Light Element Abundances
Light Element Abundances is a cosmological construct that quantifies the relative concentrations of elements such as hydrogen, helium, and lithium in the universe, serving as a critical observational constraint for models of Big Bang nucleosynthesis.
722
Publications
58.4K
Citations
1.8K
Authors
668
Institutions
Publications per year
2017–2026
110
Variants
Primordial Abundances
Parents
722
The Astrophysical Journal · 1998 · 1.2K citations · Full text
Natural Sciences, Astronomy, Physics +13
Primordial nucleosynthesis redux
Terry P. Walker, Gary Steigman, Ho-Shik Kang et al. · The Astrophysical Journal · 1991 · 804 citations
Natural Sciences, Physics, Cosmology +12
1–5 of 722
1.8K
18
h-index
15
h-index
13
h-index
12
h-index
11
h-index
1–5 of 1.8K
668

Centre National de la Recherche Scientifique
Paris, France
37 h-index
140 publications
9.1K citations
The University of Tokyo
Tokyo, Japan
29 h-index
100 publications
6.8K citations
University of Chicago
Chicago, United States
21 h-index
52 publications
19K citations

Australian National University
Canberra, Australia
21 h-index
60 publications
5.1K citations
The University of Texas at Austin
Austin, United States
21 h-index
33 publications
9.4K citations

University of Minnesota
Minneapolis, United States
20 h-index
32 publications
4.7K citations
California Institute of Technology
Pasadena, United States
18 h-index
37 publications
6.2K citations

Fermi National Accelerator Laboratory
Batavia, United States
17 h-index
36 publications
4K citations
1–8 of 668
ApJ · 155 publications · 13.5K citations
60
h-index
54 publications · 3.3K citations
34
h-index
56 publications · 4.1K citations
32
h-index
30 publications · 4.1K citations
24
h-index
26 publications · 3K citations
23
h-index
1–5