Information sharing is the key to making a successful team. And Microsoft Teams has multiple methods in order to make information sharing as easy as possible across all of your work teams. There are times, however, when information sharing is not such a good thing. Maybe there's sensitive information that only a select few members of the team need to know. Maybe it has to do with legal or financial matters that the rest of the team doesn't need to know about. But now with private channels, you now have a place to store that information within your team. To create a private channel, make sure you're the owner or have permissions to that channel and when you hover your mouse over the team name, you'll see ellipses. Click add channel and then under the privacy section, select private. On the next screen, you can add members to the channel. When complete, you can see the private channel appear in your team channel list. You can distinguish between a normal channel and a private channel simply by looking at the lock icon. If it has a lock icon, it means it's private. If you're new to Microsoft Teams and need a little help understanding the basics, we do offer a free course called Teams Essentials. It's available at our website at protectedtrust.com but we'll also leave a link for you below in the description.


on a paste, ladies and gentlemen, it is indeed a pleasure to address you today as you meet in Colombo at this Global Symposium of Regulators to discuss the new strategies for the regulation of telecommunications and focus on the progress of information and communications technology. Mr. Secretary General, thank you for the nice comments about Srinagar. You have been here, I think you are, through the end of 2009 at audition. It is timely that this symposium focus on ICG, take place the day after the International Day of the Child because it is a technology that has great attraction and mean to children. It can take their thinking and skills to new heights of achievement. It can promise them a great new world of ideas and innovation. It can also lead them to dangerous influence, draw them away from tolerance and towards extremism. It is a technology that needs to be handled in great care, imposing much more duties and responsibilities. On parents' guidance of their children, the wonders of ICG should not eliminate our children from what is best in their culture and traditional values. I welcome you all to a country that is making great progress, both in telecommunications and ICG. So, soon after ending nearly three decades of terrorism, we do significant emphasis to development of the country. With ICG playing a vital role in the path to progress, the ICG sector stands out in the progress made by Sri Lanka in the past seven years and accelerated in the three years since the defeat of terrorism. Our emphasis on communication has a key part to peace and reconciliation. Can be seen by the speed with which we restore the communication tower in Kokani in the north, destroyed by the forces of terror. This opens speed communication to the area, most damaged by it. Two weeks ago, we also linked the entire non-earlier, radish, vitality to the national power line, which will lead to the progress of telecommunications and ICG in this region. Sri Lanka recognized the need for rapid progress in the field of ICG, a technology that is rising in the height with innovations and new applications that make our world smaller each day. It opens pathways to progress to the people, breaking down the barriers of race, ethnicity, community, faith and geography. And I think pride in this, in standing, stating that our progress has been remarkable. We now have more than 20 million fixed and mobile phone users in our country exceeding the size of our population in what is considered a middle-income country. Our population is greatly bigger. We have 750 nano-cells or rural cell centers, which one can call a knowledge center, as we have largely in the rural sector, linked in the rural people to the benefits of the age of information and empowering them to progress in life. Similarly, our rate of IT in the region has gone to over 40% within the past six years, with opportunity very soon for every school to have a state-of-the-art computer training facilities. These advances have positively impacted on the rural sector and helped the world to grow to the economy. This also makes Sri Lanka a promising destination for investors in device sectors from business also saying to industries, tourism and agriculture, difference. As we move ahead in ICT, Sri Lanka has set the motion of plan to develop a policy and regulatory framework for next generation network on MGA and to have a national broadband policy before the end of this year. We see the importance of broadband connectivity throughout the land for people to fully benefit from the speedy advances in ICT. To take our communication which beyond our land, we are already engaged in constructing what will show me the tallest communication tower in South Asia. It will give telecommunications, telecom operators the opportunity to share a moment and state-of-the-art infrastructure in a faster fashion, taking us closer to be the communications hub of South Asia. Our emphasis on growth of ICT comes from the awareness of the new revolutionary age living, the technology revolution. We see this mist in the smart phone that will soon be the pockets of all. A device that has made the old child computer a primitive piece of technology. We see how mobile communications can bring revolutionary changes to the lives of new life scales, new employment opportunities and new links to markets in one's country and abroad. It can bring new educational opportunities, expand health and healing services, have a possible impact on sustainable development, increase production in agriculture and expand the market potential of small industries and also develop new media. With the essence we have in education, recognition of skills, really trainable workforce and search for new areas of competence among our youth. Sri Lanka will not be left behind in this new age of knowledge. We are ready to watch ahead to the new opportunities being opened by ICT. We have been building, we decided to build in the deep south of Sri Lanka, once the most neglected area in development. We have already other mega infrastructure facilities such as port and international port are being built by new friends. This symposium of strategies and regulators in telecommunications and ICT, look at them. Look at all the challenges ahead with the experience of recent weeks. You will take of ways to prevent this great technology being used to you so hard. Examining how to avoid the advances in the incident of communication being the source and cause of violence against faith, against culture and traditions that need respect and protection. ICT must not be the tool of society that pay homage to material values and pay no heed to the values of decency, tolerance and humility. You will study the areas where the better education is required. How this advances in technology can be abused as much as they are used to benefit people and society. You will consider a new roadmap for progress in a field of technology that is on a path of continuing speed growth. That is the challenge of this significant global forum. I thank the international telecommunications union ITU for giving Sri Lanka our telecommunications regulatory commission, the privilege and opportunity to host this important and timely. We will be able to witness first time what our landlord has been able to do in terms of infrastructure development after a war in Stela. That ended only three years back. It is the proof of our commitment to progress. You will also find our traditional hospitality encouraging for your work. And enable you to take back the best memories of beautiful and friendly people. I wish you all a great success. May you all be blessed.


Welcome everyone and welcome. This is Melissa Armo with the Stock Swoosh and Reviewing JPM, which was the Stock Swoosh Show Play of the Day. And actually, this is along. We went along today. It's like the Twilight Zone, but there wasn't any really good shorts today. So, closed here, 145.15. Boom. Gapped up and open at 146.33 and we did it. So, let's just take a look at the one minute in this. We got in this early and it shook around. It shook around a lot. So, you know, I was trying to get it up to 147 and a boop over the high, but it took all morning, all morning, all morning. Finally did it around 1030 and ran up and actually ran right up here. It looks like the high of the day so far today was 1144. But I still think this can continue here into four o'clock. So, this will close green today. It will probably close near the highs. Again, two hours plus left in the day. There's plenty of time for it to do that. And this is very strong. This is one of the strongest banks out there. Earnings are Friday for JPM, but I thought this was a nice long today. Let's take a look at the market. Let's look at the, let's look at the queues. So, the queues are back and forth today. Up, down, sideways, waiting for the number tomorrow. Let's take a look at the spy. Spy was doing a lot better. A lot better. Spy is green. Again, big inflation number tomorrow morning. And I think the market is going to wait until that. Clearly, we're not really going anywhere today. We didn't really go anywhere yesterday. Then, week after the holiday, lots going on this week with earnings season starting. Inflation number tomorrow on Wednesday. The market wants to wait. It wants to wait to see what's happening. So, not a lot of buying today, but not a lot of selling either. Let's take a look at the spy going into two. Looks strong. It looks fine. It's just not going to go anywhere until tomorrow. So, I'm watching this JPM nice move here today in and out quick is normally what I like to do. This took a little bit longer today, but the patience was well worth it. If you're interested in learning how to trade gaps with me, email me and Melissa at thestockswish.com. Have a great day, everyone.


