Talks

13321 - 13332 of 20131 Results

Dark matter densities on small scales and implications for dark matter models

Manoj Kaplinghat University of California, Irvine

July 24, 2012

PIRSA:12070000

Astrophysics
String Theory and Holography

Pedro Vieira Perimeter Institute for Theoretical Physics

July 24, 2012

PIRSA:12070005

High Energy Physics
What is the Universe Made Of? The Case for Dark Matter and Dark Energy

Cliff Burgess McMaster University

July 13, 2012

PIRSA:12070004

Astrophysics
Entanglement, Holography, and the Quantum Phases of Matter

Subir Sachdev Harvard University

July 13, 2012

PIRSA:12070010
Entangling Superconductivity and antiferromagnetism: Quantum Monte Carlo without the sign Problem

Subir Sachdev Harvard University

July 11, 2012

PIRSA:12070009

Condensed Matter
Smash, Bang, Boom: Fundamental Physics at the LHC

Natalia Toro Stanford University

July 11, 2012

PIRSA:12070002

High Energy Physics
The Path Integral Interpretation of Quantum Mechanics

Fay Dowker Imperial College London

July 10, 2012

PIRSA:12070001
TBA

Itay Yavin McMaster University

July 10, 2012

PIRSA:12070011
Modern Cosmology

Niayesh Afshordi University of Waterloo

July 09, 2012

PIRSA:12070003

Astrophysics
Causal Constraints on Possible Measurements

Leron Borsten Heriot-Watt University

June 28, 2012

PIRSA:12060078

High Energy Physics
Holographic Mutual Information is Monogamous

Patrick Hayden Stanford University

June 28, 2012

PIRSA:12060070

Quantum Physics
Quantum Tasks in Minkowski Space

Adrian Kent University of Cambridge

June 28, 2012

PIRSA:12060062

Mathematical Physics

Dark matter densities on small scales and implications for dark matter models

Manoj Kaplinghat University of California, Irvine

July 24, 2012

PIRSA:12070000

Astrophysics

We will discuss the estimated densities of dark matter in the central regions of galaxies and discuss their inconsistency with the predictions of cold dark matter only simulations. We will focus on the satellites of the Milky Way to highlight this issue and then explore dark matter with significant self-interactions as a viable alternative. Milky Way satellites also place stringent constraints on WIMP dark matter models in a completely different way through Fermi-LAT observations and we will summarize those results.
String Theory and Holography

Pedro Vieira Perimeter Institute for Theoretical Physics

July 24, 2012

PIRSA:12070005

High Energy Physics
What is the Universe Made Of? The Case for Dark Matter and Dark Energy

Cliff Burgess McMaster University

July 13, 2012

PIRSA:12070004

Astrophysics

For the first time in human thought it is now
possible to observationally determine how much matter is in the Universe as a
whole. These observations strongly support the “Concordance Model” of Hot Big
Bang Cosmology, and reinforce earlier indications that ordinary matter (atoms,
nuclei and electrons) make up at present at most 4% of the total of the
Universal energy density. The big surprise was that the rest consists of *two*
kinds of unknown forms of matter: the so-called Dark Matter and Dark Energy.
This talk summarizes for non-specialists the various lines of evidence for
their existence, and some of the theoretical ideas which have been proposed to
account for their properties
Entanglement, Holography, and the Quantum Phases of Matter

Subir Sachdev Harvard University

July 13, 2012

PIRSA:12070010
Entangling Superconductivity and antiferromagnetism: Quantum Monte Carlo without the sign Problem

Subir Sachdev Harvard University

July 11, 2012

PIRSA:12070009

Condensed Matter

It has long been known that a metal near an instability to antiferromagnetism also has a weak-coupling Cooper instability to spin-singlet d-wave-like superconductivity. However, the theory of the antiferromagnetic quantum critical point flows to strong-coupling in two spatial dimensions, and so the fate of the superconductivity has also been unclear. I will describe a method to realize the generic antiferromagnetic quantum critical in a metal in a sign-problem-free Monte Carlo simulation. Results showing Fermi surface reconstruction and unconventional spin-singlet superconductivity across the critical point are obtained.
Smash, Bang, Boom: Fundamental Physics at the LHC

Natalia Toro Stanford University

July 11, 2012

PIRSA:12070002

High Energy Physics

The world's most ambitious scientific experiment is buried 100 meters underground, straddling Switzerland and France. A billion times every minute, the Large Hadron Collider (LHC) slams together protons, while four giant detectors watch closely. - So how does the Large Hadron Collider work? - Why can slamming tiny particles into each other provide clues about the nature of all space and time? - What mysteries are physicists trying to solve with data from the LHC? - How does the cutting edge of particle physics relate to the world around us, from the patterns of stars in the sky to the fact that they shine at all? Natalia Toro, PI Faculty, works at the intersection of theories and hard data. She will explain how complex collision data from the LHC is being digested and examined right now, and how it may set the course for the science of the future.
The Path Integral Interpretation of Quantum Mechanics

Fay Dowker Imperial College London

July 10, 2012

PIRSA:12070001
TBA

Itay Yavin McMaster University

July 10, 2012

PIRSA:12070011
Modern Cosmology

Niayesh Afshordi University of Waterloo

July 09, 2012

PIRSA:12070003

Astrophysics

This presentation will cover a number of topics in cosmology today including dark energy, dark matter and the cosmological constant.
Causal Constraints on Possible Measurements

