Talks

13021 - 13032 of 20118 Results

Quantum Chaos, Information Gain and Quantum Tomography.

Vaibhav Madhok Wilfrid Laurier University

December 11, 2012

PIRSA:12120036

Quantum Physics
(0,2) Gauge Dynamics and Flux Compactifications

Callum Quigley Kirkland & Ellis

December 11, 2012

PIRSA:12120006

High Energy Physics
A robust constraint on cosmic textures from the cosmic microwave background

Stephen Feeney

December 11, 2012

PIRSA:12120034

Astrophysics
Nonlinear Extensions for the Inflationary Power Spectra

Shun-Pei Miao Utrecht University

December 11, 2012

PIRSA:12120014

Astrophysics
Mathematica - Lecture 3b

Pedro Vieira Perimeter Institute for Theoretical Physics

December 10, 2012

PIRSA:12120021

Mathematical Physics
Mathematica - Lecture 3a

Pedro Vieira Perimeter Institute for Theoretical Physics

December 10, 2012

PIRSA:12120020

Mathematical Physics
Light sleptons, Higgs phenomenology and the vacuum

Stefania Gori University of California, Santa Cruz

December 07, 2012

PIRSA:12120018

High Energy Physics
CMB as a Probe of New Physics: The Story of Cosmic Birefringence

December 06, 2012

PIRSA:12120019

Astrophysics
Renormalizing TGFTs: a 3d example on SU(2)

Sylvain Carrozza University of Burgundy

December 06, 2012

PIRSA:12120007

General Relativity & Quantum Cosmology
Approaches to modeling pulsar magnetospheres

Anatoly Spitkovsky Princeton University

December 06, 2012

PIRSA:12120001

General Relativity & Quantum Cosmology
Unitarity, black hole microstates and how Alices fuzzes but may not even know it

Andrea Puhm University of Amsterdam

December 06, 2012

PIRSA:12120029

High Energy Physics
Curiosity: How Science Became Interested in Everything

Philip Ball The Lancet Group

December 05, 2012

PIRSA:12120004

Quantum Chaos, Information Gain and Quantum Tomography.

Vaibhav Madhok Wilfrid Laurier University

December 11, 2012

PIRSA:12120036

Quantum Physics

Quantum chaos is the study of quantum systems whose classical description is chaotic. How does chaos manifest itself in the quantum world? In recent years, attempts have been made to address this question from the perspective of quantum information theory. It is in this spirit that we study the connection between quantum chaos and information gain in the time series of a measurement record used for quantum tomography. The record is obtained as a sequence of expectation values of a Hermitian operator evolving under repeated application of the Floquet operator of the quantum kicked top on a large ensemble of identical systems. We find an increase in information gain and hence higher fidelities in the process when the Floquet maps employed increase in chaoticity. We make predictions for the information gain using random matrix theory in the fully chaotic regime and show a remarkable agreement between the two.
(0,2) Gauge Dynamics and Flux Compactifications

Callum Quigley Kirkland & Ellis

December 11, 2012

PIRSA:12120006

High Energy Physics

Two-dimensional gauge theories with (0,2) supersymmetry admit a much broader, and more interesting, class of solutions than their better studied (2,2) counterparts. In this talk, we will explore some of the possibilities that are offered by this additional freedom. The moduli spaces we find can be interpreted as the target spaces for heterotic strings moving in backgrounds with non-trivial H-flux. A remarkable relationship between (0,2) gauge anomalies and H-flux will emerge.
A robust constraint on cosmic textures from the cosmic microwave background

Stephen Feeney

December 11, 2012

PIRSA:12120034

Astrophysics

Fluctuations in the cosmic microwave background (CMB) contain information which has been pivotal in establishing the current cosmological model. These data can also be used to test well-motivated additions to this model, such as cosmic textures. Textures are a type of topological defect that can be produced during a cosmological phase transition in the early universe, and which leave characteristic hot and cold spots in the CMB. We apply Bayesian methods to carry out an optimal test of the texture hypothesis, using full-sky data from the Wilkinson Microwave Anisotropy Probe. We conclude that current data do not warrant augmenting the standard cosmological model with textures. We rule out at 95% confidence models that predict more than 6 detectable cosmic textures on the full sky.
Nonlinear Extensions for the Inflationary Power Spectra

