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12/13 PSI - Cosmology Review Lecture 12

Latham Boyle University of Edinburgh
March 06, 2013

PIRSA:13030043
Cosmology
12/13 PSI - Quantum Information Review Lecture 12

Andrew Childs University of Waterloo
March 06, 2013

PIRSA:13030051
Quantum Information
Non-perturbative problems in gauge theories: N=2 quiver QCD

Vasily Pestun Institute for Advanced Study (IAS)
March 06, 2013

PIRSA:13030103
Quantum Fields and Strings
12/13 PSI - Beyond the Standard Model Lecture 12
- Itay Yavin McMaster University
- Natalia Toro Stanford University
March 06, 2013

PIRSA:13030035
Particle Physics
Advanced General Relativity - Lecture 13

Rafael Sorkin Perimeter Institute for Theoretical Physics

March 05, 2013

PIRSA:13030006
Thermodynamical Property of Entanglement Entropy for Excited States and Holographic Local Quench

Masahiro Nozaki University of Chicago
March 05, 2013

PIRSA:13030081
Quantum Fields and Strings
The correlator of two vector and one axial current in QCD

Kirill Melnikov Johns Hopkins University
March 05, 2013

PIRSA:13030099
Particle Physics
12/13 PSI - Cosmology Review Lecture 11

Latham Boyle University of Edinburgh
March 05, 2013

PIRSA:13030042
Cosmology
12/13 PSI - Quantum Information Review Lecture 11

Andrew Childs University of Waterloo
March 05, 2013

PIRSA:13030050
Quantum Information
12/13 PSI - Beyond the Standard Model Lecture 11
- Itay Yavin McMaster University
- Natalia Toro Stanford University
March 05, 2013

PIRSA:13030034
Particle Physics
Getting the Most out of a Black Hole

Alexander Tchekhovskoy Princeton University
March 04, 2013

PIRSA:13030102
Cosmology
12/13 PSI - Cosmology Review Lecture 10

Latham Boyle University of Edinburgh
March 04, 2013

PIRSA:13030041
Cosmology

12/13 PSI - Cosmology Review Lecture 12

Latham Boyle University of Edinburgh
March 06, 2013

PIRSA:13030043
Cosmology
12/13 PSI - Quantum Information Review Lecture 12

Andrew Childs University of Waterloo
March 06, 2013

PIRSA:13030051
Quantum Information
Non-perturbative problems in gauge theories: N=2 quiver QCD

Vasily Pestun Institute for Advanced Study (IAS)
March 06, 2013

PIRSA:13030103
Quantum Fields and Strings
Non-perturbative effects are responsible for the essential dynamical features of the four-dimensional gauge theories such as QCD. The N=2 supersymmetric four-dimensional theories are an interesting class of models in which non-perturbative computations can be carried out with arbitrary precision using localization of the path integrals. I will explain the new exact non-perturbative results and the relation to classical and quantum integrable systems for a large class of N=2 supersymmetric QCD.
12/13 PSI - Beyond the Standard Model Lecture 12
- Itay Yavin McMaster University
- Natalia Toro Stanford University
March 06, 2013

PIRSA:13030035
Particle Physics
Advanced General Relativity - Lecture 13

Rafael Sorkin Perimeter Institute for Theoretical Physics

March 05, 2013

PIRSA:13030006
Thermodynamical Property of Entanglement Entropy for Excited States and Holographic Local Quench

Masahiro Nozaki University of Chicago
March 05, 2013

PIRSA:13030081
Quantum Fields and Strings
In this talk, we will describe our recent work. Recently, we focus on the thermodynamical property and time dependence of entanglement entropy. Using holography, we found that the entanglement entropy for a very small subsystem obeys a property which is analogous to the first law of thermodynamics when we excite the system. In relativistic setups, its effective temperature is proportional to the inverse of the subsystem size. This provides a universal relationship between the energy and the amount of quantum information. Moreover, we will propose a new holographic model of local quench and describe some results which we got by using this model. This talk is based on arXiv:1212.1164 [hep-th] and arXiv:1302.5703 [hep-th].
The correlator of two vector and one axial current in QCD