To je zelo pravda, da imamo tudi tudi, in tudi za to, kaj je vse online zelo, zelo, da vseh vseh vseh vseh vseh vseh vseh vseh vseh vseh vseh vseh vseh vseh vseh. Vse nekaj sem počusti, da Adizh Dabulkar, ko je izvršenj iz ICTP, za druge začne. Dobro, srečo, srečo. Vse je veliko, da me nekaj pravi inograti toj spremskaj skolj, nekaj, nekaj fizika, ker je to je izvršenja iz ICTP, in fakt are remaining really in person after two years of Covid. And as I understand this is the tenth edition of this very nice school on an important topic. And as I understand this year will have about 30 participants who will participate in person in patročno tudi o 150 in in tudi, kot in vzeliš. Vseh, imam veliko prav, da se všel jih. Zelo biš ukazati, da imamo mnogo djih sprihlušt. Tudi vseh sprihlušt. Ja zelo boš sem da boš potrebojat, ki da so prej tako odstavili, ki se odpočila, da je to možemo vsega vsega vsega vsega vsega vsega vsega. Je to neko tegnične detebi, ki se prišli, da se vsega vsega vsega vsega vsega. Vsega, da je to počut, da sem vsega vsega vsega vsega vsega vsega. Čakaj. Protočno, tudi je zelo, da je počkaj počkaj, kako je nekaj počkaj, in tukaj smo počkaj v Politechniku in Torino, in v Universitetu Franco-Italienske, Ne zelo. Ne zelo. Ok. Ok. Ok. To je program. As you see we have 5 speakers, 5 courses. And the course of Tania Sharpey which will be in the afternoons is actually she could not come to Trieste so she will give her lectures online and but I will be in presence so I will do the teaching assistant for her course so and then also we have Gulce. Gulce is here, so no, not yet. So we have a teaching assistant for the course of David Wolpert will also give some lectures on introductory lectures and also Stefano Ruffo will say this and some of the last 3 lectures of this course will be given by Nicolo Defennu, right? Ok, so then this is general outline of the course as you see, lectures are 1 hour 45 minutes but we leave it to the speakers and you to split this lecture this lot of 1 hour 45 minutes eventually in 2 or to start earlier or to finish before but the important thing is that at 10.45 there is a coffee break for you which will be upstairs and with some calories for your brain and so essentially from 10.45 to 11 we have a coffee break and ok, so some rules ok, so it will take some time so your attendance is compulsory so you are supposed to attend each lecture and please be on time lecture start at 9 am start when the program at the time of the program I know it's very heavy schedule for 4 weeks it will be very intense but this is also for the also you should consider that the lectures also put a lot of effort in preparing the lectures and being on time and ok, so still not my screen sharing is post ok, I don't know why ok, so then there are final exams which are compulsory for all of you in presence and and these are essentially marked in bold here ok so at the end of the first of the second week you will have the first two exams then the exam of professor Sharpey will be at the beginning of the fourth week and the last two courses will have the exam at the end of the spring college ok, so we have a lot of online participants and and and we set up a slack space for them so that they can interact with speakers, especially those that cannot attend live the lectures because of time zone difference sorry so essentially you the virtual participants received a link to connect to this slack workspace in order so that they can ask questions offline to the lectures and these questions will be dealt by the lecturers either online or at the next lecture either offline or at the next lecture online ok, so then well this is really very important information so I should share again I don't know why this is ok, so this is working now so lunch ok, so lunch and dinner are offered in the main building of ICTP which is called Leonardo building which is up hill diploma students know very well where it is master students maybe you remember and so there are two ways to go to to the main building one is through the park and so you should go down to the to the harbor and then there are stairs that enter into the park this is a very nice walk and then there are stairs that lead you to this Leonardo building I mean we can do this walk today together if you want the other possibility is to take a shuttle that brings you from no, it's not working so maybe I'll just do like this so there will be shuttles ready at quarter to one at the reception out of the reception that can bring you up to the Leonardo building ok, so also in this building which is called Fermi building is the administration and the medical service especially if you I mean we are unfortunately still living in covid times so we should pay attention to keep this place a covid free place ok, this is a responsibility of each of us really to be extremely careful about this because this could hamper the whole spring college and unfortunately I don't see our head of administration here who could give us some more precise instructions on this but maybe we will tell you more about this for the moment just let's keep the usual I mean the measure that you learn so well in these two years ok, having said this I think we can start and enjoy the college and any problem just let us know, ok thank you very much and well, the floor is yours, one thing I don't understand maybe you know whether speakers can take their mask off you know, atish? ah, ok so I will keep it for a while if ok ok, so you can hear me welcome to the first series of lectures of this spring college and I didn't really realize that for Italy it's the day after the anniversary of the start of the epidemic it was exactly yesterday two years ago that we got the news from Codonio of the first serious case of many infected people and I really hope that nightmare will finish soon and getting together is a good sign that something is moving on so so so you can see my name Stefano Rufo I'm teaching statistical mechanics at CISA and begin in this year I will also teach a course of dynamical systems at the University of Trieste in couple of weeks so my I think one can see also the blackboard you know so my email is rufo cisa.it and you can reach me for any question but I'm also registered on Slack so those of you who are connected to Slack can ask questions also on Slack so this will be a sort of crash course in long range interactions and you will see the topic it is in a while but not for advertising I would like to show you a book which was published few years ago in Oxford University Press I'm one of the author and it collects series of results that were obtained beginning in the 90s in this field of research so the lecture I will give six lectures six lectures and the first one will be a sort of introductory lectures on generic features of long range interacting systems and and the three lectures on quantum will be given next week by Nikola Defeno so Nikola should have been here but he was called for an interview in Houston and today he's in Houston and then since he managed to go to the US and stayed next week also in Boston for another interview he is currently a postdoc in ATH Zurich and so his topic will be specifically quantum long range interactions I think he is also available especially when here it's night for discussions and questions you might have I will provide to you his email also for connection to him so let's start I hope it can go I see I have the same problem as Mattel stop sharing no, the arrows don't work so you can see in this form but if I go full screen there are problems ok, but until it is visible it's ok so I will begin by sort of general introduction some in which sense I will talk will talk about long range interactions but there are several definitions in the literature so I want to be precise to what definitions I will make reference when I speak of long range interactions and then I will I think I will spend the first half an hour to the first discussing about the first topics some of the some of the information will be on the slides and some other I will give on the blackboard so I have prepared some notes and also at the end of this lecture I will leave you with a few exercises to do and I hope that you will be able to do them easily and and of course if you have questions and I'm available even during the day to reply to the questions ok, so wow, what's happening on the screen there is ok I accept any contribution from you even this one it's ok ok, so so how to start so it's I like to start with stories and historians on my involvement in the study of this topic begins here in Trieste so I was attending a very general conference on STATMEK and at the time I was performing numerical experiments on a model that I will tell you about maybe in the third lecture and I was obtaining from my data computer simulation a negative specific key so for me was a sort of of mystery and I was very worried that my program was not working and was giving numbers from God so so there was really no no and I was lucky enough to sit near a guy in astrophysics and this shows that interdisciplinarity is very important and so he asked me what are you working on and I wanted to be provocative and I say I'm working on negative specific key so and then he looked at me and he said whoa that's standard for us so this opened to me the door long range interactions and in fact the statistical mechanics of self gravitating systems is a very interesting topic but very difficult one for several features that gravity has, Newtonian gravity has in particular the fact that the Newtonian gravity is a singular at zero distance so particles tend to collapse in a core because they attract each other and the attraction sees more and more as you get close and another feature which is difficult in I see another sign for the museum beautiful colors so so I another feature of gravitational systems is self gravitational systems is the fact that we live in three dimensions Newtonian gravity is in three dimensions and if you run a code with a self gravitating particles so the interaction is v1 over r in 3d orbits are not closed and orbits are not bounded so it happens that if you start a simulation with say thousand particles thousand Newtonian particles which is a small simulation at the end of the game you will get maybe two third of the particle in the cluster but some of them will have evaporated outside and this is a very bad feature for statistical mechanics because you would like to keep the particle confined in a box concerned boxes you learn it from kinetic theory so what people are bounded to do is to put is to put the self gravitating gas in a box and and let the particle either be absorbed rebound on the boundary of the box so and this is a field in itself is a very complicated area of research another person I could have met and I didn't meet at that meeting was a person in plasma physics plasma physics is another field of research where long range