Talks

10849 - 10860 of 18060 Results

Experimental search for quantum gravity - the hard facts

Hugo Beauchemin University of Oxford

October 25, 2012

PIRSA:12100115

General Relativity & Quantum Cosmology
Quantum Field Theory - Lecture 13A

Konstantin Zarembo Nordic Institute for Theoretical Physics

October 25, 2012

PIRSA:12100020

High Energy Physics
Lorentz symmetry: Broken, intact or deformed?

Rafael Sorkin Perimeter Institute for Theoretical Physics

Sabine Hossenfelder Ludwig-Maximilians-Universität München (LMU)

David Mattingly University of New Hampshire

Niayesh Afshordi University of Waterloo

Daniel Sudarsky Universidad Nacional Autónoma De Mexico (UNAM)

Stefano Liberati SISSA International School for Advanced Studies

Joao Magueijo Imperial College London

October 24, 2012

PIRSA:12100108

General Relativity & Quantum Cosmology
12/13 PSI Researcher Presentation

Matthew Johnson York University

October 24, 2012

PIRSA:12100050

Astrophysics
Astrophysical Searches for Quantum Gravity Signals

Jonathan Granot University of Hertfordshire

October 24, 2012

PIRSA:12100058

General Relativity & Quantum Cosmology
Dynamical Dimensional Reduction

Dejan Stojkovic State University of New York (SUNY)

Astrid Eichhorn University of Southern Denmark

Martin Reuter Johannes Gutenberg University Mainz

October 24, 2012

PIRSA:12100104

General Relativity & Quantum Cosmology
Quantum Field Theory - Lecture 12B

Konstantin Zarembo Nordic Institute for Theoretical Physics

October 24, 2012

PIRSA:12100073

High Energy Physics
Condensed Matter - Lecture 12

Assa Auerbach Technion – Israel Institute of Technology

October 24, 2012

PIRSA:12100037

Condensed Matter
Is spacetime fundamentally discrete?

Bianca Dittrich Perimeter Institute for Theoretical Physics

Seth Major Hamilton College

Daniele Oriti Ludwig-Maximilians-Universität München (LMU)

Roberto Percacci SISSA International School for Advanced Studies

Tobias Fritz Universität Innsbruck

October 24, 2012

PIRSA:12100100

Mathematical Physics
Quantum Field Theory - Lecture 12A

Konstantin Zarembo Nordic Institute for Theoretical Physics

October 24, 2012

PIRSA:12100019

High Energy Physics
Cosmological Constant

Ivan Arraut University of Saint Joseph

Stephon Alexander Brown University

Alejandro Satz

Maïté Dupuis Perimeter Institute for Theoretical Physics

Antonino Marciano Fudan University

October 23, 2012

PIRSA:12100126

Astrophysics
Quantum Gravity Effects in Black Holes and Gravitational Waves

Giovanni Amelino-Camelia Sapienza Università di Roma - Dipartimento di Fisica

David Mattingly University of New Hampshire

Nicolas Yunes University of Illinois Urbana-Champaign

Avery Broderick University of Waterloo

October 23, 2012

PIRSA:12100094

General Relativity & Quantum Cosmology

Experimental search for quantum gravity - the hard facts

Hugo Beauchemin University of Oxford

October 25, 2012

PIRSA:12100115

General Relativity & Quantum Cosmology

The LHC has been running for over 2 years and the different experiments have accumulated enough data to find a new particle which could well be the Higgs boson, achieve Standard Model measurements with precision at the percent level, and seriously constrain a large variety of new physics scenarios, giving important hints on what the physics beyond the Standard Model can be and what it cannot be. This presentation will focus on ATLAS and CMS latest searches for new physics in events featuring signatures relevant to theories of quantum gravity. Will be presented the results on searches for large extra dimensions (direct graviton emission, virtual graviton propagation, Kaluza-Klein Randall-Sundrum resonances, etc.) and other TeV-scale gravity phenomena such as black holes (rotating and non-rotating) and string balls production and decay. Results will be reported on each of the various final states investigated for each signals. The results of some searches that are not typically interpreted into bounds on quantum gravity signals, but which could provide complementary information such as the number of possible matter fields compatible with LHC data will also be presented. An attempt to present plausible future reach of the LHC will finally be briefly discussed.
Quantum Field Theory - Lecture 13A

Konstantin Zarembo Nordic Institute for Theoretical Physics

October 25, 2012

PIRSA:12100020

High Energy Physics
Lorentz symmetry: Broken, intact or deformed?

