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Infinite Chiral Symmetry in Four Dimensions

Wolfger Peelaers University of Oxford

September 16, 2014

PIRSA:14090079
Scalar Simplified Models and Dark Matter at Colliders

Matthew Buckley Rutgers University
September 16, 2014

PIRSA:14090080
Particle Physics
Cosmic flows: testing gravity and the matter power spectrum on very large scales

Mike Hudson University of Waterloo
September 16, 2014

PIRSA:14090077
Cosmology
14/15 PSI Quantum Theory-7

Joseph Emerson Institute for Quantum Computing (IQC)

September 16, 2014

PIRSA:14090050
14/15 PSI - Relativity- Lecture 7

Neil Turok University of Edinburgh

September 16, 2014

PIRSA:14090017
14/15 PSI Quantum Theory-6

Joseph Emerson Institute for Quantum Computing (IQC)

September 15, 2014

PIRSA:14090049
14/15 PSI - Relativity- Lecture 6

Neil Turok University of Edinburgh

September 15, 2014

PIRSA:14090016
Maximal supergravity, holography and the Romans mass

Oscar Varela Harvard University
September 12, 2014

PIRSA:14090071
Quantum Fields and Strings
14/15 PSI Quantum Theory-5

Joseph Emerson Institute for Quantum Computing (IQC)

September 12, 2014

PIRSA:14090046
14/15 PSI - Relativity- Lecture 5

Neil Turok University of Edinburgh

September 12, 2014

PIRSA:14090011
Stripes and pairing in t-J and Hubbard models

Steven White University of California, Irvine
September 11, 2014

PIRSA:14090074
Condensed Matter
Force-Free Electrodynamics around Extreme Kerr Black Holes

Maria J. Rodriguez Utah State University
September 11, 2014

PIRSA:14090065
Strong Gravity

Infinite Chiral Symmetry in Four Dimensions

Wolfger Peelaers University of Oxford

September 16, 2014

PIRSA:14090079

We describe a new correspondence between four-dimensional conformal field theories with extended supersymmetry and two-dimensional chiral algebras. We explore the resulting chiral algebras in the context of theories of class S. The class S duality web implies nontrivial associativity properties for the corresponding chiral algebras, the structure of which can be summarized by a generalized topological quantum field theory.
Scalar Simplified Models and Dark Matter at Colliders

Matthew Buckley Rutgers University
September 16, 2014

PIRSA:14090080
Particle Physics
Dark matter is clear evidence of the existence of new physics beyond the Standard Model, and there are compelling reasons to expect that this physics can be probed at the LHC. As we prepare for Run II, we must consider a wide range of possible phenomenology, leaving no stone unturned. In this talk, I present a set of scalar and pseudoscalar models which provide a useful framework to interpret dark matter results, and can motivate new searches in novel channels at the LHC.
Cosmic flows: testing gravity and the matter power spectrum on very large scales

Mike Hudson University of Waterloo
September 16, 2014

PIRSA:14090077
Cosmology
Peculiar velocities - deviations from Hubble expansion - are the only practical probe of the growth of matter density fluctuations on very large scales in the nearby Universe. I will discuss recent measurements of quantities of cosmological interest from our group and others. One is the "bulk" flow of nearby galaxies with respect to the frame defined by the Cosmic Microwave Background, and what this tells us about fluctuations on large very spatial scales. The second is the measurement of the growth rate of fluctuations, a critical test of Lambda CDM and modified gravity models.
14/15 PSI Quantum Theory-7

Joseph Emerson Institute for Quantum Computing (IQC)

September 16, 2014

PIRSA:14090050
14/15 PSI - Relativity- Lecture 7

Neil Turok University of Edinburgh

September 16, 2014

PIRSA:14090017
14/15 PSI Quantum Theory-6

Joseph Emerson Institute for Quantum Computing (IQC)

