• Open Access

Gravitino thermal production revisited

Helmut Eberl, Ioannis D. Gialamas, and Vassilis C. Spanos
Phys. Rev. D 103, 075025 – Published 23 April 2021

Abstract

We calculate the gravitino production rate, computing its one-loop thermal self-energy. Gravitino production processes that do not result through thermal cuts of its self-energy, have been identified and taken into account. Correcting analytical errors and numerical approximations in the previous calculations, we present our result. This deviates from the latest estimation by almost 10%. More importantly, we provide a convenient formula, for calculating the gravitino production rate and its thermal abundance, as a function of the reheating temperature of the Universe.

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  • Received 4 November 2020
  • Revised 1 February 2021
  • Accepted 22 March 2021

DOI:https://doi.org/10.1103/PhysRevD.103.075025

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 & Fields

Authors & Affiliations

Helmut Eberl1,*, Ioannis D. Gialamas2,†, and Vassilis C. Spanos2,‡

  • 1Institut für Hochenergiephysik der Österreichischen Akademie der Wissenschaften, A–1050 Vienna, Austria
  • 2National and Kapodistrian University of Athens, Department of Physics, Section of Nuclear & Particle Physics, GR–157 84 Athens, Greece

  • *helmut.eberl@oeaw.ac.at
  • i.gialamas@phys.uoa.gr
  • vspanos@phys.uoa.gr

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Issue

Vol. 103, Iss. 7 — 1 April 2021

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