interactions in the sense that I will define are at stake plasma is matter ionize matter and charges are free to fly and you get positive and negative charges so it's really I'm starting with physics 1 you have positive and negative charges and what tend to happen if you have a system of positive and negative charges there is a tendency to screen so for instance if these are ions which are heavier there will be a cloud of minus charges around the ions and this is called the device sphere and the interaction outside this device sphere there are several pluses and several minuses and globally this is neutral so what will happen if you put together a system of positive and negative charges they will tend to form a cloud clouds of neutral charge and all the excess charge will be pushed to the boundaries so if there is an excess charge it will be pushed to the boundaries this is what I teach for instance to first year physics students when I say if you have a conductor the charge will be on the boundary ok there is a strong relation here there is dynamics but ok but it's very important in plasma physics are instabilities that arise when when the charge is globally unbalanced this can happen in several regions of the plasma especially near the boundaries so plasma physics has a very strong interest in what they call a one component plasma one component plasma and the one component plasma is a system of electrons which is confined with a strong electric and magnetic field so there is a region of magnetic field be in the vacuum and as you know the electrons wiggles around these magnetic lines these are magnetic lines and then you put you put some sorry some electric field that bounce the electrons in a certain area this is what is called the one component plasma and the dynamics of this one component plasma falls into the realm of long range interactions because the electrons for instance what they do maybe I will show you a movie at some point they look at the charge in this in this plane orthogonal to the magnetic field lines and and they look at concentration of charge and curiously this charge obeys the Euler equation which is used also to understand climate on the earth surface for the motion of the atmosphere so you see very beautiful vortices cyclons and anticyclons of charge in this plane so this is for motivation but then of course as a theoretical physicist I did want let's try again to to share if it works I don't know so I will go on with so I need to define my setting so it's already 20 minutes for motivations so my setting will be very general and I will define long range interactions by the potential sorry, I will put again ok, so let's take matter in a certain volume and particles interact each other with binary interactions we have one particle here particle i particle j there will be a certain distance r between the two particles and the potential is between the particles is v of r one over r to the alpha at large distance so I concentrate on matter which interacts with power law so alpha equal one for both Newton gravity and coulomb and there are not many examples in nature but one interesting one is alpha equal 3 which is dipolar interaction there, in the room you don't see so we can put it down it's better now? ok, I'm sorry but I'm used to use all the blackboard in three dimensions, yes in three dimensions, yes you will see also what happens in other dimensions for the moment I fix the dimension and ok, so for instance in these dimensions in this slide you see a region of values of alpha for which you can do a very simple calculation which is keep drafted here so I would like to compute the energy per part of matter that is homogeneously distributed between an inner radius small delta and an outer radius r ok, so what I do I do an integral I do an inter, you see it here between delta and r of in these dimensions d dr which is dx dy d times times rho ok, I take matter homogeneously distributed times 1 over r to the alpha this will be the so in matter here I didn't put interaction let's say it's coupled with interaction j or g or any interaction j ok so so it's very easy to see what happens if there is a spherical symmetry this integral will give you I didn't put the expression but you can derive it can look ah, this could be an exercise what is this quantity here, so it's the angular volume of in the dimensions times rho and then you count ok, this is d minus alpha and you have to estimate d minus alpha between r and d so you get as an estimate of this integral rho j the coupling ok, divided by d minus alpha is a constant is important and then you have r to the d minus alpha minus delta to the d minus alpha ok, now you understand why I have put this delta here because it serves as a regularization of the interaction at short distances because there could be divergencies of this interaction at small delta so for the moment I keep this delta fixed and this is something which is really done in practice in the two examples that I've shown for instance in Newtonian gravity the potential is regularized at short distance in several different ways or the particles when they arrive at very short distance they interact in a different way so they could be for instance hard particles that when they get close they collide or they could be soft particles when they get close they interact with a different potential or matter could be quantum and then at very short distance you will have the effects either of the Pauli principle for instance if you if you take fermions or of the Heisenberg principle because you cannot follow the trajectories and the velocities of the particles when they get too close so I exclude this part it's a phenomenological parameter but what is important is this part here and it is clear that when alpha is larger than d when alpha is larger than d then epsilon goes to a constant when r goes to infinity k when r goes to infinity and alpha is larger than d this exponent is negative and so as r goes to infinity this term drops down and you get a finite epsilon ok this property was realized by Gibbs himself the founder of statistical mechanics it's not easy to find the quote but if you are patient enough and you go to the very first rigorous book in statistical mechanics which is the book of Gibbs you find this remark interaktion should decrease faster than 3 in 3 dimensions and this was known to the physicists to 50 years ago physicists and mathematicians like Michael Fisher and David Ruel in the beginning of the 60s were setting the base for the study of matter using what is called the thermodynamic limit and they realized that they could get thermodynamic potentials in like here we get the energy only if it exists of decreasing fast with distance of the interaction potential was made of course if the decay I've chosen the power law instead of an exponential because of course the exponential would fall for instance Yukawa potential would call faster than the exponential this is a sort of critical situation in which I'm testing the stability of my thermodynamic description ok so most of what has been done in the 60s and the 70s on the on the short range but in case which is alpha larger than d is very interesting but will not be the subject of my lecture course because the subject of my lecture course will be the case in which alpha is less than d or maybe ok I will introduce a quantity which is called sigma which is alpha minus d so and if sigma is positive I'm a little bit invading the region of of the founder of statistical mechanics because you see I'm going in a region where the energy per particle is well defined but I will reach only a value that I call sigma star and if sigma is less than sigma star and the sigma star will be defined depending on the problem and you will hear a lot about sigma star in the lectures by Nicolò Defeno you can get collective phenomena that are due to long range interactions although the system is extensive so although the system of energy per particle is well defined for instance an exercise that I will do pretty soon very interesting one maybe not well known the fact that there can be phase transition in one dimension in this region between sigma star and zero sigma star and zero so phase transitions in one dimension who has heard about phase transition in one dimension is there in the audience someone who knows no so what what would you argue first of all you know what is phase transition I think so okay and there is an argument which is due to Landau to Landau and Leafsheets which tells that if the interaction is short range and I will repeat the argument I will leave the argument at the end of the lecture as an exercise so first exercise check exercise check an expression for omega d and study this expression and see that in three dimensions it is angular volume of the sphere and so on in Italija we say solid angle I don't know if it's spread out in the world this this term okay so what happens if alpha is less than d now let's take over again so what happens is alpha is less than d alpha is less than d that's all equal d and 0 then it's easy to check that the energy per particle it's here is the volume to the 1 minus alpha over d this is a simple calculation the volume if you want is r to the d so you can express the energy per particle both using the volume and using the radius of the region where matter is contained so if alpha is less than d this is less than 1 so 1 minus alpha over d is a number less than 1 I'm not considering alpha negative I'm considering alpha positive and of course I could include alpha 0 alpha 0 is a very interesting case in which each particle interact with all other particles and there is no decay of the interaction so alpha equal 0 is what usually called the mean field or all to all okay the mean field or all to all interaction so, okay what can you do if this happens so if energy is super extensive in the volume so grows with the volume and the solution to this problem was given long ago okay let's first of all try to talk about the physics and then give the solution which is interesting mathematical solution but it's a mathematical solution and I would like to understand the physics okay, usually in nature we have systems that are described by Hamiltonians by energy functions and the energy function is made of kinetic energy plus potential energy kinetic energy in standard conditions is the sum of is the sum of single particle contributions the velocity squares of each particles okay so this part of the energy is goes like n because you are summing contributions of of each part if I'm going to slow, please don't tell me you're going to slow I know all these so I will go faster because there's slides, I have 20 slides and I am now at 9.39 and I have covered two slides so I'm filling up the notions what is not on the slides but it is in the book and I will give you the PDF of the book for free by the way just to relax for a while you see this beautiful picture