Spontaneous symmetry breaking in inflationary cosmology: on the fate of Goldstone Bosons
Daniel Boyanovsky

TL;DR
In inflationary cosmology, spontaneous symmetry breaking does not produce massless Goldstone bosons due to infrared effects, leading to massive modes and a first-order phase transition influenced by the Hawking temperature.
Contribution
This paper demonstrates that in de Sitter space, Goldstone bosons acquire a mass and the symmetry breaking transition is first order, contrasting with standard expectations.
Findings
Goldstone modes gain a radiatively generated mass in de Sitter space
Spontaneous symmetry breaking occurs for finite N below a critical Hawking temperature
The transition is first order with a specific jump in the order parameter
Abstract
We argue that in an inflationary cosmology a consequence of the lack of time translational invariance is that spontaneous breaking of a continuous symmetry and Goldstone's theorem \emph{do not} imply the existence of \emph{massless} Goldstone modes. We study spontaneous symmetry breaking in an O(2) model, and implications for O(N) in de Sitter space time. The Goldstone mode acquires a radiatively generated mass as a consequence of infrared divergences, and the continuous symmetry is spontaneously broken for any finite , however there is a \emph{first order phase transition} as a function of the Hawking temperature . For O(2) the symmetry is spontaneously broken for where is the quartic coupling and is the tree level vacuum expectation value and the Goldstone mode acquires a radiatively generated mass $\mathcal{M}^2_\pi…
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