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New Light Species and the CMB - Joint Cosmology/Particle Physics Seminar

Christopher Brust Duolingo, Inc.
November 19, 2013 PIRSA:13110051
Particle Physics
The Amplitude Mode in Condensed Matter : Higgs Hunting on a Budget

Daniel Arovas University of California, San Diego
November 19, 2013 PIRSA:13110054
Condensed Matter
General Relativity for Cosmology - Lecture 18

Achim Kempf University of Waterloo

November 19, 2013 PIRSA:13110005
13/14 PSI - Quantum Field Theory II - Lecture 8

Francois David Commissariat a Energie Atomique (CEA) - Saclay - Institut de Physique Théorique (IPhT)

November 20, 2013 PIRSA:13110017
13/14 PSI - Condensed Matter - Lecture 8
- Anushya Chandran Perimeter Institute for Theoretical Physics
- Roger Melko University of Waterloo
- Xiao-Gang Wen Massachusetts Institute of Technology (MIT) - Department of Physics
November 20, 2013 PIRSA:13110036
Light and matter: towards macroscopic quantum systems

Jacob Taylor Office of Science and Technology
November 20, 2013 PIRSA:13110060
Quantum Information
Quantum Adversary (Upper) Bound

Shelby Kimmel Massachusetts Institute of Technology (MIT)
November 20, 2013 PIRSA:13110090
Quantum Information
13/14 PSI - Quantum Field Theory II - Lecture 9

Francois David Commissariat a Energie Atomique (CEA) - Saclay - Institut de Physique Théorique (IPhT)

November 21, 2013 PIRSA:13110018
13/14 PSI - Condensed Matter - Lecture 9
- Anushya Chandran Perimeter Institute for Theoretical Physics
- Roger Melko University of Waterloo
- Xiao-Gang Wen Massachusetts Institute of Technology (MIT) - Department of Physics
November 21, 2013 PIRSA:13110037
Generalized Kahler geometry and T-duality (no audio)

Marco Gualtieri University of Toronto

November 19, 2004 PIRSA:04110016
Charged particle motion in magnetized black holes

Valeri Frolov University of Alberta
November 21, 2013 PIRSA:13110066
Strong Gravity
Dimensional reduction in the sky
November 21, 2013 PIRSA:13110059
Quantum Gravity

New Light Species and the CMB - Joint Cosmology/Particle Physics Seminar

Christopher Brust Duolingo, Inc.
November 19, 2013 PIRSA:13110051
Particle Physics
The effective number of neutrino species in our universe, Neff, is capable of probing the presence of new light or massless species in our universe. I will first review relevant facts about both CMB measurements of new light species and thermodynamics in the early universe. Then, I will present the effects of many models of BSM physics containing new light species on the CMB, including models containing eV-scale sterile neutrinos compatible with anomalies in neutrino experiments, and interpret the compatibility of the parameter space of these models in terms of the recent results from the Planck satellite. I will argue that the bounds on couplings obtained from the Planck measurement of the CMB are competitive with bounds coming from other areas of physics.
The Amplitude Mode in Condensed Matter : Higgs Hunting on a Budget

Daniel Arovas University of California, San Diego
November 19, 2013 PIRSA:13110054
Condensed Matter
The amplitude mode is a ubiquitous phenomenon in systems with broken continuous symmetry and effective relativistic dynamics, and has been observed in magnets, charge density waves, cold atom systems, and superconductors. It is a simple analog of the Higgs boson of particle physics. I will discuss the properties of the amplitude mode and its somewhat surprising visibility in two-dimensional systems, recently confirmed in cold atom experiments. The behavior in the vicinity of a quantum critical point will be stressed, comparing theoretical, numerical, and experimental results.
General Relativity for Cosmology - Lecture 18

Achim Kempf University of Waterloo

November 19, 2013 PIRSA:13110005
13/14 PSI - Quantum Field Theory II - Lecture 8

Francois David Commissariat a Energie Atomique (CEA) - Saclay - Institut de Physique Théorique (IPhT)

November 20, 2013 PIRSA:13110017
13/14 PSI - Condensed Matter - Lecture 8
- Anushya Chandran Perimeter Institute for Theoretical Physics
- Roger Melko University of Waterloo
- Xiao-Gang Wen Massachusetts Institute of Technology (MIT) - Department of Physics
November 20, 2013 PIRSA:13110036
Light and matter: towards macroscopic quantum systems

Jacob Taylor Office of Science and Technology
November 20, 2013 PIRSA:13110060
Quantum Information
Advances in quantum engineering and material science are enabling new approaches for building systems that behave quantum mechanically on long time scales and large length scales. I will discuss how microwave and optical technologies in particular are leading to new domains of many-body physics, both classical and quantum, using photons and phonons as the constituent particles. Furthermore, I will highlight practical consequences of these advances, including improved force and acceleration sensing, efficient signal transduction, and topologically robust photonic circuits. Finally, I will consider how such large quantum systems may help us measure and constrain theories of quantum gravity and gravity-induced decoherence.
Quantum Adversary (Upper) Bound