Kirill Melnikov Johns Hopkins University
March 05, 2013

PIRSA:13030099
Particle Physics
It is known that the correlator of one axial and two vector currents, that receives leading contributions through one-loop fermion triangle diagrams, is not modified by QCD radiative corrections at two loops. It was suggested that this non-renormalization of the VVA correlator persists in higher orders in perturbative QCD as well. To check this assertion, I compute the three-loop QCD corrections to the VAA-correlator using the technique of asymptotic expansions. I find that these corrections do not vanish and that they are proportional to the QCD beta-function. I will also review some properties of the VVA correlator that were discovered in recent years.
12/13 PSI - Cosmology Review Lecture 11

Latham Boyle University of Edinburgh
March 05, 2013

PIRSA:13030042
Cosmology
12/13 PSI - Quantum Information Review Lecture 11

Andrew Childs University of Waterloo
March 05, 2013

PIRSA:13030050
Quantum Information
12/13 PSI - Beyond the Standard Model Lecture 11
- Itay Yavin McMaster University
- Natalia Toro Stanford University
March 05, 2013

PIRSA:13030034
Particle Physics
Getting the Most out of a Black Hole

Alexander Tchekhovskoy Princeton University
March 04, 2013

PIRSA:13030102
Cosmology
As black holes accrete surrounding gas, they often produce relativistic, collimated outflows, or jets. Jets are expected to form in the black hole vicinity making them powerful probes of strong-field gravity. However, how jet properties are connected to black hole and accretion flow properties has been unclear. Recent progress in computer simulations of black hole accretion enables studies of jet formation in unprecedented detail. For the first time, 3D general relativistic magnetohydrodynamic numerical simulations allow one to determine the maximum efficiency with which accretion onto black holes can power relativistic jets. I will present the dependence of this maximum efficiency on black hole spin and discuss how this dependence allows one to probe strong-field gravity. In realistic astrophysical systems, the angular momentum vector of the accretion flow can be tilted relative to the spin of the black hole. I will present the first simulations of jets from such tilted accretion systems and discuss their observational signatures.
12/13 PSI - Cosmology Review Lecture 10

Latham Boyle University of Edinburgh
March 04, 2013

PIRSA:13030041
Cosmology

Title	Date	Collection	Type	Info
12/13 PSI - Cosmology Review Lecture 12	2013‑03‑06	12/13 PSI - Cosmology Review	Course	View details
12/13 PSI - Quantum Information Review Lecture 12	2013‑03‑06	12/13 PSI - Quantum Information Review	Course	View details
Non-perturbative problems in gauge theories: N=2 quiver QCD	2013‑03‑06	Colloquium	Scientific Series	View details
12/13 PSI - Beyond the Standard Model Lecture 12	2013‑03‑06	12/13 PSI - Beyond the Standard Model	Course	View details
Advanced General Relativity - Lecture 13	2013‑03‑05	Elements of General Relativity	Course	View details
Thermodynamical Property of Entanglement Entropy for Excited States and Holographic Local Quench	2013‑03‑05	Quantum Fields and Strings	Scientific Series	View details
The correlator of two vector and one axial current in QCD	2013‑03‑05	Particle Physics	Scientific Series	View details
12/13 PSI - Cosmology Review Lecture 11	2013‑03‑05	12/13 PSI - Cosmology Review	Course	View details
12/13 PSI - Quantum Information Review Lecture 11	2013‑03‑05	12/13 PSI - Quantum Information Review	Course	View details
12/13 PSI - Beyond the Standard Model Lecture 11	2013‑03‑05	12/13 PSI - Beyond the Standard Model	Course	View details
Getting the Most out of a Black Hole	2013‑03‑04	Colloquium	Scientific Series	View details
12/13 PSI - Cosmology Review Lecture 10	2013‑03‑04	12/13 PSI - Cosmology Review	Course	View details

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