Video URL

https://pirsa.org/17100017

Tunneling in Quantum Field Theory and the Ultimate Fate of our Universe

Andreassen, A. (2017). Tunneling in Quantum Field Theory and the Ultimate Fate of our Universe. Perimeter Institute for Theoretical Physics. https://pirsa.org/17100017

Andreassen, Anders. Tunneling in Quantum Field Theory and the Ultimate Fate of our Universe. Perimeter Institute for Theoretical Physics, Oct. 03, 2017, https://pirsa.org/17100017 

          @misc{ scivideos_PIRSA:17100017,
            doi = {10.48660/17100017},
            url = {https://pirsa.org/17100017},
            author = {Andreassen, Anders},
            keywords = {Particle Physics},
            language = {en},
            title = {Tunneling in Quantum Field Theory and the Ultimate Fate of our Universe},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2017},
            month = {oct},
            note = {PIRSA:17100017 see, \url{https://scivideos.org/pirsa/17100017}}
          }

Anders Andreassen Harvard University

DOI 10.48660/17100017
Source Repository PIRSA
Collection
Talk Type Scientific Series
Subject

Abstract

One of the most concrete implications of the discovery of the Higgs boson is that, in the absence of physics beyond the standard model, the long term fate of our universe can now be established through precision calculations. Are we in a metastable minimum of the Higgs potential or the true minimum? If we are in a metastable vacuum, what is its lifetime? To answer these questions, we need to understand tunneling in quantum field theory.

This talk will give an overview of the interesting history of tunneling rate calculations and all of its complications in calculating functional determinants of fluctuations around the bounce solutions. Several problems has persisted for the last four decades, and we present new solutions to these problems that enabled us to calculate exact closed-form expressions of the functional determinant. Applied to the Standard model, we then get the first-ever complete calculation of the lifetime of our universe.