Shelby Kimmel Massachusetts Institute of Technology (MIT)
November 20, 2013 PIRSA:13110090
Quantum Information
I discuss a technique - the quantum adversary upper bound - that uses the structure of quantum algorithms to gain insight into the quantum query complexity of Boolean functions. Using this bound, I show that there must exist an algorithm for a certain Boolean formula that uses a constant number of queries. Since the method is non-constructive, it does not give information about the form of the algorithm. After describing the technique and applying it to a class of functions, I will outline quantum algorithms that match the non-constructive bound.
13/14 PSI - Quantum Field Theory II - Lecture 9

Francois David Commissariat a Energie Atomique (CEA) - Saclay - Institut de Physique Théorique (IPhT)

November 21, 2013 PIRSA:13110018
13/14 PSI - Condensed Matter - Lecture 9
- Anushya Chandran Perimeter Institute for Theoretical Physics
- Roger Melko University of Waterloo
- Xiao-Gang Wen Massachusetts Institute of Technology (MIT) - Department of Physics
November 21, 2013 PIRSA:13110037
Generalized Kahler geometry and T-duality (no audio)

Marco Gualtieri University of Toronto

November 19, 2004 PIRSA:04110016

Please Note: There is no audio for most presentations from November 18th due to technical issues. We appologize to presenters and interested parties for this inconvenience.
Charged particle motion in magnetized black holes

Valeri Frolov University of Alberta
November 21, 2013 PIRSA:13110066
Strong Gravity
There exist evidences that magnetic field in the vicinity of astrophysical black holes plays an important role. In particular it is required for explanation of such phenomenon as jet formation. Study of such problems in all their complexity requires 3D numerical simulations of the magnetohydrodynamics in a strong gravitational field. Quite often when dealing with such a complicated problem it is instructive to consider first its simplifications, which can be treated either analytically, or by integrating ordinary differential equations. Motion of a charged particle in a weakly magnetized black hole is an important example. We consider a non-rotating black hole in the weak magnetic field which is homogeneous at infinity. In the talk I discuss the following problems: How does such a magnetic field affect charged particle motion in the equatorial plane? How does it change the radius of the innermost stable circular orbits (ISCO) and period of rotation? I shall demonstratethat the magnetic field increases the efficiency of the energy extraction from the black hole and that magnetized black holes can be used as "particle accelerators". Finally, I shall discuss out-of-equatorial-plane motion and demonstrate that it is chaotic. Possible applications of these results to astrophysics are briefly discussed.
Dimensional reduction in the sky
November 21, 2013 PIRSA:13110059
Quantum Gravity
In several approaches to quantum-gravity, the spectral dimension of spacetime runs from the standard value of 4 in the infrared (IR) to a smaller value in the ultraviolet (UV). Describing this running in terms of deformed dispersion relations, I show that a striking cosmological implication is that that UV behavior leading to 2 spectral dimensions results in an exactly scale-invariant spectrum of vacuum scalar and tensor fluctuations. I discuss scenarios that break exact scale-invariance and show that the tensor to scalar ratio is fixed by the UV ratio between the speed of gravity and the speed of light. Cosmological perturbations in this framework display a wavelength-dependent speed of light, but by transforming to a suitable "rainbow frame" this feature can be removed, at the expense of modifying gravity. In particular it turns out that the following concepts are closely connected: scale-invariance of vacuum fluctuations, conformal invariance of the gravitational coupling, UV reduction to spectral dimension 2 in position space and UV reduction to Hausdorff dimension 2 in energy-momentum space.

Title	Speaker(s)	Date	Collection	Type	Info
New Light Species and the CMB - Joint Cosmology/Particle Physics Seminar	Christopher Brust	2013‑11‑19	Particle Physics	Scientific Series	View details
The Amplitude Mode in Condensed Matter : Higgs Hunting on a Budget	Daniel Arovas	2013‑11‑19	Condensed Matter	Scientific Series	View details
General Relativity for Cosmology - Lecture 18	Achim Kempf	2013‑11‑19	General Relativity for Cosmology - 2013	Course	View details
13/14 PSI - Quantum Field Theory II - Lecture 8	Francois David	2013‑11‑20	13/14 PSI - Quantum Field Theory II	Course	View details
13/14 PSI - Condensed Matter - Lecture 8	Anushya Chandran, Roger Melko, Xiao-Gang Wen	2013‑11‑20	13/14 PSI - Condensed Matter	Course	View details
Light and matter: towards macroscopic quantum systems	Jacob Taylor	2013‑11‑20	Colloquium	Scientific Series	View details
Quantum Adversary (Upper) Bound	Shelby Kimmel	2013‑11‑20	Perimeter Institute Quantum Discussions	Scientific Series	View details
13/14 PSI - Quantum Field Theory II - Lecture 9	Francois David	2013‑11‑21	13/14 PSI - Quantum Field Theory II	Course	View details
13/14 PSI - Condensed Matter - Lecture 9	Anushya Chandran, Roger Melko, Xiao-Gang Wen	2013‑11‑21	13/14 PSI - Condensed Matter	Course	View details
Generalized Kahler geometry and T-duality (no audio)	Marco Gualtieri	2004‑11‑19	Thematic Program on The Geometry of String Theory 2004 - 2005: Mirror Symmetry	Other	View details
Charged particle motion in magnetized black holes	Valeri Frolov	2013‑11‑21	Strong Gravity	Scientific Series	View details
Dimensional reduction in the sky		2013‑11‑21	Quantum Gravity	Scientific Series	View details

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