Talks

10201 - 10212 of 18369 Results

Jets Without Jets

Daniele Bertolini Massachusetts Institute of Technology (MIT)

December 04, 2013

PIRSA:13120052

High Energy Physics
Quantum Mechanics as Classical Physics

Charles Sebens University of Michigan–Ann Arbor

December 03, 2013

PIRSA:13120006

Quantum Physics
Fully exploring exotic production of the 125 GeV Higgs

Felix Yu Fermi National Accelerator Laboratory (Fermilab)

December 03, 2013

PIRSA:13120047

High Energy Physics
Acceleration, Then and Now

Cliff Burgess McMaster University

December 03, 2013

PIRSA:13120059

Astrophysics
Cornering Gluinos at the LHC

Jared Evans Rutgers University

December 02, 2013

PIRSA:13120057

High Energy Physics
13/14 PSI - Condensed Matter - Lecture 15

Anushya Chandran Perimeter Institute for Theoretical Physics

Roger Melko University of Waterloo

Xiao-Gang Wen Massachusetts Institute of Technology (MIT) - Department of Physics

November 29, 2013

PIRSA:13110045
13/14 PSI - Quantum Field Theory II - Lecture 15

Francois David CEA Saclay

November 29, 2013

PIRSA:13110026
General Relativity for Cosmology - Lecture 22

Achim Kempf University of Waterloo

November 28, 2013

PIRSA:13110007
Divergences in Spinfoam Quantum Gravity

Aldo Riello Perimeter Institute for Theoretical Physics

November 28, 2013

PIRSA:13110063

General Relativity & Quantum Cosmology
Collisions in AdS and the thermalisation of heavy-ion collisions

Wilke van der Schee European Organization for Nuclear Research (CERN)

November 28, 2013

PIRSA:13110089

General Relativity & Quantum Cosmology
13/14 PSI - Condensed Matter - Lecture 14

Anushya Chandran Perimeter Institute for Theoretical Physics

Roger Melko University of Waterloo

Xiao-Gang Wen Massachusetts Institute of Technology (MIT) - Department of Physics

November 28, 2013

PIRSA:13110044
13/14 PSI - Quantum Field Theory II - Lecture 14

Francois David CEA Saclay

November 28, 2013

PIRSA:13110025

Jets Without Jets

Daniele Bertolini Massachusetts Institute of Technology (MIT)

December 04, 2013

PIRSA:13120052

High Energy Physics

Jets are key tools for physics at the LHC. Usually, jets are identified through a jet algorithm. In this talk, I will present an alternative way of thinking about jets, by showing how a broad class of inclusive jet-based observables can be replaced by event shapes. These event shapes do not require any jet clustering, but they still implement a jet-like pT cut on "jets" with an R-like radius. I will discuss various applications, including event selection at trigger-level, event-wide trimming, and alternative definitions for boosted objects identifiers.
Quantum Mechanics as Classical Physics

Charles Sebens University of Michigan–Ann Arbor

December 03, 2013

PIRSA:13120006

Quantum Physics

On the face of it, quantum physics is nothing like classical physics. Despite its oddity, work in the foundations of quantum theory has provided some palatable ways of understanding this strange quantum realm. Most of our best theories take that story to include the existence of a very non-classical entity: the wave function. Here I offer an alternative which combines elements of Bohmian mechanics and the many-worlds interpretation to form a theory in which there is no wave function. According to this theory, all there is at the fundamental level are particles interacting via Newtonian forces. In this sense, the theory is classical. However, it is still undeniably strange as it posits the existence of many worlds. Unlike the many worlds of the many-worlds interpretation, these worlds are fundamental, not emergent, and are interacting, not causally isolated. The theory will be presented as a fusion of the many-worlds interpretation and Bohmian mechanics, but can also be seen as a foundationally clear version of quantum hydrodynamics. A key strength of this theory is that it provides a simple and compelling story about the connection between the amplitude-squared of the wave function and probability. The theory also gives a natural explanation of the way the wave function transforms under time reversal and Galilean boosts.
Fully exploring exotic production of the 125 GeV Higgs

Felix Yu Fermi National Accelerator Laboratory (Fermilab)