this is an artist that I met, his name is Neil Sudo from Finland and I like very much his land art this is oranges and he rotated the camera in order to make a sort of cluster of particles and this reminded me the clustering phenomena in self-gravitating system so I asked him can you give me the the rights to put it on the cover and he said, okay, yes and then I said, okay let's get Oxford and tell them you want to be paid for that and then he contacted and lost contact with him and so finally got to be paid by Oxford and then I asked him how much he said $100 I said, oh these Oxford guys these are really bad guys I mean you should have asked at least $500 no, I was so excited that my cover finishes on on a book, okay, but it's I like it very much you can look at the arts of this guy okay this is what my friend Jan Levina from Brazil calls core halo distribution so there are sometimes in self-gravitating systems situations in which they form a core, very dense core and then there is a halo around and you will see that they can arise in much simpler situations okay, let's go back to my Hamiltonian and of course since this is pair potentials because I can square okay, so already there is a problem at this level because if you let and grow and there is no way that you get an energy per particle this part of the energy will keep growing keep growing and keep growing and dominate over the kinetic energy one could say okay, no bad because as potential energy grows matter will get colder and colder and finally it will reach zero temperature because kinetic energy will be extremely small with respect to to potential energy so do you see around that we are all at zero temperature? no, I would say no okay so in fact what happens is that as you increase system size because of short range interaction the system is chopped into parts and equilibrium will be an equilibrium with zero temperature because of that because kinetic energy can compete with potential energy but if you don't have additivity which is the first hypothesis that you find in any book of statistical mechanics which is a consequence of the interaction to decay faster than d you won't get the equilibrium that we see around us because the energy will dominate and kinetic energy will be dropped off and also you could not see boiling water you put fire under a pot and you would like to see water to boil and then to become vapor so to go through a phase transition and this you cannot appear because the system will be dominated by energy and entropy will not play any role in the matter so it won't be able to compete with energy because again entropy which is combinatorial grows with n and another consequence of this effect is that since free energy is u minus ts u goes like n squared s goes like n and the system will be dominated by energy ok so you won't see phase transitions so what was the idea and the idea is due to fantastic mathematicians that I encourage to read the biography of this guy which is really impressive so he was born and lived part of his life in a country which is nowadays in big trouble he was known to the mathematicians in Leopold in Lviv or Lviv in now in Ukraine at that time was part of Poland and then emigrated to the US and he was I mean he is responsible for so many contributions to random process Feynman-Katz integrals and so on this is really a minor contribution he got a very strange and funny idea so ok, if the energy is so there is energy per particle go like this so the energy is N time this and you can rewrite N in terms of volume so you see in this slide that if alpha is larger than D as I was telling the energy goes like volume if alpha is smaller than D the energy goes like volume to the 2 minus alpha over D energy now I am playing with extensive variables but I will follow the rule that A is an extensive variable and A is an intensive variable so I will try to keep the 2 definitions during all my talk so the free energy goes like the volume because the entropy goes like the volume the energy goes like the volume everything is ok if alpha is larger than D but what can I do if alpha is smaller than D and what cuts propose is to rescale to rescale the coupling to rescale the coupling in such a way that you get a free energy that increases with the volume and that's a very simple exercise just rescale the coupling I don't write it it's called the cuts trick it is a mathematical trick you rescale the coupling by V to the alpha over D minus 1 and if you do this you get a free energy that goes like the volume alternative what could you do you could rescale the temperature ok by 1 minus alpha over D in such a way that the free energy now grows like 2 minus alpha over D it grows like the energy so it's an unusual scaling for the free energy but it allows the temperature which now depends on the sides to reach the scale of the energy of the potential energy so I believe that you are not used to neither of both so where is in nature an interaction that depends on the sides that's why it's a trick and on the other hand if you measure temperature with a thermometer you believe and we have a thermometer at the entrance of the building you believe that this does not depend on the sides of the body to which the temperature is measured ok so both are tricks and why you do these tricks you do these tricks because you want to go to the thermodynamic limit without encountering the problem of competition between kinetic energy and potential energy and without encountering the problem of lack of competition of entropy with energy ok but then you know that also the thermodynamic limit we are made of moles of matter so none of us I invite you to compute how many moles you are instead of kilos but none of us is an infinite number of moles so you can play the cast trick at the reverse once you get a very very large system you fix the size of the system and you read back what are the intensive variables in terms of extensive variables given the volume given the finite size of the system so that's the idea you do the trick in order for the limits to converge it's a typical mathematical trick and once you reach the limit with intensive variable you fix the size and you read back the extensive variable of the system this is the idea this is the conceptual idea it has been done very successfully even more sophisticated ways for instance for the theory of liquids there is a very important series of papers mathematical papers where which is by the way the only way of getting phase transition rigorously in liquids ok, so but I don't want to enter in these so I've put here the slide to be more specific on another feature I mostly spoken about about extensivity so the fact that I want to increase the number of particles the volumes in order to get the density and so on but I didn't speak about another feature of which is in fact even more important now that we are able by the cut streak to perform the thermodynamic limit I think I will stop at 10 and then I will do 5 minutes break ok, so be prepared for stopping 5 minutes you should resist and accept the cut streak for a while and then you will destroy it ok, in 5 minutes ok, so and this this property has been in some sense it has been confused with extensivity so if you open a book in Statmeck the two concepts are sort of superposed so ok, if it is extensive it's also additive I would like to make an example very simple example can be more complicated examples the simplest you can think where you see that they are not the same ok and the simplest example is the Curivice Hamiltonian I leave it on there so the Curivice Hamiltonian is the simplest model of magnetism that you can think of spins can think of them as plus and minus variables classical variables interact all to all and I have put the cut streak in this Hamiltonian can one see where is the cut streak in this Hamiltonian there is cut hidden somewhere in the J over N because I have just said that the cut streak is to scale with minus alpha over D and this is a mean field all to all model so alpha is zero in the interaction so I think all of you have been presented to the Curivice model reading books of Statmeck but no one was aware that there is a cut streak in this Hamiltonian and no one was aware that this is an example that contradicts chapter one of the book because chapter one begins by saying we will treat in this book systems that are both extensive and additive and this is extensive for sure because the Hamiltonian grows like N the number of pairs grows like N squared divide by N Hamiltonian grows like N but it's very simple to construct states you can play with that I have constructed the simplest one I construct a state with zero magnetization zero magnetization so the sum of the spins is zero this Hamiltonian can be also written as magnetization squared so if the magnetization is zero also the Hamiltonian is zero so the two parameters magnetization and energy are tightly related into this model and I divide the system in two parts and it's very simple to see that the energy of the total which is zero magnetization is zero while the energy of the parts is minus j over a10 you can do the exercise of computing the energy in case of the two parts and hence the sum of the energies is not the total energy of the system even if you go to very large N you will not solve the problem that's because as you grow with the size of the system there will be cross links between the two parts there is no surface in this model there is no surface in this model because there are old cross links so that this is not true so yes yes yes sorry I was too fast it's not in the denominator anyway you can check it might be a mistake so please check I'm sure that it's not going to zero minus j minus because in the Hamiltonian which proves that ok then you say oh that's a disaster because no one did this remark to the teacher look this example contradicts chapter one of the book but there is no disaster fortunately and Katz was right and that's a very very interesting the model has been studied also mathematically and gives a phase transition of second order of the Q revise type, mean field type which is a good description of what happens in magnetism in this limit of the mean field now you will learn at the end of the of the series of talk maybe already on lecture two that we have been very very lucky to use spins that can take only two values because if we would have used spins that can take three values would have come in big troubles and in particular you will see that this is already an example it's called the POTS model where which describes some mixtures, some other different systems and magnetics also some magnetic systems that the entropy I mean thermodynamic entropy entropy as a function of energy is non-concave so for this case is in extreme situation where the entropy although there is a second order phase transition the entropy remains concave and I will compute the entropy for the Q revise