Rafael Sorkin Perimeter Institute for Theoretical Physics

Sabine Hossenfelder Ludwig-Maximilians-Universität München (LMU)

David Mattingly University of New Hampshire

Niayesh Afshordi University of Waterloo

Daniel Sudarsky Universidad Nacional Autónoma De Mexico (UNAM)

Stefano Liberati SISSA International School for Advanced Studies

Joao Magueijo Imperial College London

October 24, 2012

PIRSA:12100108

General Relativity & Quantum Cosmology

Is aether technically natural?
I will discuss whether higher energy Lorentz violation should be considered a natural expectation in theories of quantum gravity with a preferred frame.
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If spacetime is a causal set then Lorentz symmetry is unbroken
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Quantum superpositions of the speed of light
If the metric is an operator, it can exist in superpositions. The simplest case one can look at is a superposition of flat spaces which differ only in the value of the speed of light. I will lay out how such superpositions can be incorporated into quantum field theory, and discuss the fate of Lorentz-invariance in this scenario.
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Relative locality and fate of Lorentz symmetry
In my talk I will briefly introduce the idea of relative locality, being a particular regime of quantum gravity characterized by negligible Planck length and finite Planck mass. Then I will discuss possible scenarios concerning the fate of Lorentz symmetry in this regime.
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Observational constraints on scale hierarchy in Horava-Lifshiftz gravity
Horava-Lifshitz gravity models contain higher order operators suppressed by a characteristic scale, which is required to be parametrically smaller than the Planck scale. We show that recomputed synchrotron radiation constraints from the Crab nebula suffice to exclude the possibility that this scale is of the same order of magnitude as the Lorentz breaking scale in the matter sector. This highlights the need for a mechanism that suppresses the percolation of Lorentz violation in the matter sector and is effective for higher order operators as well.
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Breaking Lorentz invariance: the Universe loves it!
I show how the local Lorentz and / or diffeomorphism invariances may be broken by a varying speed of light, softly or harshly, depending on taste. Regardless of the fundamental implications of such dramas, these smmetry breakings may be of great practical use in cosmology. They may solve the horizon and flatness problesm. A near scale-invariant sprectrum of fluctuation may arise, even without inflation. Distinct observational imprints may be left.
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Quantum Gravity Phenomenology without Lorentz Invariance Violation
Is there hope to see quantum gravity effects if the underlying theory is strictly respecting of Lorentz invariance? I will discuss a novel class of possibilities, suggested by analogy with some simple solid state physics, including one that has lead to an actual experiment, which has placed the first relevant constraints on these kind of effects
12/13 PSI Researcher Presentation

Matthew Johnson York University

October 24, 2012

PIRSA:12100050

Astrophysics
Astrophysical Searches for Quantum Gravity Signals

Jonathan Granot University of Hertfordshire

October 24, 2012

PIRSA:12100058

General Relativity & Quantum Cosmology

Some recent searches for quantum gravity signatures using observations of distant astrophysical sources will be discussed, focusing on the search for Lorentz invariance violation (LIV) in the form of a dependence of the photon propagation speed on its energy. Fermi gamma-ray space telescope observations of ~8 keV to ~30 GeV photons from a short (< 1 s) gamma-ray burst (GRB 090510) at a cosmological distance (z = 0.903), enabled for the first time to put a direct time of flight limit on a possible linear variation of the speed of light with photon energy that is beyond the Planck scale. Parameterizing |v/c-1| = E/E_{QG} our most conservative limits are E_{QG}/E_{Planck} > 1.2, while less conservative limits are up to 1-2 orders of magnitude stricter. Other types of astrophysical searches for LIV will be briefly outlined, along with some prospects for the future.
Dynamical Dimensional Reduction

Dejan Stojkovic State University of New York (SUNY)

Astrid Eichhorn University of Southern Denmark

Martin Reuter Johannes Gutenberg University Mainz

October 24, 2012

PIRSA:12100104

General Relativity & Quantum Cosmology

Dynamical dimensional reduction and Asymptotic Safety
The effective average action approach to Quantum Einstein Gravity (QEG) is discussed as a natural framework for exploring the scale dependent Riemannian geometry and multifractal micro-structure of the effective spacetimes predicted by QEG. Their fractal properties are related to the functional RG flow on theory space, and the special role of the running cosmological constant is emphasized. The prospects of an experimental verification will also be discussed.
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Vanishing dimension: theory and phenomenology
Lower-dimensionality at higher energies has manifold theoretical advantages as recently pointed out. Moreover, it appears that experimental evidence may already exists for it - a statistically significant planar alignment of events with energies higher than TeV has been observed in some earlier cosmic ray experiments. If this alignment is not a fluke, then the LHC should be able to see effects associated with the dimensional crossover. Further, (2+1)-dimensional spacetimes have no gravitational degrees of freedom, and gravity waves cannot be produced in that epoch in the early universe. This places a universal maximum frequency at which primordial gravity waves can propagate, which may be accessible to future gravitational wave detectors such as LISA. In this talk, the theoretical motivation for "vanishing dimensions" as well as generic experimental and observational signature will be discussed
Quantum Field Theory - Lecture 12B

Konstantin Zarembo Nordic Institute for Theoretical Physics

October 24, 2012

PIRSA:12100073

High Energy Physics
Condensed Matter - Lecture 12

Assa Auerbach Technion – Israel Institute of Technology

October 24, 2012

PIRSA:12100037

Condensed Matter
Is spacetime fundamentally discrete?

