- published: 02 Feb 2011
- views: 3445
- author: ICTP PIO
62:15

Cumrun Vafa, Topological Strings and Their Diverse Applications (Strings 2012)
This talk was given by the influential theoretical physicist Cumrun Vafa at Strings 2012. ...
published: 04 Feb 2013
author: Jason Payne
Cumrun Vafa, Topological Strings and Their Diverse Applications (Strings 2012)
Cumrun Vafa, Topological Strings and Their Diverse Applications (Strings 2012)
This talk was given by the influential theoretical physicist Cumrun Vafa at Strings 2012. This talk the applications of topological strings. Numerous papers ...- published: 04 Feb 2013
- views: 333
- author: Jason Payne
60:02

Strings and the Magic of Extra Dimensions - Prof Cumrun Vafa
Cumrun Vafa Harvard University, MA 05 Jun 2013 Faculty Hall, IISc, Bangalore The extra dim...
published: 04 Jul 2013
author: ICTStalks
Strings and the Magic of Extra Dimensions - Prof Cumrun Vafa
Strings and the Magic of Extra Dimensions - Prof Cumrun Vafa
Cumrun Vafa Harvard University, MA 05 Jun 2013 Faculty Hall, IISc, Bangalore The extra dimensions of string theory which were originally viewed as a source o...- published: 04 Jul 2013
- views: 1245
- author: ICTStalks
3:42

VAFA
This Vid is the off-line meeting history....
published: 20 Nov 2009
author: kongchoong
VAFA
6:34

Vafa Animal Shelter
An overview of Vafa Animal Shelter in Hashtgerd, Tehran. Faranak, a Vafa volunteer in the ...
published: 02 Jun 2010
author: WINBroadcasting
Vafa Animal Shelter
Vafa Animal Shelter
An overview of Vafa Animal Shelter in Hashtgerd, Tehran. Faranak, a Vafa volunteer in the US is interviewed by WIN TV. Vafa Animal Shelter's website: http://...- published: 02 Jun 2010
- views: 5230
- author: WINBroadcasting
12:03

Joseph Polchinski: "Holography and Unification" - 2
Dirac Medalists' Lecture Series....
published: 02 Feb 2011
author: ICTP PIO
Joseph Polchinski: "Holography and Unification" - 2
Joseph Polchinski: "Holography and Unification" - 2
Dirac Medalists' Lecture Series.- published: 02 Feb 2011
- views: 1355
- author: ICTP PIO
10:33

Фрагмент фильма "Элегантная Вселенная"
Режиссер: Джулия Корт (Julia Cort), Джозеф Мак-Мастер (Joseph McMaster) В ролях: Michael D...
published: 03 May 2010
author: sublime4free
Фрагмент фильма "Элегантная Вселенная"
Фрагмент фильма "Элегантная Вселенная"
Режиссер: Джулия Корт (Julia Cort), Джозеф Мак-Мастер (Joseph McMaster) В ролях: Michael Duff, Sheldon Glashow, Brian Greene, Michael B. Green, Walter Lewin,...- published: 03 May 2010
- views: 5708
- author: sublime4free
8:51

Black hole thermodynamics [Wikipedia Article]
In physics, black hole thermodynamics is the area of study that seeks to reconcile the law...
published: 18 Sep 2013
Black hole thermodynamics [Wikipedia Article]
Black hole thermodynamics [Wikipedia Article]
In physics, black hole thermodynamics is the area of study that seeks to reconcile the laws of thermodynamics with the existence of black hole event horizons. Much as the study of the statistical mechanics of black body radiation led to the advent of the theory of quantum mechanics, the effort to understand the statistical mechanics of black holes has had a deep impact upon the understanding of quantum gravity, leading to the formulation of the holographic principle. Black hole The only way to satisfy the second law of thermodynamics is to admit that black holes have entropy. If black holes carried no entropy, it would be possible to violate the second law by throwing mass into the black hole. The increase of the entropy of the black hole more than compensates for the decrease of the entropy carried by the object that was swallowed. Starting from theorems proved by Stephen Hawking, Jacob Bekenstein conjectured that the black hole entropy was proportional to the area of its event horizon divided by the Planck area. Bekenstein suggested (½ ln 2)/4π as the constant of proportionality, asserting that if the constant was not exactly this, it must be very close to it. The next year, Hawking showed that black holes emit thermal Hawking radiation corresponding to a certain temperature (Hawking temperature). Using the thermodynamic relationship between energy, temperature and entropy, Hawking was able to confirm Bekenstein's conjecture and fix the constant of proportionality at 1/4: where A is the area of the event horizon, calculated at 4πR2, k is Boltzmann's constant, and is the Planck length. This is often referred to as the Bekenstein--Hawking formula. The subscript BH either stands for "black hole" or "Bekenstein-Hawking". The black hole entropy is proportional to the area of its event horizon. The fact that the black hole entropy is also the maximal entropy that can be obtained by the Bekenstein bound (wherein the Bekenstein bound becomes an equality) was the main observation that led to the holographic principle. Although Hawking's calculations gave further thermodynamic evidence for black hole entropy, until 1995 no one was able to make a controlled calculation of black hole entropy based on statistical mechanics, which associates entropy with a large number of microstates. In fact, so called "no hair" theorems appeared to suggest that black holes could have only a single microstate. The situation changed in 1995 when Andrew Strominger and Cumrun Vafa calculated the right Bekenstein-Hawking entropy of a supersymmetric black hole in string theory, using methods based on D-branes. Their calculation was followed by many similar computations of entropy of large classes of other extremal and near-extremal black holes, and the result always agreed with the Bekenstein-Hawking formula. In Loop quantum gravity (LQG) it is possible to associate a geometrical interpretation to the microstates: these are the quantum geometries of the horizon. LQG offers a geometric explanation of the finiteness of the entropy and of the proportionality of the area of the horizon. It is possible to derive, from the covariant formulation of full quantum theory (Spinfoam) the correct relation between energy and area (1st law), the Unruh temperature and the distribution that yields Hawking entropy. The calculation makes use of the notion of dynamical horizon and is done for non-extremal black holes. The laws of black hole mechanics The four laws of black hole mechanics are physical properties that black holes are believed to satisfy. The laws, analogous to the laws of thermodynamics, were discovered by Brandon Carter, Stephen Hawking and James Bardeen. Statement of the laws The laws of black hole mechanics are expressed in geometrized units. The Zeroth Law The horizon has constant surface gravity for a stationary black hole. The First Law For perturbations of stationary black holes, the change of energy is related to change of area, angular momentum, and electric charge by: where is the energy, is the surface gravity, is the horizon area, is the angular velocity, is the angular momentum, is the electrostatic potential and is the electric charge. The Second Law The horizon area is, assuming the weak energy condition, a non-decreasing function of time, This "law" was superseded by Hawking's discovery that black holes radiate, which causes both the black hole's mass and the area of its horizon to decrease over time. The Third Law It is not possible to form a black hole with vanishing surface gravity. = 0 is not possible to achieve. Discussion of the laws The Zeroth Law Attribution: Article text available under CC-BY-SA sourced from: http://en.wikipedia.org/wiki/Black_hole_thermodynamicsPublic domain image sourced from http://wikipedia.org/wiki/File:Black_Hole_Merger.jpg- published: 18 Sep 2013
- views: 0
0:59