Leron Borsten Heriot-Watt University

June 28, 2012

PIRSA:12060078

High Energy Physics

A crucial question in any approach to quantum information processing is: first, how are classical bits encoded physically in the quantum system, second, how are they then manipulated and, third, how are they finally read out? These questions are particularly challenging when investigating quantum information processing in a relativistic spacetime. An obvious framework for such an investigation is relativistic quantum field theory. Here, progress is hampered by the lack of a universally applicable rule for calculating the probabilities of the outcomes of ideal measurements on a relativistic quantum field in a collection of spacetime regions. Indeed, a straightforward relativistic generalisation of the non-relativistic formula for these probabilities leads to superluminal signalling.

Motivated by these considerations we ask what interventions/ideal measurements can we in principle make, taking causality as our guiding criterion. In the course of this analysis we reconsider various aspects of ideal measurements in QFT, detector models and the probability rules themselves. In particular, it is shown that an ideal measurement of a one–particle wave packet state of a relativistic quantum field in Minkowski spacetime enables superluminal signalling. The result holds for a measurement that takes place over an intervention region in spacetime whose extent in time in some frame is longer than the light crossing time of the packet in that frame.
Holographic Mutual Information is Monogamous

Patrick Hayden Stanford University

June 28, 2012

PIRSA:12060070

Quantum Physics

I'll describe a special information-theoretic property of quantum field theories with holographic duals: the mutual informations among arbitrary disjoint spatial regions A,B,C obey the inequality I(A:BC) >= I(A:B)+I(A:C), provided entanglement entropies are given by the Ryu-Takayanagi formula. Inequalities of this type are known as monogamy relations and are characteristic of measures of quantum entanglement. This suggests that correlations in holographic theories arise primarily from entanglement rather than classical correlations. Moreover, monogamy property implies that the Ryu-Takayanagi formula is consistent with all known general inequalities obeyed by the entanglement entropy, including an infinite set recently discovered by Cadney, Linden, and Winter; this constitutes significant evidence in favour of its validity.
Quantum Tasks in Minkowski Space

Adrian Kent University of Cambridge

June 28, 2012

PIRSA:12060062

Mathematical Physics

The fundamental properties of quantum information and its applications to computing and cryptography have been greatly illuminated by considering information-theoretic tasks that are provably possible or impossible within non-relativistic quantum mechanics. In this talk I describe a general framework for defining tasks within (special) relativistic quantum theory and illustrate it with examples from relativistic quantum cryptography.

Title	Date	Collection	Type	Info
Dark matter densities on small scales and implications for dark matter models	2012‑07‑24	Cosmology and Gravitation	Scientific Series	View details
String Theory and Holography	2012‑07‑24	ISSYP 2012		View details
What is the Universe Made Of? The Case for Dark Matter and Dark Energy	2012‑07‑13	ISSYP 2012		View details
Entanglement, Holography, and the Quantum Phases of Matter	2012‑07‑13	Quantum Matter	Scientific Series	View details
Entangling Superconductivity and antiferromagnetism: Quantum Monte Carlo without the sign Problem	2012‑07‑11	Quantum Matter	Scientific Series	View details
Smash, Bang, Boom: Fundamental Physics at the LHC	2012‑07‑11	Particle Physics		View details
The Path Integral Interpretation of Quantum Mechanics	2012‑07‑10	Quantum Foundations	Scientific Series	View details
TBA	2012‑07‑10	Particle Physics	Other	View details
Modern Cosmology	2012‑07‑09	Cosmology and Gravitation		View details
Causal Constraints on Possible Measurements	2012‑06‑28	Relativistic Quantum Information - 2012	Conference	View details
Holographic Mutual Information is Monogamous	2012‑06‑28	Relativistic Quantum Information - 2012	Conference	View details
Quantum Tasks in Minkowski Space	2012‑06‑28	Relativistic Quantum Information - 2012	Conference	View details

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Format results

Dark matter densities on small scales and implications for dark matter models

String Theory and Holography

What is the Universe Made Of? The Case for Dark Matter and Dark Energy

Entanglement, Holography, and the Quantum Phases of Matter

Entangling Superconductivity and antiferromagnetism: Quantum Monte Carlo without the sign Problem

Smash, Bang, Boom: Fundamental Physics at the LHC

The Path Integral Interpretation of Quantum Mechanics

TBA

Modern Cosmology

Causal Constraints on Possible Measurements

Holographic Mutual Information is Monogamous

Quantum Tasks in Minkowski Space

Dark matter densities on small scales and implications for dark matter models

String Theory and Holography

What is the Universe Made Of? The Case for Dark Matter and Dark Energy

Entanglement, Holography, and the Quantum Phases of Matter

Entangling Superconductivity and antiferromagnetism: Quantum Monte Carlo without the sign Problem

Smash, Bang, Boom: Fundamental Physics at the LHC

The Path Integral Interpretation of Quantum Mechanics

TBA

Modern Cosmology

Causal Constraints on Possible Measurements

Holographic Mutual Information is Monogamous

Quantum Tasks in Minkowski Space