diagnose on observations alone. We settled into what would be a long afternoon. The family told me that they were done walking. They were ready to get picked up by their ride. I tailed deeply and began my explanation of where we were of the Border Patrol checkpoints which lay north on each road. Even if I called an ambulance, they would be captured upon leaving the hospital. If they wished to continue freely, they had only one option, going back into the desert and walking north. There were many miles to go. The younger woman told me she hoped to have her child in the U.S. so that he or she may become a citizen. She looked over at her boyfriend and squeezed his hands, trying to affirm resilience, but morale was low. Her mother started crying. I told them that they should rest, that there was no rush to begin their journey again. It didn't need to happen today. Katarina returned from phoning the doctor, hoping to get medicine sent from Tucson. Until then, there was nothing to do but wait.  It's on a remote property just north of the Mexican border in January. What an idea of the day. This one here, the God of mums and kids that should not be separated. And now we need to get rid of health somehow. Why magic? We got that. Why magic? Don't you look sad, man? Katarina said, When the sun sets, When the rain stop, When you leave the sun, When the sun is rising, When the sun is shining, When the sun is shining. And when the sun rises, When the sun is rising, When the sun rises, When the sun is shining, The Earth is burning. And the world is recognizein my children, they are all here. Oh Hallelujah!


The 10th Annual Open Source Jobs Report Produced by Linux Foundation Research in partnership with edX and Linux Foundation Training and Certification 86% of hiring managers say hiring open source talent is a priority for 2022 78% of hiring managers are hiring the same or more open source professionals compared to 2021 93% of hiring managers report difficulty finding professionals with the needed open source experience 58% of hiring managers have given higher salary increases to retain open source talent 77% of organizations are growing their use of cloud container technologies 76% of professionals work on open source projects related to Linux 73% of open source professionals believe it would be easy to find a new position 90% of hiring managers are willing to pay for certifications 69% of hiring managers are more likely to hire certified open source professionals 67% of hiring managers seek open source professionals with architectural skills 48% of open source professionals and hiring managers rate their employer diversity efforts as good or excellent 62% of organizations employing open source professionals encourage diversity in hiring


So what are some of the new innovations that are coming up? I'm sure that you're working on some groundbreaking, cutting edge technology, so could you share that with us? Absolutely, so it probably the biggest technology that we're trying to focus on is a process called painless defibrillation. What do we mean by that? We've all seen on television, when someone has a cardiac arrhythmia, for example, they say V-fib, cardiac arrest, or things of that nature, they bring the paddles out and they shock the patient and the patient jumps off the table. Unfortunately, that's not that much of an exaggeration, that's really often what happens. So what we're trying to do is to create a system where we can treat the rhythm without having to shock it. And that way you eliminate the discomfort for patients, a lot of patients get PTSD, post-traumatic stress disorder with these repeated shocks and what our real goal at the end is to really make these treatments imperceptible even to the patient and eliminate all that collateral anxiety, risk of complications, infections, all these things in one false swoop by having a wireless miniaturized pacemaker.  It truly is, and so what in terms of where you are in the process, where are you right now? Right now we're in the preclinical phases. We are hoping to have initial clinical work probably within about three years, three to five years. But the movement has been actually quite brisk. We have had a number of federal grants to support this. These are very competitive grants from the National Institutes of Health and we have a couple of those grants that we're very proud of. So it's been moving along at quite a brisk clip. Obviously with the pandemic and everything, the last few months we've had to kind of be a little bit more cautious, judicious, but nonetheless, the work is progressing.


