Helium photodisintegration and nucleosynthesis: Implications for topological defects, high-energy cosmic rays, and massive black holes

Mar, 1995
20 pages
Published in:
  • Phys.Rev.D 52 (1995) 6682-6693
e-Print:
Report number:
  • FERMILAB-PUB-95-051-A

Citations per year

199520022009201620210246810
Abstract: (arXiv)
We consider the production of 3^3He and 2^2H by 4^4He photodisintegration initiated by non-thermal energy releases during early cosmic epochs. We find that this process cannot be the predominant source of primordial 2^2H since it would result in anomalously high 3^3He/D ratios in conflict with standard chemical evolution assumptions. We apply this fact to constrain topological defect models of highest energy cosmic ray (HECR) production. Such models have been proposed as possible sources of ultrahigh energy particles and gamma-rays with energies above 102010^{20}eV. The constraints on these models derived from 4^4He-photodisintegration are compared to corresponding limits from spectral distortions of the cosmic microwave background radiation (CMBR) and from the observed diffuse gamma-ray background. It is shown that for reasonable primary particle injection spectra superconducting cosmic strings, unlike ordinary strings or annihilating monopoles, cannot produce the HECR flux at the present epoch without violating at least the 4^4He-photodisintegration bound. The constraint from the diffuse gamma-ray background rules out the dominant production of HECR by the decay of Grand Unification particles in models with cosmological evolution assuming standard fragmentation functions. Constraints on massive black hole induced photodisintegration are also discussed.
  • cosmological model
  • helium: photofission
  • light nucleus: production
  • production: light nucleus
  • cosmic radiation: production
  • production: cosmic radiation
  • defect: topological
  • photon: cosmic radiation
  • black hole: massive
  • massive: black hole