model you will see it in many different ways and the entropy remains concave so all thermodynamics works although the system is non-additive so it's not necessary that thermodynamic works if the system is non-additive so it can happen that if the system is non-additive you get standard thermodynamics there's no problem with thermodynamics but there are cases and I will show several where if you violate additivity non-concave entropy and this is the case of this is the right time to finish self-graditating system one component plasmas oiler equations and many others so in the second part of the talk I will go on with the slides and now I leave 5 minutes of break you just sit or questions first of all questions, yes I would like Angelo, are you there? Yes, yes Can we have Can you hear me? Can you hear me? Yes, I can hear Angelo From Angelo Can we have the audio only from your computer, right? But we here we can hear Hello, Angelo But if you open the audio Hello? No Maybe Hello, Angelo In the hall, can you hear in the hall? Not quite Maybe this one Hello? Just a moment Angelo Hello, try now Yes Very good, great Ok, thank you very much So, my name is Angelo Rose I am organizing with with this spring college So today I couldn't be there with you because I am recovering unfortunately from a small accident but so what I want to tell you that I am working in CIS and so we are organizing a visit to the CISA labs of Neuroscience that will be for the third or fourth week of the spring college so that will be in March so I will let you know and maybe I will coordinate for sure I will coordinate with Matteo to arrange the visits in safety so probably I think it will be two groups of people so to not get I mean to avoid big gatherings and to know about that and enjoy the school and the speakers I think it's a really fantastic opportunity for all of you, thank you Ok, thank you Angelo Ok, so we take 5 minutes break


Lindsay Lohan was always one of my favorite Disney stars growing up. She was known best for being an actress and singer, and now she's also a reality star and businesswoman. Her series Lindsay Lohan's Beach Club premiered on MTV a few months ago in January, and it documents Lindsay launching her club, the Lohan Beach House in Mykonos, Greece. From watching the show, you can see just how much Lindsay has changed from her beginnings in Hollywood. Lindsay has ended up as a center of drama pretty often, be it arrests, rehab stints, you name it. However, in this video we'll be talking less about all of this and more about her transformation over the years. We'll look at how her once Disney image has changed. What's going on guys and girls, my name is Cara and this series we've titled Before and After. We're going to talk about Lindsay's hair, body, any work she's had done, and more. I've done other celebrity transformation videos on the likes of Ariana Grande and Trisha Peitas, and we'll have links to those at the end of this video. If there's anyone else who want me to document, let me know in the comments down below. Now let's get into this video. Lindsay has been out of the spotlight for some time now and she looks a lot different these days.  She's in her 30s now, so it's a given that she would look older, but I think she looks different more so because of the work she's gotten done than simply age. Although Lindsay has denied getting any plastic surgery, her face looks much different from a few years ago. While starring in Mean Girls, her face looked healthy and fuller. Her features such as her nose and eyes didn't seem to change since then, so I don't think she's gotten any invasive surgeries. However, it would appear that she's a fan of fillers.  This definitely would affect the way her face looks, but it isn't all that's going on here. It's obvious at least to me that Lindsay has gotten Botox or some type of fillers in her cheeks because they're much puffier, smooth, and higher up on her face. You can also tell that Lindsay has gotten lip fillers as well, especially when looking at her top lip in some photos. Her cupid's bow on the upper lip isn't as defined, which is often a result of too much filler. Lindsay's face in general appears more frozen now in my opinion, so I'm not sure if she's gotten fillers anywhere else. Now let's take a look at Lindsay's body. Since her early days, her body has changed a lot and she definitely lost weight. She looked great as a teen star and still looked healthy. After her huge success in Mean Girls, she started leaning away from her Disney girl image. When she debuted as a singer post-Disney, it was hard not to notice her chest in her music video for rumors. Lindsay's chest size was seemingly natural as she was still pretty young. She definitely was known at the time for this and it helped her get rid of her good girl persona. There was obviously speculation about whether or not Lindsay got a boob job. In 2004, she denied any of these rumors, stating, I'm 17 years old, my mother would never let me. I'd be deathly afraid and it's unnecessary, but I'm glad people think I have a nice chest. I believe that. But with Lindsay's rising fame like many young female celebrities, she started to lose weight quickly. Around 2005, 2006, Lindsay got a lot thinner, even scary skinny at one point and it's safe to say that she lost her curves at that time. Since then, her weight has gone up and down a lot, but she does seem to have her boob back. It's been a while so I'm not sure if she's gone any implants or work done in that area, but if she has, she hasn't admitted it. The star's body size does seem to fluctuate a lot, but there could be many reasons why. It's been known that Lindsay previously had struggles with drugs and partying, so these could have been significant factors in weight change. Now at age 32, she looks like her weight is more stable and healthier. Her time living in Mekunos may be doing her good. Moving on to Lindsay's hair, Lindsay is a natural redhead, which I believe set her apart since the very beginning. Her red hair all over freckles and green eyes were kind of like a signature. But after Mean Girls, Lindsay began to experiment with her hair like most of us do. Way back in 2004 when her first album Speak came out, she went for a darker reddish brown hue, which I really liked on her. She then went blonde for the first time the year after, and then tried out dark brown in 2006. Ever since, Lindsay has gone between shades of blonde, reddish hues, and back to dark. These days, while she's back to her roots with red hair again, and I think it looks great. Being famous since she was a little girl means that we were able to see Lindsay's fashion change with the times too. As a child, she looked cute and stylish, and she was clearly already used to the spotlight. The star embraced all the trends while she was a teen, as we can see from her red carpet outfits back in the day. I actually really liked this one outfit and always wanted that top, even though low-rise jeans are so yesterday. In fact, I think some of my fave Lindsay outfits were from years back, and they were actually super cute, in my opinion. It's clear that Lindsay is no stranger to dressing up for the red carpet and being photographed, and she'll probably always be ready to get glammed up. These days, with her new show and being a boss, Lindsay also seems to be sporting some sophisticated looking outfits and suits too. Lindsay has changed her image plenty over the last decade or more. I mean, she even has a handful of famous mug shots, which somehow she still looks good in. She's had her fair share of struggles, and it's got to be even harder when you're constantly in the public eye. Her style and appearance has definitely evolved to say the least. From the innocent child star we were all introduced to way back when. I'm not sure if Lindsay has settled down in her 30s by running her own beach club, or if she still likes to have fun and party like she used to. I just really love those clips of her dancing. But hopefully, she keeps looking good and staying out of trouble. All right, guys and girls, that wraps up this video here on Before and After. If you want to talk more about Lindsay's transformation, you can hit me up on Instagram. Let me know who else you would like me to make a Before and After video on, and I'll see you guys in the next video. Bye.


I think certainly in radio documentaries I made in the past I felt like you were often encouraged to take yourself out of the picture, you know, particularly in the BBC because of the nature of them having to be an impartial organisation. You find yourself reporting rather than experiencing, you know, so like, you know, you go somewhere and you report the facts as you see them and it's all very much about sort of providing the evidence to back up. You know, you're not really making an argument, you're showing something and you're using evidential stuff to show that picture, you know, so you say like here's the professor I've just found and here's the, you know, expert on the stuff and these people all show that this is how things are, you know. And in making podcasts, you know, it's very much about this kind of going on a journey and experiencing things and how you respond to stuff is incredibly important because that is shaping and informing how the audience feel about it and it's kind of, it's okay to express views and opinions and you can do that. The thing I've loved most about making podcasts is that sense of building up a community. We've haunted, it was just lovely to kind of see, you know, this thing growing and people talking on Twitter about it and coming on board and sending emails about it, sending their own ghost stories to me and also having opinions on stuff.  Here's a YouTube video ball lightning. It could have been ball lightning. And I love that and the kind of conversation that grows around stuff.  And, you know, I think that's great. And I think like, it's a nice idea that this isn't just your thing. It's kind of, it's collectively owned by all these people. And you're the one making it and putting stuff down on tape.  And so they all feel an ownership of it.  And if you can break into someone's kind of core listens, then you go like, yes, great. That's Danny Robbins. And this is the podcast producers podcast with me, Neil Mossy. It's a place where podcast producers share their tips and experiences so that everyone can start a podcast and keep going. There's details of how to subscribe in the description. Thanks so much for getting to this point in the podcast. And thanks again to Danny, the links to him and his podcasts are in the description. And if you've got this far into the podcast, it's really good to have you here. Why not give me a thumbs up or a comment or tweet me. It'd be lovely to hear from you. And there's also details in the description for where you can find the next episode. Can you please help my daddy get 1000 subscribers? Just click on his face. Thanks. Bye.