Andrew Strominger
This Article Andrew Strominger is composed of Creative Common Content.
The Original Artic...
published: 28 Sep 2013
Andrew Strominger
Andrew Strominger
This Article Andrew Strominger is composed of Creative Common Content. The Original Article can be location at WikiPedia.org. Andrew Eben Strominger born 1955 is an American theoretical physicist who works on string theory and son of Jack L. Strominger. He is currently a professor at Harvard University and a senior fellow at the Society of Fellows. He attended the Cambridge School of Weston for high school and received his undergraduate degree from Harvard University in 1977 and his Ph.D from the Massachusetts Institute of Technology in 1982 under the supervision of Roman Jackiw. His contributions to physics include a paper with Cumrun Vafa that explains the microscopic origin of the black hole entropy originally calculated thermodynamically by Stephen Hawking and Jacob Bekenstein from string theory a paper with Philip Candelas Gary Horowitz and Edward Witten in the 1980s about the relevance of CalabiYau manifolds for obtaining the Standard Model from string theory other articles discussing the dSCFT correspondence a variation of AdSCFT correspondence Sbranes a variation of Dbranes- published: 28 Sep 2013
- views: 0
Youtube results:
8:52

Stephen Adler: "Localising numerical integration by 2^p subdivisions in p dimensions" - 2
Dirac Medalists' Lecture Series....
published: 02 Feb 2011
author: ICTP PIO
Stephen Adler: "Localising numerical integration by 2^p subdivisions in p dimensions" - 2
Stephen Adler: "Localising numerical integration by 2^p subdivisions in p dimensions" - 2
Dirac Medalists' Lecture Series.- published: 02 Feb 2011
- views: 42
- author: ICTP PIO
13:58

Michele Parrinello: The phase diagram of Sodium or using a sledgehammer to crack a nut
Dirac Medalists' Lecture Series....
published: 03 Feb 2011
author: ICTP PIO
Michele Parrinello: The phase diagram of Sodium or using a sledgehammer to crack a nut
Michele Parrinello: The phase diagram of Sodium or using a sledgehammer to crack a nut
Dirac Medalists' Lecture Series.- published: 03 Feb 2011
- views: 443
- author: ICTP PIO
106:36

Civilizations, String Theory, Space Missions and Cosmology
WATCH THE LATEST VIDEOS THAT CAME OUT TODAY HERE
http://www.youtube.com/user/NationsTruthT...
published: 02 Jul 2013
Civilizations, String Theory, Space Missions and Cosmology
Civilizations, String Theory, Space Missions and Cosmology
WATCH THE LATEST VIDEOS THAT CAME OUT TODAY HERE http://www.youtube.com/user/NationsTruthTV http://www.youtube.com/subscription_center?add_user=NationsTruthTV Subscribe To www.youtube.com/user/NationsTruthTV- published: 02 Jul 2013
- views: 10
11:21

Michael Green - 1
Connections between string theory and perturbative supersymmetric quantum field theory - 1...
published: 26 Jan 2011
author: ICTP PIO
Michael Green - 1
Michael Green - 1
Connections between string theory and perturbative supersymmetric quantum field theory - 1 Dirac Medalists' Lecture Series.- published: 26 Jan 2011
- views: 2729
- author: ICTP PIO