Hostname: page-component-76fb5796d-5g6vh Total loading time: 0 Render date: 2024-04-25T16:44:24.582Z Has data issue: false hasContentIssue false
  • English
  • Français

Change in Primordial Abundances Due to a Change in the Primordial Plasma Energy Density

Published online by Cambridge University Press:  25 May 2016

M. Opher  and
R. Opher
M. Opher
Affiliation:
Dept. of Physics, UCLA, Los Angeles, Calif., USA
R. Opher
Affiliation:
Instituto Astronômico e Geofísico - IAG/USP, Av. Miguel Stéfano, 4200 CEP 04301-904 São Paulo, S.P., Brazil

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We recently showed that the energy density of a plasma is appreciably different than previously thought when high frequency plasma fluctuations, ω ≥ kB/ħ, are taken into account (M. Opher &R. Opher, 1999). A change in the primordial plasma energy density changes the primordial expansion rate of the universe, the neutron temperature freeze-out, and the primordial nucleosythesis abundances. The change in the primordial abundances due to the change in the primordial plasma energy density is evaluated, taking into account the high frequency, as well as the low frequency fluctuations of the plasma.

Type
2. Production and Destruction of the Elements
Information
Symposium - International Astronomical Union , Volume 198: The Light Elements and their Evolution , 2000 , pp. 116 - 117
Copyright
Copyright © Astronomical Society of the Pacific 2000 

References

Kolb, E. W. & Turner, M. S. 1990, The Early Universe (Redwood City: Addison-Wesley)Google Scholar
Opher, M. & Opher, R. 1999, Phys. Rev. Lett, 82, 4835 Google Scholar
Viegas, S. M. & Gruenwald, R. 2000, (see article in these proceedings) Google Scholar
Peimbert, M. 2000, (see article in these proceedings) Google Scholar