• Open Access

Radiative first-order phase transitions to next-to-next-to-leading order

Andreas Ekstedt, Oliver Gould, and Johan Löfgren
Phys. Rev. D 106, 036012 – Published 16 August 2022

Abstract

We develop new perturbative tools to accurately study radiatively induced first-order phase transitions. Previous perturbative methods have suffered internal inconsistencies and been unsuccessful in reproducing lattice data, which is often attributed to infrared divergences of massless modes (the Linde problem). We employ a consistent power counting scheme to perform calculations and compare our results against lattice data. We conclude that the consistent expansion removes many previous issues and indicates that the infamous Linde problem is not as big a factor in these calculations as previously thought.

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  • Received 24 May 2022
  • Accepted 3 August 2022

DOI:https://doi.org/10.1103/PhysRevD.106.036012

Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI. Funded by SCOAP3.

Published by the American Physical Society

Physics Subject Headings (PhySH)

Particles & FieldsGravitation, Cosmology & Astrophysics

Authors & Affiliations

Andreas Ekstedt1,2,3,*, Oliver Gould4,†, and Johan Löfgren1,‡

  • 1Department of Physics and Astronomy, Uppsala University, Box 516, SE-751 20 Uppsala, Sweden
  • 2II. Institute of Theoretical Physics, Universität Hamburg, D-22761 Hamburg, Germany
  • 3Deutsches Elektronen-Synchrotron DESY, Notkestrasse 85, 22607 Hamburg, Germany
  • 4School of Physics and Astronomy, University Park, University of Nottingham, Nottingham NG7 2RD, United Kingdom

  • *andreas.ekstedt@desy.de
  • oliver.gould@nottingham.ac.uk
  • johan.lofgren@physics.uu.se

Article Text

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Issue

Vol. 106, Iss. 3 — 1 August 2022

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