December 03, 2013

PIRSA:13120047

High Energy Physics

I consider the effects of exotic production modes of the 125 GeV Higgs and their impact on Higgs searches and the Higgs discovery. I emphasize that new production modes have been largely overlooked in contemporary tests of the Standard Model nature of the Higgs boson but experimental tests of exotic production modes are viable now or will be soon. I present a couple explicit examples of exotic production arising from chargino-neutralino associated production in the MSSM. As a corollary of this work, I point out that current Higgs coupling fits do not adequately explore the complete space of new physics deviations possible in Higgs measurements.
Acceleration, Then and Now

Cliff Burgess McMaster University

December 03, 2013

PIRSA:13120059

Astrophysics

There is good evidence that the universe underwent an epoch of accelerated expansion sometime in its very early history, and that it is entering a similar phase now. This talk is in two parts. The first part describes what I believe to be the take-home message about inflationary models, coming both from the recent Planck results and from attempts to embed inflation within a UV completion (string theory). I will argue that both point to a particularly interesting class of inflationary models that also evade many of the tuning problems of inflation. These models also turn out to make the tantalizing prediction that the scalar-to-tensor ratio, r, could be just out of reach, being predicted to be proportional to (n_s - 1)^2, where n_s ~ 0.96 is the spectral tilt of the scalar spectrum. The second part provides an update on an approach to solving the "cosmological constant problem", which asks why the vacuum energy seems to gravitate so little. This is the main theoretical obstruction that makes it so difficult to understand the origins of the present epoch of acceleration. In the approach described - Supersymmetric Large Extra Dimensions - observations can be reconciled with a large vacuum energy because the vacuum energy curves the extra dimensions and not the ones measured in cosmology. It leads to a picture of very supersymmetric gravity sector coupled to a completely non-supersymmetric particle-physics sector (which predicts in particular no superpartners to be found at the LHC). The update presented here summarizes the underlying mechanism whereby supersymmetry in the extra dimensions acts to suppress the gravitational effects of quantum fluctuations. Because the large quantum contributions are under control it becomes possible to estimate the size of to be expected of the observed dark energy. For the simplest configuratin the result is of order C (m Mg/4 pi Mp)^4, where m is the heaviest particle on the branes (and so no smaller than the top quark mass), Mg is the extra-dimensional gravity scale (no smaller than 10 TeV due to astrophysical constraints, implying two extra dimensions that are of order a micron in size) and Mp is the 4D Planck mass. C is a constant unsuppressed by symmetry-breaking effects, and C = 6 x 10^6 gives the observed dark energy density, using the smallest values given above for m and Mg. If there is time I will sketch arguments as to why there must be other light degrees of freedom in the theory as well, whose implications might ultimately be used to test the picture.
Cornering Gluinos at the LHC

Jared Evans Rutgers University

December 02, 2013

PIRSA:13120057

High Energy Physics

Gluinos are expected to be light for a natural electroweak scale, but the LHC has not seen them yet. Many possibilities have been proposed to hide natural gluinos in the LHC data, but are these methods really effective? In this talk, I will discuss the current status of kinematically accessible gluinos. By noting the most common features - MET, tops, and high multiplicity - which pervade natural gluino decays, I will argue that there are few places left to hide. I will briefly discuss the remaining weaknesses in LHC coverage and how to bolster them.
13/14 PSI - Condensed Matter - Lecture 15

Anushya Chandran Perimeter Institute for Theoretical Physics

Roger Melko University of Waterloo

Xiao-Gang Wen Massachusetts Institute of Technology (MIT) - Department of Physics

November 29, 2013

PIRSA:13110045
13/14 PSI - Quantum Field Theory II - Lecture 15

Francois David CEA Saclay

November 29, 2013

PIRSA:13110026
General Relativity for Cosmology - Lecture 22

Achim Kempf University of Waterloo

November 28, 2013

PIRSA:13110007
Divergences in Spinfoam Quantum Gravity

Aldo Riello Perimeter Institute for Theoretical Physics

November 28, 2013

PIRSA:13110063

General Relativity & Quantum Cosmology

The most relevant evidences in favour of the Lorentzian EPRL-FK spinfoam model come from its capibility of reproducing the expected semiclassical limit in the large spin regime. The main examples of this are the large spin limit of the vertex amplitude, later extended to arbitrary triangulations, and that of the spinfoam graviton propagator, which was calculated on the simplest possible two complex. These results are very promising. Nonetheless, their relevance may be endangered by the effects associated to radiative corrections. In this seminar, I will focus on the role played by the simplest diverging graph, the so called 'melon graph', which is known to play a fundamental role in tensorial group field theories. In particular, I will discuss its most divergent part and its geometrical interpretation. I will finally comment on the result, with particular attention to its physical consequences, especially in relation with the semiclassical limit of the spinfoam graviton propagator.
Collisions in AdS and the thermalisation of heavy-ion collisions