. All right ladies and gentlemen, well once again got about an hour and 15 minutes left in the show. We're approaching the last hour of the show pretty quickly. I would have loved to at least get that capstone pack done tonight. That's going to help sell out because we got to do two of these fillers, right? It's break 75 and 76. If we can get at least number 75 done tonight, then I can load up 76 as well. And then we can finish that off tomorrow. That new Fanatics promo is pretty crazy. I mean that mixer that's on the site right now, that's on Fanatics Live right now, is a good way to hunt for some of those things, I think. I actually don't know the details. Is this just any Steph Curry Superfractor from any break? These must be from specific breaks, right? Some of them are like the Corbin Carroll, right? That's out of Bowman's Best. Well, yeah. I'm assuming that these have to be pulled in a break that you're in, right? I'm assuming this has to be pulled on a Fanatics Live break. So yeah, the card would obviously be yours if you have that. And then get $10,000 of break credit to Fanatics Live. That'll go a long way for a long time. I would save it for the high-end stuff. Are these parties from a certain product? It's a pretty awesome promo, though. Pretty awesome. Right, yeah. I don't think they're going to be giving away $10,000 of break credit if we pull it here on YouTube. All right. I'm also going to might as well put 2019 NT football into a filler, I guess, kind of in sitting at 16 for a little bit. These teams are a lot cheaper than 2022. So even with a lot of teams, it might be still might be a little bit more affordable. Excuse me, there's the filler for 2019 NT football. I'm just my test guys at least an H1 block. The XList can do your taxes online. I've never won anything in my whole life. You used to make a switch. I have an H1 block taxable. Do your taxes in person or online. Okay, see it. Continue. The situation of the slide just continues to go. Just go out of 10 minutes. A different situation perhaps. That's what the word really means. The trailer by two is opposed to any by two. The home center in Colorado to start the free game. Care to play in the ambulance one day. Okay. Sits in. Everything, everything, anything. Increase the pace of the game. Lots to do. Lots to do. Lots to do. You can, you know, accept you in the same time. You can run for a long time. You can face the game. You've never seen all of this before. You can run with your, with your interest in doing it. Alex, a pair of hair. Just under two minutes left in the third. All the kids are here. Going on a government morning. This evening. Yeah, any time of the hour.  Just two months over two years of hanging Passes in time. The answer is he The answer. Put this game. The game's like most games, but I need someone to share a small amount of that matters. The game's on the way to get this next round, they do. Yeah, got more money to see, it's 31, it's 31, you get that crowd back into the game. You get the momentum going, you know, you break back to change, right? This guy starts 1-0, no sense, Cassey, they're on the perimeter now. Right again to the inside, get it on down, starting out 1-0. Right into the man, right into the ground, there we go to do. Two halfs, sit back inside, hit, there he goes. Alright, thank you very much. From a turn one to the drive for a downy, downy along the wall. Works out the right field, but it's one, right to the circle. On the stick, it's long on contact, but if it's hit to the hands, as you see the extension of the stick, way out the front, toward near the body of Kepa, he's reaching up, close to the wall. Look for a shorty, they have the opportunity to sit, and any opportunity they get, the kids have to be aggressive again. Maybe they can even hit it. Alright gang, well we are in the last hour of the show. I'm going to try to at least get, here's what I'm going to do. I think we can do this in the hour. I'm going to take out six spots out of there, and the final six spots will be buy one, get one. That's tonight only. Why did the cat abandon its kitten? Oh dear. Alright, I'll bite. Why? Why did the cat abandon its kitten? So this is just for the people listening right now folks. Last six, buy one, get one. Buy a spot, I'll add another spot for you. Buy a spot, add a spot. Buy a spot, add a spot. Because it wasn't perfect. What a terrible parent that cat is. Awful. What an awful cat. Cats are mean. And hopefully this will be able to get the break done tonight. But buy one, get one. Be smart. Get a spot. What am I, what am I guessing Eric? Yeah cats are terrible. Don't tell me later, okay. That's your prerogative. Rex and his cat joked right meow. Ladies and gentlemen, buy a spot. I took, there's 12 spots left, right? I took six out, buy one, get one. This should sell it out, right? Then I could post the last filler for that hit parade. Let's focus. Don't, let's forget about Rex's cat jokes. Let's focus on this capstone. Not cat stone, capstone. Ah, that was a joke. Didn't realize that was a joke, Eric. Thought jokes were supposed to be funny. Got him. Got him. So get into that cat stone baseball, ladies and gentlemen. It's buy one, get one.  I mean, I don't know, I'm giving spots away. Literally. Buy one and you get one free. And this is tonight only. Yeah, you're funny too, Rex. Funny looking. Got him again. Got him again. Who's going to get this? Last six spots in capstone tonight only. Buy one, get one. And we should be able to sell it out. There's got to be six people to get, I mean, there's Eric. There's Rex. There's Oliver. That's three spots right there. Buy a spot. I'm giving you a spot and two spots. Buy one, get one.  And then I can load up the last one. And we should probably be able to fill that up tomorrow. But let's get at least this done tonight. Buy a spot. You get a spot for free. Get an extra spot for free. Buy one, get one, ladies and gentlemen. And we can do the break. This is tonight only. We are giving away nothing. Everyone's like, no. Nobody wants a free spot for getting a spot. I mean, no good deed goes unpunished, ladies and gentlemen. Come on, hockey kings. I don't need to upgrade to premium at block, but thank you. Give it away a spot. Buy one, get one. No one's going to take advantage of this, huh? I'm trying to give away spots. And people are like, yeah, we'll just pay full price for it tomorrow. Which I guess I appreciate. Who's excited about Masters of the Air? Masters of the Air? The Air? From the makers of Band of Brothers, which is probably one of the best mini-series that are out there. Masters of the Air, Apple TV, starts on Friday. Looks good. Looks almost as good as that buy one, get one in that capstone. I think that'll make it clear in the chat as well. Buy one, get one free.  Let's not do that. Buy one, get one free, boys and girls. Six, there were originally 12 spots remaining. I took six out. The second someone buys a spot, I'm giving them an extra spot. Tonight only. We got 45 minutes left. Yeah, that warrior ceremony was sad.  If we sell this out all over, we'll get golf talk going. Right now, we got buy one, get one talk going. Buy a spot in capstone, get another one for free. Just automatically. You don't have to do anything extra. All you gotta do is buy a spot there and your name gets added in twice. Buy one, get one. It's pretty easy. Nothing, no really extra work to do. Just go to jaspyscasebreaks.com. Click the link in the site. Buy one, get one. Buy a spot, get another spot. Just like that. There's this free spot for you, Eric. You gotta buy one and that'll give you a free spot. Easy, easy. Buy one, get one free. Someone's gotta buy at least one. Steve? No, Steve gets the Lions in 2022 NT, which is fine. But that's not a buy one, get one. Capstone pack, buy one, get one. And if we, I just need six people and then we can do that capstone break. Give away some hit parade spots. You might stumble into a nice hit parade spot for a fraction of the price. I could load up the last filler and then we can work on that hit parade tomorrow. I appreciate that, Oliver. But the buy one, get one is with capstone baseball, ladies and gentlemen. Buy one, get one. Trying to give away spots. No one's like, ah, we don't, I don't want to win hit parade spots. I don't want to get one free. Gotta find, there's gotta be at least one person who wants to get an extra spot. Try to win their way into that hit parade break. That's great, Eric. But right now, we're trying to buy one, that's right. And Espanola as well. We're trying to get someone to buy one and at least get, no, it can, at least one person has to take advantage of this, right? This is tonight only, you know? Now, Michael Jaspie is an employee, cannot join in our own breaks. We're talking about people that can't buy into our breaks. We got people watching that are crying poor. They can't buy one, get one free. There's gotta be someone else out there who wants to buy one and get one. Who's out there? Buy one, get one. This is all I'm gonna do for the next 40 minutes. Buy one, get one. In that capstone. I gotta find at least one person to buy one and get one free. You know? Si. All I have to do is Compre uno. But nobody's compre uno right now. Buy one, get one free. Easy. Es fácil. One spot. There were