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hep-phFeb 1, 2001
7
citations (OpenAlex)
authors
  • G. Mangano
  • G. Miele
  • S. Pastor
  • M. Peloso
institutions
  • Istituto Nazionale di Fisica Nucleare, Sezione di Napoli
  • Max Planck Institute for Physics
  • University of Bonn
  • University of Naples Federico II
arXiv abstractPDF
paper

Bose Einstein condensation at reheating

arXiv:hep-ph/0102080 · doi:10.1103/PhysRevD.64.123509

Abstract

We discuss the possibility that a perturbative reheating stage after inflation produces a scalar particle gas in a Bose condensate state, emphasizing the possible cosmological role of this phenomenon for symmetry restoration.

4 pages, 4 figures. Revised version, with an improved analysis of the condensate formation

References in corpus (2)

  • Dynamics of Symmetry Breaking and Tachyonic Preheating
  • Nonthermal production of gravitinos and inflatinos

Cited by in corpus (7)

  • Cosmological Constraints on Bose-Einstein-Condensed Scalar Field Dark Matter
  • Bose-Einstein-condensed scalar field dark matter and the gravitational wave background from inflation: new cosmological constraints and its detectability by LIGO
  • Viability of complex self-interacting scalar field as dark matter
  • Reheating and leptogenesis in a SUGRA inspired brane inflation
  • The curvaton as a Bose-Einstein condensate of chiral pseudo Nambu-Goldstone bosons
  • Leptogenesis and rescattering in supersymmetric models
  • Electroweak Asymmetric Early Universe via a Scalar Condensate
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