Structure Formation Constraints
Structure Formation Constraints is a theoretical framework that specifies the conditions under which cosmological models of dark matter must reproduce the observed large-scale structure of the universe, distinguishing it from other dark matter constraints by its focus on the timing, distribution, and hierarchical growth of cosmic structures.
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20.1K
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832
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377
Institutions
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2017–2026
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Structure Formation with a Self-Tuning Scalar Field
Pedro G. Ferreira, Michael Joyce · Physical Review Letters · 1997 · 546 citations · Full text
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Centre National de la Recherche Scientifique
Paris, France
13 h-index
23 publications
1.9K citations
The University of Tokyo
Tokyo, Japan
11 h-index
18 publications
993 citations
University of Cambridge
Cambridge, United Kingdom
11 h-index
20 publications
1.2K citations
University of California, Santa Cruz
Santa Cruz, United States
10 h-index
16 publications
689 citations
Commissariat à l'Énergie Atomique et aux Énergies Alternatives
Paris, France
9 h-index
18 publications
2.8K citations
CEA Paris-Saclay
Gif-sur-Yvette, France
9 h-index
18 publications
2.8K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
9 h-index
12 publications
780 citations
University of California, Berkeley
Berkeley, United States
9 h-index
24 publications
1.9K citations
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JCAP · 45 publications · 2.4K citations
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32 publications · 2.5K citations
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ApJ · 22 publications · 1.3K citations
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19 publications · 1.3K citations
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14 publications · 1.5K citations
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