Bianca Dittrich Perimeter Institute for Theoretical Physics

Seth Major Hamilton College

Daniele Oriti Ludwig-Maximilians-Universität München (LMU)

Roberto Percacci SISSA International School for Advanced Studies

Tobias Fritz Universität Innsbruck

October 24, 2012

PIRSA:12100100

Mathematical Physics

Modelling continuum dynamics on discrete space time
We will discuss perfect discretizations which aim at mirroring exactly continuum physics on a given lattice. Such discretizations avoid typical artifacts like Lorentz violation, energy dissipation, particle doubling and in particular breaking of diffeomorphism symmetry. Thus the question arises how to distinguish such lattice dynamics from continuum physics.

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Turning Weyl’s tile argument into a mathematically rigorous no-go theorem
Weyl's tile argument notes that if space was fundamentally discrete then the set of allowed velocities of a classical particle would not be isotropic. I will generalize Weyl's heuristic argument to a no-go theorem applying to any discrete periodic structure. Since this theorem does not take quantum mechanics into account it should only be regarded as the first step of a program of understanding the phenomenology of discrete spacetimes in a mathematically rigorous way.See arXiv:1109.1963

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On the Observability of Discrete Spatial Geometry
If quantum geometry is an accurate model of microscopic spatial geometry then two related questions arise, one observational and one theoretical: How and at what scale is the discreteness manifest? And, how is the general relativistic limit achieved? These questions will be discussed in the context of studies of a single atom of geometry. It will be shown that the effective scale of the discreteness could be much larger than the Planck scale. Before this scale can be predicted, the relations between discrete geometry, coherent states, and the semiclassical limit need to be clarified. Work towards this goal, using coherent states in spin foams and the spin geometry theorem of Penrose and Moussouris will be described.

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Asymptotic safety and minimal length
Since asymptotic safety - if true - would make a quantum field theory of gavity consistent "up to arbitrarily high energy", it would seem that this notion is incompatible with the existence of a minimal length. I will argue that this is not necessarily the case, due to ambiguity in the notion of minimal length.
Quantum Field Theory - Lecture 12A

Konstantin Zarembo Nordic Institute for Theoretical Physics

October 24, 2012

PIRSA:12100019

High Energy Physics
Cosmological Constant

Ivan Arraut University of Saint Joseph

Stephon Alexander Brown University

Alejandro Satz

Maïté Dupuis Perimeter Institute for Theoretical Physics

Antonino Marciano Fudan University

October 23, 2012

PIRSA:12100126

Astrophysics

Dark Matter and Dark Energy as a Possible Manifestation of a Fundamental Scale
If we take the idea of the Planck length as a fundamental (minimum) scale and if additionally we impose the Cosmological Constant ($Lambda$) as and infrared (IR) cut-off parameter. Then it is possible to demonstrate that Dark Matter effects can emerge as a consequence of an IR-UV mix effect. This opens the possibility of unifying the Dark Energy and Dark matter effects in a single approach.

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Geometric Operators in Loop Quantum Gravity with a Cosmological Constant
Loop quantum gravity is a candidate to describe the quantum gravity regime with zero cosmological constant. One of its key results is that geometric operators such as area angle volume are quantized. Not much is known when the cosmological constant is not zero. It is usually believed that to introduce this parameter in the game we need to use quantum groups. However due to the complicated algebraic structure inherent to quantum groups the geometric operators are not yet properly defined (except the area operator). I will discuss how the use of tensor operators can circumvent the difficulties and allow to construct a natural set of observables. In particular I will construct the natural geometric observables such as angle or volume and discuss some of their implications.

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Interplay Between Cosmological Constant and DSR Scale
I offer brief remarks on several ways in which the cosmological constant could provide a clue toward quantum gravity. I then focus on how DSR-relativistic theories can be made compatible with spacetime expansion (possibly cosmological-constant-governed spacetime expansion), and how this interplay could manifest itself in data.