M is for mom. Is that your mom's name? Yeah. In case those of you didn't know that. It's a beautiful name. That's the Hindi word for mom. Mada chod. Mada. Mada is mom. And chod is love. Love. I love you, mom.  Josh!  Instagram followers there. Thanks to Patreon followers for the camera. We've got to be a squabby. That's the first place you would have found out I'm married. He's a betrothed man. Wait. Yeah, betrothed. That's correct. Is betrothed after you get married, or is it pregnant? If you are a betrothed. Oh. That's what I was wondering. I didn't know betrothed in like the other day. Is betrothal engagement? And yeah, for many of you who saw the thing, you're like, oh, congratulations on your engagement. No, we're hitched. Yeah. So today, a new teaser drop. Just this morning, I think it was our own one. I felt it. 6am. Yeah, around 6am, I felt a little tickle. Yeah, that's a little teaser. 4.3. Yep, teaser. On the teaser scale. This is for Vikram. I think you've seen one teaser for this. It was an announcement. I'm trying to remember what it was. He was just in a room, because it's Kamahasaan, right? It's called Vikram. Yeah. Was he just in a room, and stuff was blown up? I think so. If that's Mary serves me right. I'm thinking of something different. No, I think that's right. But this is called Vikram, the first glance. It's kind of like RR. It's not really a teaser. This is kind of just a big video now. It's just the new way things are done. I know. It's like there's pictures, there's character introductions, there's glances, there's teasers, then there's trailers. And songs. Yeah, so now pretty soon, what we're going to have for most big films is at least six different things before they're coming to traction. I'm coming. Used to just be trailers. Yeah, it used to be. Yeah, never even. Do you know why they're called trailers? They used to. They used to follow the feature. They used to trail the end, used to stay afterwards. And then they realized, wait, no one's staying to watch the trailers. Let's do it again. Put it up at the front, but didn't change the name. Here we go. Nice. That was good. Lighting was beautiful. And a couple of those things, really great. So he's playing basically John Wick or something like that. I feel like that's a huge. He's going to kick some butt. I mean, not that Indian films have been doing that for a long, long time. Just one guy kicking ass, right? Of course. But I feel like that's a huge trend now, even in Hollywood, since the, I mean, I guess it's not new.  It's like John Wick. It's basically James Bond 100-fold. Yeah. It's like Bond was the first big action hero who could kick everybody's butt, get all the girls. And I'm sure there were some heroes. I mean, there were. There were the swashbuckling heroes of the silent era. But yeah, it's a, that's never going to go away. It's a really fun thing to see a seager hero kicking butt. Now the headshots, those are definitively John Wick. Yeah. I remember Mike and I going to see the last John Wick. The house was packed. And Guy comes in with popcorn.  And everybody's like, yeah! I'm trying to, I swear we did it. It was a title teaser, right? I think so. Anyways, because it, remember that. He's in a room, right? He's in a room. With a legendary stash. I don't know where our reaction to it is. Let's see, 11 months ago. Yeah, he was in a room. We saw that, he's in a room. Absolutely. Did ours get blocked or? It may be blocked on my Patreon. That might not be the reason it's not there. I have no idea where it is. That's weird. I absolutely remember that. It was a while ago. November 7th. So it was a year ago. Oh wow. Wow. Probably got delayed due to COVID. He was in a room, he looked awesome with the legendary moustache. It was super cool. Yeah. Shit hit the fan, I think. Exactly, stuff started, he just started. Oh yeah, he had stuff under the table. Yep. That's what it was. So is he, I'm guessing he's like an assassin of some sort. I don't know. I think he'll kick butt. We haven't seen, what's our most modern Kamala son? Is it, hey Rob, is that our most modern? Wow, for our most modern film of his life. Oh yeah, I haven't seen much of him outside. In terms of watching his films yet, we've seen I think four, maybe. Why do I feel like we saw something that he was in that's more recent and he didn't have a big, it wasn't like his starring role? Well, we've seen a bunch of songs, obviously, and trailers and stuff. But I think films, we saw that first one, which was the playing strings on automobiles one, and hey Rom, and then the Naya Khan. And I think it's hey Rom. It's another one. I think you're right. And I think we've only seen about four, which we will get to a lot more because we think he's a great actor. But it'll be interesting to see him more modern. He looks epic in that beard. And I love the, I think they had that Vikram song in the first one as well. I remember that. Vikram. I love the song at the end. I thought there was a real kick ass, as the kids say. As the kids say. As the kids say. This reminded me also, a lot of you have sent us messages about what had happened on the set with the fire, with, you know. The rust. Yeah, with rust. And yeah, we were both, if you follow us on Instagram and Twitter, you know what we feel about most everybody in the industry. And I'm sure in the Indian film industry, it's like, why? There's no reason under the sun ever a real gun or live ammunition should be on set. Ever. Period. So very, it made me think of it, especially with, there's the one shot was straight at camera. Yeah. And yeah, it's just a horrible. That's not pointed at the other actor. That's pointing right at the camera. Right at the lens. That's why the one who died is the cinematographer. It's a common occurrence to have a shot that's looking like that. And I'm sure it was staged that way. But and obviously more at the filming of this, there's still investigations going on. But yeah, the bottom line is that there should just have never been. And I'm sure it's the same way in Indian cinemas, is there shouldn't be live rounds and there shouldn't be working guns. The technology is so good. No one should ever die on set. Yeah, it should never happen. It's not a thing that you should even think about. Exactly. Even the people that are doing the death to find like stunt formers, they should never die on set. No. Like they're the ones going to be the most at risk, but they're professionals. And so all the safety precaution is still taken through those. Exactly. If you expect it to happen to anybody, it should be a stunt person doing an extraordinarily dangerous stunt, not your DP. Even still. Even still it shouldn't happen. The stunt formers should never die on set. Nobody should ever die on set. Like it shouldn't be a complex issue. But here we are. Yeah. But yeah, this looks really good. I don't know when it said it comes out, but I'm sure it'll be here in the next few months. We just got the first drop of a big Indian film this past weekend with the Renviers and Akshay's. Yeah. With that big cop one, right? Yeah. No, I imagine it'll get dropped. But I think I'll be surprised if any films drop anywhere near the week of our hour. I think everybody's going to avoid the box office that week. I think Alia's is coming on that same day. That same day. I think she has two films coming on that day. Well, that works. Because if she's in the film, that you're like, because she's in, maybe. Yeah. I still wouldn't. I still would. I would leave a stay away. If it was my film, I would say stay away from the video. Let us know what else we need to know. But this one should be our next Kamal Hassan film that we should watch. Let us know down below. Josh!