Wilke van der Schee European Organization for Nuclear Research (CERN)

November 28, 2013

PIRSA:13110089

General Relativity & Quantum Cosmology

The motivation of this seminar is to understand the thermalisation of heavy ion collisions using AdS/CFT. These collisions can be modelled as colliding planar gravitational shock waves. This gives rise to rich and interesting dynamics; wide shocks come to a full stop and expand hydrodynamically, as was previously found by Chesler and Yaffe. High energy collisions (corresponding to thin shocks) pass through each other, after which a plasma forms in the middle, within a proper time 1/T, with T the local temperature at that time. After this I will discuss recent results where we studied the influence of microscopic structure in the longitudinal direction of the shock waves, and thereby found a coherent regime. This has implications for both fluctuations in nucleus-nucleus collisions, and for recent proton-lead collisions at at LHC. The final part will cover a radially expanding calculation, where some simplifications allowed us to solve the model all the way till the final particle spectra, with an interesting comparison with experimental data.
13/14 PSI - Condensed Matter - Lecture 14

Anushya Chandran Perimeter Institute for Theoretical Physics

Roger Melko University of Waterloo

Xiao-Gang Wen Massachusetts Institute of Technology (MIT) - Department of Physics

November 28, 2013

PIRSA:13110044
13/14 PSI - Quantum Field Theory II - Lecture 14

Francois David CEA Saclay

November 28, 2013

PIRSA:13110025

Title	Date	Collection	Type	Info
Jets Without Jets	2013‑12‑04	Particle Physics	Scientific Series	View details
Quantum Mechanics as Classical Physics	2013‑12‑03	Quantum Foundations	Scientific Series	View details
Fully exploring exotic production of the 125 GeV Higgs	2013‑12‑03	Particle Physics	Scientific Series	View details
Acceleration, Then and Now	2013‑12‑03	Cosmology and Gravitation	Scientific Series	View details
Cornering Gluinos at the LHC	2013‑12‑02	Particle Physics	Scientific Series	View details
13/14 PSI - Condensed Matter - Lecture 15	2013‑11‑29	13/14 PSI - Condensed Matter	Course	View details
13/14 PSI - Quantum Field Theory II - Lecture 15	2013‑11‑29	13/14 PSI - Quantum Field Theory II	Course	View details
General Relativity for Cosmology - Lecture 22	2013‑11‑28	General Relativity for Cosmology - 2013	Course	View details
Divergences in Spinfoam Quantum Gravity	2013‑11‑28	Quantum Gravity	Scientific Series	View details
Collisions in AdS and the thermalisation of heavy-ion collisions	2013‑11‑28	Strong Gravity	Scientific Series	View details
13/14 PSI - Condensed Matter - Lecture 14	2013‑11‑28	13/14 PSI - Condensed Matter	Course	View details
13/14 PSI - Quantum Field Theory II - Lecture 14	2013‑11‑28	13/14 PSI - Quantum Field Theory II	Course	View details

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Format results

Jets Without Jets

Quantum Mechanics as Classical Physics

Fully exploring exotic production of the 125 GeV Higgs

Acceleration, Then and Now

Cornering Gluinos at the LHC

13/14 PSI - Condensed Matter - Lecture 15

13/14 PSI - Quantum Field Theory II - Lecture 15

General Relativity for Cosmology - Lecture 22

Divergences in Spinfoam Quantum Gravity

Collisions in AdS and the thermalisation of heavy-ion collisions

13/14 PSI - Condensed Matter - Lecture 14

13/14 PSI - Quantum Field Theory II - Lecture 14

Jets Without Jets

Quantum Mechanics as Classical Physics

Fully exploring exotic production of the 125 GeV Higgs

Acceleration, Then and Now

Cornering Gluinos at the LHC

13/14 PSI - Condensed Matter - Lecture 15

13/14 PSI - Quantum Field Theory II - Lecture 15

General Relativity for Cosmology - Lecture 22

Divergences in Spinfoam Quantum Gravity

Collisions in AdS and the thermalisation of heavy-ion collisions

13/14 PSI - Condensed Matter - Lecture 14

13/14 PSI - Quantum Field Theory II - Lecture 14