Published August 12, 2010 | Version v1
Journal article

Effects of the variation of fundamental constants on Pop III stellar evolution

  • 1. Centre de Spectrometrie Nucleaire et de Spectrometrie de Masse (CSNSM), UMR 8609, CNRS/IN2P3 and Universite Paris Sud 11, Batiment 104, 91405 Orsay Campus (France)
  • 2. Geneva Observatory, University of Geneva, Maillettes 51, 1290 Sauverny (Switzerland)
  • 3. Physique Nucleaire Theorique et Physique Mathematique, C.P. 229, Universite Libre de Bruxelles (ULB), B-1050 Brussels (Belgium)
  • 4. Institut d'Astrophysique de Paris, UMR-7095 du CNRS, Universite Pierre et Marie Curie, 98 bis bd Arago, 75014 Paris (France)

Description

The effect of variations of the fundamental constants on the thermonuclear rate of the triple alpha reaction, 4He(αα, γ)12C, that bridges the gap between 4He and 12C is investigated. We have followed the evolution of 15 and 60 M· zero metallicity stellar models, up to the end of core helium burning. They are assumed to be representative of the first (Population III) stars. The calculated oxygen carbon abundances resulting from helium burning can then be used to constrain the variation of the fundamental constants.

Additional details

Identifiers

Publishing Information

Journal Title
AIP Conference Proceedings
Journal Volume
1269
Journal Issue
1
Journal Page Range
p. 21-26
ISSN
0094-243X
CODEN
APCPCS

Conference

Title
10. international symposium on origin of matter and evolution of galaxies
Acronym
OMEG-2010
Dates
8-10 Mar 2010
Place
Osaka (Japan)

Optional Information

Notes
(c) 2010 American Institute of Physics