13–19 Jun 2015
University of Alberta
America/Edmonton timezone
Welcome to the 2015 CAP Congress! / Bienvenue au congrès de l'ACP 2015!

Session

R1-5 Quantum Gravity and Quantum Cosmology (DTP) / Gravité quantique et cosmologie quantique (DPT)

R1-5
18 Jun 2015, 08:45
University of Alberta

University of Alberta

Edmonton, AB

Conveners

R1-5 Quantum Gravity and Quantum Cosmology (DTP) / Gravité quantique et cosmologie quantique (DPT)

  • Arundhati Dasgupta (University of Lethbridge)

Presentation materials

There are no materials yet.

  1. Douglas Gingrich (University of Alberta (CA))
    18/06/2015, 08:45
    Theoretical Physics / Physique théorique (DTP-DPT)
    Invited Speaker / Conférencier invité
    Less than two decades ago, brane world scenarios offered paradigms to reinterpret the 4-D Planck scale as an effective gravity scale arising for a more fundamental lower gravity scale in higher dimensions. These ideas allowed new phenomenological models to be developed and helped guide searches for low-scale gravity at the Tevatron and LHC. One of the most exciting outcomes of these...
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  2. Prof. Philip Stamp (UBC)
    18/06/2015, 09:15
    Theoretical Physics / Physique théorique (DTP-DPT)
    Invited Speaker / Conférencier invité
    It is argued that gravity should cause a breakdown of quantum mechanics, at low energies, accessible in principle to table-top experiments. I show that one can formulate a theory of quantum gravity in which gravitational correlations exist between worldline or worldsheet paths, for the particle or field of interest. Using a generalized equivalence principle, one can give a unique form...
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  3. Soumen Deb (University of Lethbridge)
    18/06/2015, 09:45
    Theoretical Physics / Physique théorique (DTP-DPT)
    Oral (Student, In Competition) / Orale (Étudiant(e), inscrit à la compétition)
    Quantum gravity induced modifications of position/momentum commutation relation brings about a modification of the Heisenberg's uncertainty principle, to what is known as the generalized uncertainty principle (GUP). It has been shown earlier that the GUP-induced corrections to the Schrödinger equation, when applied to a non-relativistic particle in a one-dimensional infinite potential well,...
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  4. Mr Matthew Robbins (University of Lethbridge)
    18/06/2015, 10:00
    Theoretical Physics / Physique théorique (DTP-DPT)
    Oral (Student, In Competition) / Orale (Étudiant(e), inscrit à la compétition)
    As it is currently not possible to access the natural energy scale of quantum gravity (the Planck scale), it is important to look for low-energy effects, e.g. the quantum gravity induced perturbative corrections to non-relativistic quantum mechanics. One such avenue of approach is studying the corrections to the Schrödinger equation via the Generalized Uncertainty Principle (GUP) proposed in...
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  5. Dr Jonathan Ziprick (urn:Google)
    18/06/2015, 10:15
    Theoretical Physics / Physique théorique (DTP-DPT)
    Oral (Non-Student) / orale (non-étudiant)
    We study a pressureless dust coupled to gravity with an arbitrary cosmological constant $\Lambda$ in 2+1 dimensions. This theory has interesting classical solutions and yet remains simple enough to explore the non-perturbative quantization of gravitational degrees of freedom. On the classical side we find the Banados-Teitelboim-Zanelli black hole as a static solution when $\Lambda<0$, and for...
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  6. Keith Ng (University of Waterloo)
    18/06/2015, 10:30
    Theoretical Physics / Physique théorique (DTP-DPT)
    Oral (Student, In Competition) / Orale (Étudiant(e), inscrit à la compétition)
    Classically, the equivalence principle tells us that an observer cannot determine the global structure of spacetime using local measurements. After reviewing previous results demonstrating the sensitivity of detectors to spacetime, I proceed to our most recent result: that one can distinguish between a detector in flat space and one inside a hollow spherical shell by measuring the energy...
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