Shun-Pei Miao Utrecht University

December 11, 2012

PIRSA:12120014

Astrophysics

We expound several principles in an attempt to clarify the debate over infrared loop corrections to the primordial scalar and tensor power spectra from inflation. Among other things we note that existing proposals for nonlinear extensions of the scalar fluctuation field $\zeta$ introduce new ultraviolet divergences which no one understands how to renormalize. Loop corrections and higher correlators of these putative observables would also be enhanced by inverse powers of the slow roll parameter $\epsilon$. We propose an extension which might be better behaved.
Mathematica - Lecture 3b

Pedro Vieira Perimeter Institute for Theoretical Physics

December 10, 2012

PIRSA:12120021

Mathematical Physics
Mathematica - Lecture 3a

Pedro Vieira Perimeter Institute for Theoretical Physics

December 10, 2012

PIRSA:12120020

Mathematical Physics
Light sleptons, Higgs phenomenology and the vacuum

Stefania Gori University of California, Santa Cruz

December 07, 2012

PIRSA:12120018

High Energy Physics

We analyze the implications for Susy theories of a Higgs to di-photon rate enhanced, if compared to the Standard Model prediction. We show how models predicting a sizable enhancement have generically an electroweak vacuum that is not absolutely stable. In particular we discuss the only viable scenario that can predict sizable new physics effects in the di-photon rate in the framework of the MSSM: a scenario with light and heavily mixed staus. We conclude with the phenomenology of this model and with the prospects of probing it at the LHC, through the direct production of light staus.
CMB as a Probe of New Physics: The Story of Cosmic Birefringence

December 06, 2012

PIRSA:12120019

Astrophysics

Cosmological birefringence is a postulated rotation of the linear polarization of photons that arises due to a Chern-Simons coupling of a new scalar field to electromagnetism. In particular, it appears as a generic feature of simple quintessence models for Dark Energy, and therefore, should it be detected, could provide insight into the microphysics of cosmic acceleration. Prior work has sought this rotation, assuming the rotation angle to be uniform across the sky, by looking for the parity-violating TB and EB correlations in the CMB temperature/polarization. However, if the scalar field that gives rise to cosmological birefringence has spatial fluctuations, then the rotation angle may vary across the sky. In this talk, I will present the results of the first CMB-based search for direction-dependent cosmological birefringence, using WMAP-7 data, and report the constraint on the rotation-angle power spectrum for all multipoles up to the resolution of the instrument. I will discuss the implications for a specific models for rotation, and show forecasts for Planck and future experiments. I will then conclude with a brief discussion of other exotic physical models, such as chiral gravity, and astrophysical scenarios, such as inhomogeneous reionization, that can be probed using the same analysis.
Renormalizing TGFTs: a 3d example on SU(2)

Sylvain Carrozza University of Burgundy

December 06, 2012

PIRSA:12120007

General Relativity & Quantum Cosmology

I will recall the main motivations for considering spin foam models in their Group Field Theory (GFT) versions, which are quantum field theories defined on group manifolds. As for any other quantum field theory, a fully consistent definition of the latter must involve renormalization. I will briefly review a specific class of GFTs, called tensorial, for which progress in this direction has recently been possible. A new just-renormalizable model, in three dimensions and on the SU(2) group, will be presented. Interestingly, it includes the geometric constraint of the Boulatov model, and might as such be related to Euclidean quantum gravity in three dimensions. Furthermore, this opens the way to a similar analysis of current 4d gravity spin foam models.
Approaches to modeling pulsar magnetospheres

Anatoly Spitkovsky Princeton University

December 06, 2012

PIRSA:12120001

General Relativity & Quantum Cosmology

Pulsars are rotating magnetized neutron stars that emit broadband pulses of radiation. Our ability to model magnetospheres of pulsars has been hampered by the difficulty of solving the self-consistent behavior of strongly magnetized relativistic plasmas. I will describe
recent progress in numerical modeling of magnetically-dominated plasmas and show applications to pulsar magnetospheres in increasing levels of realism, including ideal and resistive force-free,
relativistic MHD and kinetic models. The knowledge of the magnetospheric shape together with the new observations of gamma-ray emission from pulsars with Fermi telescope allow to directly constrain the location and physics of the acceleration regions in the magnetosphere and the origin of high energy emission. The pulsar magnetosphere is a prototype for other strongly magnetized
astrophysical objects, and I will discuss how the lessons from pulsar modeling can be useful in predicting EM counterparts to gravitational wave sources.
Unitarity, black hole microstates and how Alices fuzzes but may not even know it

