Video URL

https://pirsa.org/24020067

Invariant observables in quantum gravity and graviton loop corrections to the Hubble rate and the Newtonian potential - VIRTUAL

Fröb, M. (2024). Invariant observables in quantum gravity and graviton loop corrections to the Hubble rate and the Newtonian potential - VIRTUAL. Perimeter Institute for Theoretical Physics. https://pirsa.org/24020067

Fröb, Markus. Invariant observables in quantum gravity and graviton loop corrections to the Hubble rate and the Newtonian potential - VIRTUAL. Perimeter Institute for Theoretical Physics, Feb. 15, 2024, https://pirsa.org/24020067 

          @misc{ scivideos_PIRSA:24020067,
            doi = {10.48660/24020067},
            url = {https://pirsa.org/24020067},
            author = {Fr{\"o}b, Markus},
            keywords = {Quantum Gravity},
            language = {en},
            title = {Invariant observables in quantum gravity and graviton loop corrections to the Hubble rate and the Newtonian potential - VIRTUAL},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2024},
            month = {feb},
            note = {PIRSA:24020067 see, \url{https://scivideos.org/index.php/pirsa/24020067}}
          }

Markus Fröb Universität Leipzig

DOI 10.48660/24020067
Source Repository PIRSA
Collection
Talk Type Scientific Series
Subject

Abstract

I present work done in the last years on the construction of dynamical coordinate systems for highly symmetric backgrounds, such as Minkowski, de Sitter, and FLRW cosmologies, and which are needed in the relational approach to construct gauge-invariant observables in gravity. I show that it is possible to restrict the inevitable non-local contributions to the past light cone such that the obtained observables are causal. Lastly, I present some applications, namely the leading quantum gravitational corrections to the local expansion rate of our universe (the Hubble rate) and the Newtonian gravitational potential.

Based on arXiv:1711.08470, arXiv:1806.11124, arXiv:2108.11960, arXiv:2109.09753, and arXiv:2303.16218.

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