Moduli-Induced Gravitino Problem

Motoi Endo, Koichi Hamaguchi, and Fuminobu Takahashi
Phys. Rev. Lett. 96, 211301 – Published 1 June 2006

Abstract

We investigate the cosmological moduli problem by studying a modulus decay in detail and find that the branching ratio of the gravitino production is generically of O(0.011), which causes another cosmological disaster. Consequently, the cosmological moduli problem cannot be solved simply by making the modulus mass heavier than 100 TeV. We also illustrate our results by explicitly calculating the branching ratio into the gravitinos in the mixed modulus-anomaly model.

  • Figure
  • Received 10 February 2006

DOI:https://doi.org/10.1103/PhysRevLett.96.211301

©2006 American Physical Society

Authors & Affiliations

Motoi Endo1,2, Koichi Hamaguchi1, and Fuminobu Takahashi1,2

  • 1Deutsches Elektronen Synchrotron DESY, Notkestrasse 85, 22607 Hamburg, Germany
  • 2Institute for Cosmic Ray Research, University of Tokyo, Chiba 277-8582, Japan

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Issue

Vol. 96, Iss. 21 — 2 June 2006

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