Big bang nucleosynthesis constraints on hadronically and electromagnetically decaying relic neutral particles

By K. Jedamzik. 2006

382 citations recorded by the source corpus.

Big bang nucleosynthesis in the presence of decaying relic neutral particles is examined in detail. All nonthermal processes important for the determination of light-element abundance yields of {sup 2}H, {sup 3}H, {sup 3}He, {sup 4}He, {sup 6}Li, and {sup 7}Li are coupled to the thermonuclear fusion reactions to obtain comparatively accurate results. Predicted light-element yields are compared to observationally inferred limits on primordial light-element abundances to infer constraints on the abundances and properties of relic decaying particles with decay times in the interval 0.01 sec(less-or-similar sign){tau}{sub X}(less-or-similar sign)10{sup 12} sec. Decaying particles are typically constrained at early times by {sup 4}He or {sup 2}H, at intermediate times by {sup 6}Li, and at large times by the {sup 3}He/{sup 2}H ratio. Constraints are shown for a large number of hadronic branching ratios and decaying particle masses and may be applied to constrain the evolution of the early universe.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/c18bdc01dfc7c1960fd4326e7388c0311d3dfb92

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In Astronomy and Astrophysics

  1. J. March-Russell
  2. S. West
  3. K. Jedamzik
  4. J. Ruderman
  5. A. Falkowski
  6. T. Volansky
  7. L. Hall
  8. R. Iengo

In Nuclear and High Energy Physics

  1. J. March-Russell
  2. S. West
  3. T. Volansky
  4. K. Jedamzik
  5. J. Ruderman
  6. A. Falkowski
  7. L. Hall
  8. Tongyan Lin

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