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Quantum Gravity RG Flow: A Cosmological Limit Cycle
I will discuss evidence for the existence of a limit cycle in the renormalization group for quantum gravity which is visible in a minisuperspace approximation. The emergence of the limit cycle can be studied through a tuning parameter representing the number of dimensions in which fluctuations of the conformal factor are suppressed. At the critical value of the tuning parameter all RG trajectories reaching the UV fixed point have an extended semiclassical regime with a small positive cosmological constant providing a possible model for a viable cosmology without fine-tuning.
Quantum Gravity Effects in Black Holes and Gravitational Waves

Giovanni Amelino-Camelia Sapienza Università di Roma - Dipartimento di Fisica

David Mattingly University of New Hampshire

Nicolas Yunes University of Illinois Urbana-Champaign

Avery Broderick University of Waterloo

October 23, 2012

PIRSA:12100094

General Relativity & Quantum Cosmology

Quantum-gravity effects as noise for gravity-wave detectors
I discuss a mechanism that can allow Planck scale effects to manifest themselves as a source of lof-frequency noise for interferometers. The mechanism requires a discrete formulation of dynamics at the Planck scale.
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Dancing in the Dark: Images of Quantum Black Holes
There have recently been a number of rather surprising suggestions that the quantum nature of black holes is manifested on macroscopic scales. This raises the question of just what the image of such an object should look like. The answer is more than simply academic; with the advent of the Event Horizon Telescope (EHT), a millimetre-wave very long baseline array, it is now possible to probe a handful of supermassive black holes with angular resolutions sufficient to image their horizons. I will discuss what we might expect to see, and how in the near future we will begin to empirically probe the existence of black hole quantum states with horizon scale curvature deviations from general relativity.
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The Irritating Persistence of Horizons
In some approaches to quantum gravity Lorentz invariance is modified. Without Lorentz invariance one can theoretically see behind the usual Killing horizon of a black hole if, for example, one allowed for superluminal propagation. This in turn raises the possibility that one could in principle probe the singularity and the quantum gravity regime. We discuss how Lorentz violating black hole solutions in Einstein-aether theory unfortunately possess another causal boundary behind the Killing horizon that is impenetrable to any superluminal mode. We also detail progress in determining the laws of black hole mechanics and the radiation spectrum from these so-called "universal horizons". Our results suggest that even if superluminal dispersion at high frequencies did exist in nature, singularities and their associated quantum gravity resolutions may very well remain locked behind horizons.

Title	Date	Collection	Type	Info
Experimental search for quantum gravity - the hard facts	2012‑10‑25	Experimental Search for Quantum Gravity 2012	Conference	View details
Quantum Field Theory - Lecture 13A	2012‑10‑25	12/13 PSI - Quantum Field Theory 1	Course	View details
Lorentz symmetry: Broken, intact or deformed?	2012‑10‑24	Experimental Search for Quantum Gravity 2012	Conference	View details
12/13 PSI Researcher Presentation	2012‑10‑24	12/13 PSI Researcher Presentations	Course	View details
Astrophysical Searches for Quantum Gravity Signals	2012‑10‑24	Experimental Search for Quantum Gravity 2012	Scientific Series	View details
Dynamical Dimensional Reduction	2012‑10‑24	Experimental Search for Quantum Gravity 2012	Conference	View details
Quantum Field Theory - Lecture 12B	2012‑10‑24	12/13 PSI - Quantum Field Theory 1	Course	View details
Condensed Matter - Lecture 12	2012‑10‑24	12/13 PSI - Condensed Matter	Course	View details
Is spacetime fundamentally discrete?	2012‑10‑24	Experimental Search for Quantum Gravity 2007	Conference	View details
Quantum Field Theory - Lecture 12A	2012‑10‑24	12/13 PSI - Quantum Field Theory 1	Course	View details
Cosmological Constant	2012‑10‑23	Experimental Search for Quantum Gravity 2012	Conference	View details
Quantum Gravity Effects in Black Holes and Gravitational Waves	2012‑10‑23	Experimental Search for Quantum Gravity 2012	Conference	View details

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Format results

Experimental search for quantum gravity - the hard facts

Quantum Field Theory - Lecture 13A

Lorentz symmetry: Broken, intact or deformed?

12/13 PSI Researcher Presentation

Astrophysical Searches for Quantum Gravity Signals

Dynamical Dimensional Reduction

Quantum Field Theory - Lecture 12B

Condensed Matter - Lecture 12

Is spacetime fundamentally discrete?

Quantum Field Theory - Lecture 12A

Cosmological Constant

Quantum Gravity Effects in Black Holes and Gravitational Waves

Experimental search for quantum gravity - the hard facts

Quantum Field Theory - Lecture 13A

Lorentz symmetry: Broken, intact or deformed?

12/13 PSI Researcher Presentation

Astrophysical Searches for Quantum Gravity Signals

Dynamical Dimensional Reduction

Quantum Field Theory - Lecture 12B

Condensed Matter - Lecture 12

Is spacetime fundamentally discrete?

Quantum Field Theory - Lecture 12A

Cosmological Constant

Quantum Gravity Effects in Black Holes and Gravitational Waves