September 15, 2014

PIRSA:14090049
14/15 PSI - Relativity- Lecture 6

Neil Turok University of Edinburgh

September 15, 2014

PIRSA:14090016
Maximal supergravity, holography and the Romans mass

Oscar Varela Harvard University
September 12, 2014

PIRSA:14090071
Quantum Fields and Strings
At large N, an important sector of the ABJM field theory defined on a stack of N M2-branes can be described holographically by the D=4 N=8 SO(8)-gauged supergravity of de Wit and Nicolai. Since its inception, the latter has been tacitly assumed to be unique. Recently, however, a one-parameter family of SO(8) gaugings of N=8 supergravity has been discovered, the de Wit-Nicolai theory being just a member in this class. I will explain how this overlooked family of SO(8)-gauged supergravities is deeply related to electric/magnetic duality breaking in four dimensions. I will then discuss some predictions that can be made about the family of dual large-N field theories that these supergravities define, focusing on the structure of superconformal phases and the RG flows between them. I will finally argue that when the gauging is chosen to be related, but different, to the SO(8) one, the D=4 N=8 family arises as consistent truncation of massive IIA on the six-sphere, with the Romans mass identified as the electric/magnetic duality-breaking parameter.
14/15 PSI Quantum Theory-5

Joseph Emerson Institute for Quantum Computing (IQC)

September 12, 2014

PIRSA:14090046
14/15 PSI - Relativity- Lecture 5

Neil Turok University of Edinburgh

September 12, 2014

PIRSA:14090011
Stripes and pairing in t-J and Hubbard models

Steven White University of California, Irvine
September 11, 2014

PIRSA:14090074
Condensed Matter
This has been a leading question in condensed matter physics since the discovery of the cuprate superconductors. In this talk I will review some of the DMRG and tensor network results for the ground states of these models. A key question I'll address is the issue of stripes: are the ground states striped? Do stripes compete with or induce d-wave superconductivity? Another question I'll address is: how well does 2D DMRG do in comparison with iPEPS and quantum Monte Carlo. I will also show recent results for a standard 3-band Hubbard model for the cuprates. The asymmetry between hole and electron doped systems which is seen in the cuprates arises naturally from this model.
Force-Free Electrodynamics around Extreme Kerr Black Holes

Maria J. Rodriguez Utah State University
September 11, 2014

PIRSA:14090065
Strong Gravity
Plasma-filled magnetospheres can extract energy from a spinning black hole and provide the power source for a variety of observed astrophysical phenomena. These magnetospheres are described by the highly nonlinear equations of force-free electrodynamics, or FFE. Typically these equations can only be solved numerically. In this talk I will explain how to analytically obtain several infinite families of exact solutions of the full nonlinear FFE equations very near the horizon of a maximally spinning black hole, where the energy extraction takes place.

Title	Date	Collection	Type	Info
Infinite Chiral Symmetry in Four Dimensions	2014‑09‑16	Quantum Fields and Strings	Scientific Series	View details
Scalar Simplified Models and Dark Matter at Colliders	2014‑09‑16	Particle Physics	Scientific Series	View details
Cosmic flows: testing gravity and the matter power spectrum on very large scales	2014‑09‑16	Cosmology and Gravitation	Scientific Series	View details
14/15 PSI Quantum Theory-7	2014‑09‑16	14/15 PSI - Quantum Theory	Course	View details
14/15 PSI - Relativity- Lecture 7	2014‑09‑16	14/15 PSI -Relativity	Course	View details
14/15 PSI Quantum Theory-6	2014‑09‑15	14/15 PSI - Quantum Theory	Course	View details
14/15 PSI - Relativity- Lecture 6	2014‑09‑15	14/15 PSI -Relativity	Course	View details
Maximal supergravity, holography and the Romans mass	2014‑09‑12	Quantum Fields and Strings	Scientific Series	View details
14/15 PSI Quantum Theory-5	2014‑09‑12	14/15 PSI - Quantum Theory	Course	View details
14/15 PSI - Relativity- Lecture 5	2014‑09‑12	14/15 PSI -Relativity	Course	View details
Stripes and pairing in t-J and Hubbard models	2014‑09‑11	Quantum Matter	Scientific Series	View details
Force-Free Electrodynamics around Extreme Kerr Black Holes	2014‑09‑11	Strong Gravity	Scientific Series	View details

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