Andrea Puhm University of Amsterdam

December 06, 2012

PIRSA:12120029

High Energy Physics

The information paradox and the infall problem have been long-standing puzzles in the understanding of black holes. The idea of free infall is in considerable tension with unitarity of the evaporation process and recent developements have made this tension sharp. In the first part of my talk I will address the information question and argue that unitarty requires every quantum of radiation leaving the black hole to carry information about the initial state. Unitary evaporation is thus inconsistent with an information-free horizon at every step of the evaporation process and this extends the recent firewall result. This immediately raises the question of What is the required horizon-scale structure? I will show an explicit construction of near-extremal black hole microstates which put flesh and branes on the fuzzball proposal and may realize firewalls in string theory. In the second part I will address the question of What happens to an observer falling into a fuzzball? I will argue that the answer is dependent on the energy scale of the infalling observer.
Curiosity: How Science Became Interested in Everything

Philip Ball The Lancet Group

December 05, 2012

PIRSA:12120004

Title	Date	Collection	Type	Info
Quantum Chaos, Information Gain and Quantum Tomography.	2012‑12‑11	Quantum Foundations	Scientific Series	View details
(0,2) Gauge Dynamics and Flux Compactifications	2012‑12‑11	Quantum Fields and Strings	Scientific Series	View details
A robust constraint on cosmic textures from the cosmic microwave background	2012‑12‑11	Cosmology and Gravitation	Scientific Series	View details
Nonlinear Extensions for the Inflationary Power Spectra	2012‑12‑11	Cosmology and Gravitation	Scientific Series	View details
Mathematica - Lecture 3b	2012‑12‑10	12/13 PSI - Front End	Course	View details
Mathematica - Lecture 3a	2012‑12‑10	12/13 PSI - Front End	Course	View details
Light sleptons, Higgs phenomenology and the vacuum	2012‑12‑07	Particle Physics	Scientific Series	View details
CMB as a Probe of New Physics: The Story of Cosmic Birefringence	2012‑12‑06	Cosmology and Gravitation	Scientific Series	View details
Renormalizing TGFTs: a 3d example on SU(2)	2012‑12‑06	Quantum Gravity	Scientific Series	View details
Approaches to modeling pulsar magnetospheres	2012‑12‑06	Strong Gravity	Scientific Series	View details
Unitarity, black hole microstates and how Alices fuzzes but may not even know it	2012‑12‑06	Quantum Fields and Strings	Scientific Series	View details
Curiosity: How Science Became Interested in Everything	2012‑12‑05	Public Lecture Series	Public Lectures	View details

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Format results

Quantum Chaos, Information Gain and Quantum Tomography.

(0,2) Gauge Dynamics and Flux Compactifications

A robust constraint on cosmic textures from the cosmic microwave background

Nonlinear Extensions for the Inflationary Power Spectra

Mathematica - Lecture 3b

Mathematica - Lecture 3a

Light sleptons, Higgs phenomenology and the vacuum

CMB as a Probe of New Physics: The Story of Cosmic Birefringence

Renormalizing TGFTs: a 3d example on SU(2)

Approaches to modeling pulsar magnetospheres

Unitarity, black hole microstates and how Alices fuzzes but may not even know it

Curiosity: How Science Became Interested in Everything

Quantum Chaos, Information Gain and Quantum Tomography.

(0,2) Gauge Dynamics and Flux Compactifications

A robust constraint on cosmic textures from the cosmic microwave background

Nonlinear Extensions for the Inflationary Power Spectra

Mathematica - Lecture 3b

Mathematica - Lecture 3a

Light sleptons, Higgs phenomenology and the vacuum

CMB as a Probe of New Physics: The Story of Cosmic Birefringence

Renormalizing TGFTs: a 3d example on SU(2)

Approaches to modeling pulsar magnetospheres

Unitarity, black hole microstates and how Alices fuzzes but may not even know it

Curiosity: How Science Became Interested in Everything