An introduction to effective potential methods in field theory

Fuente: arXiv
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Main Authors: Masina, Isabella, Quiros, Mariano
Format: Preprint
Published: 2025
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author Masina, Isabella
Quiros, Mariano
author_facet Masina, Isabella
Quiros, Mariano
contents In this chapter we give a pedagogical introduction to effective potential methods in field theories. We first review the general functional methods leading to the concept of effective action and effective potential. Focusing on the effective potential we review the methods to compute radiative contributions, starting from the original 1973 seminal paper by Sidney Coleman and Erick Weinberg on one-loop corrections, along with its improvement by the renormalization group equations, as well as some basic results from thermal field theory, including the one-loop thermal corrections to the effective potential. We concentrate on some physical applications of the effective potential: i) the possibility of spontaneous symmetry breaking by radiative corrections, ii) the metastability of the electroweak vacuum in the Standard Model, and iii) the relevance of quantum effects in the dynamics of Higgs inflation. We then apply the previous results to cosmological phase transitions in the early universe and the possibility of generating a stochastic background of gravitational waves as well as primordial black holes.
format Preprint
id arxiv_https___arxiv_org_abs_2501_12713
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle An introduction to effective potential methods in field theory
Masina, Isabella
Quiros, Mariano
High Energy Physics - Phenomenology
High Energy Physics - Theory
In this chapter we give a pedagogical introduction to effective potential methods in field theories. We first review the general functional methods leading to the concept of effective action and effective potential. Focusing on the effective potential we review the methods to compute radiative contributions, starting from the original 1973 seminal paper by Sidney Coleman and Erick Weinberg on one-loop corrections, along with its improvement by the renormalization group equations, as well as some basic results from thermal field theory, including the one-loop thermal corrections to the effective potential. We concentrate on some physical applications of the effective potential: i) the possibility of spontaneous symmetry breaking by radiative corrections, ii) the metastability of the electroweak vacuum in the Standard Model, and iii) the relevance of quantum effects in the dynamics of Higgs inflation. We then apply the previous results to cosmological phase transitions in the early universe and the possibility of generating a stochastic background of gravitational waves as well as primordial black holes.
title An introduction to effective potential methods in field theory
topic High Energy Physics - Phenomenology
High Energy Physics - Theory
url https://arxiv.org/abs/2501.12713