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Predicting big bang deuterium

Journal Article · · Astrophysical Journal
DOI:https://doi.org/10.1086/176845· OSTI ID:281670
; ; ; ;  [1]
  1. Department of Physics, Ohio State University, Columbus, Ohio 43210 (United States)
We present new upper and lower bounds to the primordial abundances of deuterium and {sup 3}He based on observational data from the solar system and the interstellar medium. Independent of any model for the primordial production of the elements we find (at the 95{percent} C.L.): 1.5{times}10{sup {minus}5}{le}(D/H){sub {ital P}}{le}10.0{times}10{sup {minus}5} and ({sup 3}He/H){sub {ital P}}{le}2.6{times}10{sup {minus}5}. When combined with the predictions of standard big bang nucleosynthesis, these constraints lead to a 95{percent} C.L. bound on the primordial abundance deuterium: (D/H){sub best}=(3.5{sup +2.7}{sub {minus}1.8}){times}10{sup {minus}5}. Measurements of deuterium absorption in the spectra of high-redshift QSOs will directly test this prediction. The implications of this prediction for the primordial abundances of {sup 4}He and {sup 7}Li are discussed, as well as those for the universal density of baryons. {copyright} {ital 1996 The American Astronomical Society.}
Research Organization:
Ohio State University Research Foundation
DOE Contract Number:
AC02-76ER01545
OSTI ID:
281670
Journal Information:
Astrophysical Journal, Journal Name: Astrophysical Journal Journal Issue: 2 Vol. 458; ISSN ASJOAB; ISSN 0004-637X
Country of Publication:
United States
Language:
English

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