once 12. I took out six. And for the last six spots, if you buy one, I'm gonna give you one free. I'm gonna add your name there. Buy two, you get two. Buy three, you get three. You buy six, you get six. And this will be a good little late night rally just to knock out this single pack right here. Give away some hip rate spots and get us one step closer to getting that break done tomorrow. You know, let all the squares buy them at full price tomorrow. You're sharp. You're gonna buy one and then you're gonna get one. Be sharp. Don't be a square. Let the squares pay full price tomorrow. The sharps will buy one, get one tonight. Who cares about tomorrow Rex? Tonight is buy one, get one. Tomorrow full price. And back to full 12 spots. And we can get this pack done. Give away some hip rate spots. Load up the last feather. We gotta do one more of these. Wanna get at least one more tonight. I'm feeling like we should buy one, get one, Oliver. That's what I'm feeling. I feel like if James Paxton was here, he'd buy a spot and get one free if he's healthy enough to buy spots. If he's healthy enough to buy spots, he'd be pretty effective in this group break. So I feel like the Dodgers have another trade in them in there somewhere. I don't know, I feel like it's not like Paxton's injury history is really is clean. So I'll bet that's just seems like more of a depth move. I can't imagine that they're thinking that that Paxton will be healthy all season long. I don't know, but I guess there'll be a lot of... I don't know. Yeah, it sounds like a classic, yeah, Dodgers reclamation project.  They know good value plays. Like this value play right here. So I think the Dodgers feel like they're still a trade in them. Maybe they'll wait until the mid-sees. Maybe that trade is not going to happen. I thought maybe Dylan Cease, but now I'm thinking they'll probably just pick up some of these reclamation projects, you know, try to see what they can get out of them and then reevaluate by the trade deadline. Because I would imagine they'll get a clearer picture of what Walker Bueller is going to look like, what Dustin May is going to look like, what Gonslin is going to look like, how their arms are going to look in the middle of the season. And if... And then we'll see how the other pitchers, you know, remember, the glass now pitched a, you know, his career high in innings last year, which wasn't a lot, which is like 120-ish, which is not a lot. So he's going to suddenly bang out 200 innings, 220 innings, work-horse tile innings? Probably not. You know, does Bobby Miller progress or regress a little bit, which as a young player, could either wake and happen. I think long-term he'll be fine, but we'll have to see what happens with him. So there's actually a lot of questions with the pitching staff. Yeah, maybe six-man rotation happens. Might as well get used to it, and that's what's going to happen when Otani is around, right? So we'll see. Obviously, a regular season they'll be fine, but I don't think they're going to make... They shouldn't make the same mistake they made last year. I think at the trading deadline, they have to go for whoever the bonafide pitcher is that year, if they're on an expiring deal or something like that, or on a bad team. Like, if the Brewers are terrible this year, right? Which I'm kind of hoping. Sorry, Brewers fans, because I think the Dodgers have the pieces to get a Corbin Burns, for example. You know, I think that would be great. And the pitching will still be an issue for the Dodgers. They won't go very far without that. The Barnes firm, this jingle is terrible. What happened to Salino? What happened to Salino? This personal injury commercial used to be Salino and Barnes. Now it's just the Barnes firm. Where did Barnes go? Where did Salino go? Did a mysterious injury befall Salino? Why is Salino and Barnes splitting up? Oh no! Salino sued to dissolve the firm in 2017, citing a breakdown of his professional relationship with his business partner, Steve Barnes. The Barnes firm was launched by Rich Barnes, Steve's brother after Steve died in a plane crash in 2020. That sounds really shady. I feel like this Salino definitely made that plane crash. Wow. Barnes along with his niece killed in a TBM-700 single-engine private airplane in New York. Wow. That sounds very mysterious. I think Ross Salino might have something to do with this. Whose last name is shady? Salino or Barnes? Rex with classic prejudice against Italian Americans, upstanding Italian Americans. Last name ends in a vowel, must be a mobster. You're part of the problem, Rex. I thought that racism against Italians was gone by the mid-60s, but no, alive and well in the backwaters of Indiana. Where that anti-Italian sentiment still thrives in Indiana, I guess, Rex. Oh, can't be. I love Tony Danza, says Rex. Wow. Wow. He's going with the windy. It's like when people go, how could I be a massage? How could I hate women when my own mother's a woman? Some of my best friends are dot, dot, dot. Dang. It is Jason. Classic, Rex. Classic. Also, we got to buy one, get one, ladies and gentlemen. Last six spots in this capstone pack, buy one and get one free. And that, if we can get six people going with that, or if a few people get multiple spots, we can finish off this pack tonight, rip the pack tonight, add the last filler so we can get that done tomorrow. Jason will be on here tomorrow. Does the YouTube emoji, do they not have like a hat or cap? Wait, what did you, what did you type in for that? And anyway, there's, there's a graduation capstone. All I get is Capricorn. Anyway, there's a graduation capstone baseball, buy one, get one. Let's make it happen, folks. We've got 30 minutes. Well, let's put it this way. I've only seen one order in the last, I've only seen one order in the last 45 minutes anyway. So we'll give it another 10 or 15 minutes. And if we don't sell, I mean, if we don't sell a single spot here, then we'll call it a night a little early and we'll add those spots back in. Not even one person. I thought one person at least get a, get a spot for free. We're here in the week about the memories you have from this tournament, you made your professional debut 10 years ago right here. What's it like to shoot 67 for the farmers here this year? Just really happy with the start. It's tough to finish with the bogey in a last hole, but I'm happy to get off to a good start and within striking distance. But tomorrow is the southpaw. So we'll have to play, play probably even better tomorrow. Your former college teammate, Max, so one of the defending champions, Gracie, you draw from then seeing what he's achieved in this game. A ton. You know, he's had his fair share of ups and downs like I have, and to see how far he's come from those downs is very inspiring and hoping to, you know, get up to or either. How does this golf course change from how you remember playing the heads of junior 10, 15, 20 years ago? The golf course changed a ton after the redesign. Some of the grains are completely different than how I remember it, which sometimes kind of confuses me at times. But the southpaw course is really similar and you've got played enough tournament rounds here now at the Farmers that I feel really comfortable. Staying with mom and dad this week, are they still tough on you? Great tough. But they're very supportive, I'm sure. Always good to catch up, keep you going, Michael. Let's go back to you guys. I'm talking about a truly old town event with a high school just down the road from here at the same name of the golf course. Touring by Michael Kidd, off to a nice start. It was just the regular bottles. What's up? Can I present all dams of 2 degrees? I needed a vertical. So I lost strength to wear a marvellous hat. It was such an immediate hit. Hey, is this a circle? Let me see that. So, I got the hope to tell you. Have you even said one back? What about the future? I'm gonna need an address and a set code. Okay, if this is what we did for the schedule, see what we can do for your business. Then X. Every shot has its own unique feel. The trick? It'll be comfortable with each one. If you want to, I can go and come back into a very DNA or something like that. Our justice material provides supreme comfort and durability while our fingerprint technology creates a strong connection and unforgettable touch. The game trainers you've tried to show, the failure hand, children, lack, and illusory. The symptoms of E-cell treatment for RMS that have powerful results are reduced rate of relapses, have depletions, and slow disability progression. I'm taking my son for two months that's all we've got to do. And I'm ready to take his symptoms if you have hepatitis B and tell your doctor if you have had it as it could come back. They did it. They did it. The symptoms are serious symptoms. All right. That's all we got. While no cases of PNR were reported in RMS, I'm glad you told us they couldn't have it. Tell your doctor if you had it. Oh, I didn't.  I think we're good at this. The symptoms they cause a decrease in symptoms in many ways. The most common side effects are the relapses of choice. So, I'm probably holding that. That's all I'm trying to tell you. Hello. The symptoms in my life. So, how I feel like I have had it. I think it's up to you. Tell your doctor if I like to sit. It's up to you. All right. Swamp. That mixer is going to be fun. I got the schedule cleared. Do-do-do-do-do-do. I've got something on the bed. I'm just going to open the safe. It's your other shirt. Yes, Mark. Play that, Greg. Put the box in there so it sleeps. And then I want to put the big holes around it and feel a little light. At the 7th, Kevin, you will be sauteed. Lift on and arrange yourselves right now for anything. This is what I'm wishing for. This is at 13, Min-Woo Lee, played his way onto the PGA Tour. It's going to be a star. This is for evil. Face. That's for giving distance. Play big. With the only launcher, XL2 driver. This leaves him golf. Ultimaris is for adults who have generalized the necrographis who are anti-acidiculin receptor and antibody positive. It is lasting control over GMG symptoms. And Ultimaris is the only long-acting GMG treatment with eight weeks of freedom between infusions. Ultimaris can only read system's ability to fight infections, increasing the chance of serious, like-looking meningococcal and other types of infections. If not bouncing in, we must receive meningococcal vaccines at least two weeks before starting Ultimaris. And Ultimaris is urgent. We should also receive two weeks of antibiotics with your race. But before starting Ultimaris, do you want to adopt all of your medical conditions and medications? Ultimaris can cause renaissance. Tasty leaveers are covered in carrying pics from the swallow. Seven hundred with at your can. The can has got a significantly colder up here over the last half hour. Forty-five days. I swear to God. What was six years and seven hours around the North versus North? Fourteen? Dan Marine Leaders have been there all day long. There's feedouts every time you're here. What do you think? That's a real praise. So all the time you guys speak a little about it. Thirteen now. Here it is on the T40. Because you walk two shots for the ride. You go to the T-Shop without driving technology. It's presented by Paradigmote driver Calaway. And so on. And so on. And so on. And so on. And so on. And so on. And so on. And so on. And so on. And so on. And so on. And so on. And so on. I think they're really good! Do you want to call that? Hey cast! The first time here in six years from dürfen remal When was the first staff here at Mind tweeted 66 How did you characterise your staff? Was everybody there? The most good I anywhere in the area is here north right. I know you were welcome to فهههه they used the staff who's here Riley pilots minutes were hard so I don't have conditions why this And of course, I think that the opportunity to get a lot of things, this could be the data, the hold up that board. And so, starting beyond, like I said, I was just trying to be, you know, I'm starting to be, you know, the members of all the law enforcement, you know, I am, I'm just starting to focus on taking justice and getting it. And I mean, I didn't know what that was. Yeah.  Just the same thing, you know, it's just a new data model that she's today, where they're going to make money, just trying to show us what's going down, give everybody the kind and make these boards. That's great. If it's not, you just move on. All right, guys, we'll see you. I'll see you on Friday. Jason will be here tomorrow. We're switching, Jay. Jason's going out of town on Friday. So let's fill up some more breaks tomorrow.


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it's Care The Vampire Slayer back with another exclusive house tour here on Famous Entertainment. And today we're checking out the homes of Sherry Sheppard as well as what that part of her life is like behind closed doors. Don't forget to like, subscribe and hit me up on Instagram to chat. And now, let's get into this video. At the offset of their relationship around 2012, Sherry Sheppard and her former husband Lamar Sallie couldn't have appeared happier. Not only did Lamar embrace being a stepfather to Sherry's then-7-year-old son, Jeffrey, but together they moved into what Sherry considered to be her dream house, a nearly $2 million home in Allendale, New Jersey.  Meanwhile, on the inside, the living room included wooden floors, high ceilings and a ton of open space. The kitchen offered custom cabinets with marble countertops and an extra-wide kitchen island with optional bar seating. Sherry and her family could share their meals in an elegant formal dining room with a chandelier hanging down from the ceiling, which sat overtop a somewhat unusual marble dining table. Upstairs were three bedrooms with a spare office including Sherry's master suite, which offered enough space to include its very own cozy sitting area in the corner and a sleek looking en suite with a deep set soaking tub as well as an all-glass shower stall. And on the very top floor, you could find a guest suite with its own little kitchenette as well as a few different plush leather couches to relax on. Finally, down in the basement, Sherry and Lamar set up their own home theater with a screen projector that's adjacent to a nearby game space. But what might have been the biggest highlight was this gorgeous backyard that included not only a classic-looking swimming pool but a canopy seating area and an accompanying web bar for all their entertainment needs. Picture perfect, right? Well, it sure seemed that way for about two years, but then everything changed. In 2014, Sherry filed for divorce from Lamar, leaving him floored and heartbroken. And not just because their relationship was coming to an end, but because the couple were only a month away from having a surrogate deliver their newborn son. It would later be revealed that Lamar, a former TV writer and occasional school teacher, never had his name added to the deed of the home he shared with Sherry, and she wound up putting the home on the market herself after giving Lamar the boot and sending him back to LA. Sherry would then eat a small loss when she sold the property for around $1.72 million, which was roughly $100,000 less than what she originally spent on it. After getting rid of the house, Sherry continued to shore up her finances and told Lamar that she wanted nothing to do with the child, even going so far as to refuse to pay child support. When the child was finally born, Sherry never made the trip to meet him, but she did manage to trek all the way to court in the hopes of exempting herself from any legal or financial responsibility. Despite that, the court actually ruled against Sherry, and following a denied appeal, they ordered that she must pay around $4,000 a month in child support until the boy is 18 years old. I don't know about you guys, but that wasn't the kind of story I was expecting to find. It's crazy how fast things can go from picture-perfect to a nightmarish scenario just like that. At the end of the day, this type of behavior just wasn't what I was expecting from Sherry, largely because she generally presents herself as someone who's very caring. After serving as Wendy Williams' season-long guest host, Sherry Shepherd was given the opportunity to host her very own talk show for this upcoming season, titled Simply Enough, Sherry. The show is set to premiere this month, but in order to embrace this new opportunity, Sherry had to pack up the life she'd been living in LA for these past couple years and head back to New York City. Rather than simply handle all of this on her own, Sherry made something of a spectacle of her cross-country move, with the help of the Hertz Moving Company. She packed up her belongings in Los Angeles and had them driven all the way to Manhattan. Once her belongings arrived in New York, Sherry would once more let go of her past by handing out a ton of her former household items to people on the streets. She explained to People Magazine, You want to hold on to everything, but what I've learned is that you have to let go of things because if you hold on to the past, it doesn't fit into the new space of energy that you are living in. I gotta say I get what she's going for with that sentiment, but that's definitely not how she treated her former family. Anyway, Sherry handed out a ton of furniture, shoes, clothing, and even appliances after she posted up at a Hertz location in Manhattan. After giving away so many of her former belongings, Sherry then moved into a brownstone that she owns in New York's Harlem District. I believe it's a property that she's owned for at least the past few years, but unfortunately outside of an appearance on HGTV's Celebrity Holiday Homes, which is also nowhere to be found, Sherry hasn't given us a taste of what this house looks like. But once she's all settled in, hopefully she'll open up and share some of her new surroundings with the rest of us. Well, that's gonna bring our Sherry Shepherd house tour to a close. Let me know what you thought of where she used to live in the comments below or more importantly, if you knew about that story about her ex-husband and son. I sure didn't. Thanks for watching, hit that subscribe button if you haven't, follow me on Instagram to chat and I will see you all in another video. Bye! In these videos, we don't reveal any addresses, and even though I've done a house tour of my own place, please do not show up at any private residences because it's not safe for anyone.