Baryonic Processes
Baryonic Processes is a theoretical construct in astrophysics that encompasses the physical mechanisms governing the behavior and evolution of ordinary matter—such as gas cooling, star formation, supernova feedback, and chemical enrichment—within galaxies, distinguishing it from dark matter dynamics and large-scale gravitational processes in galaxy formation models.
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Baryonic Features in the Matter Transfer Function
Daniel J. Eisenstein, Wayne Hu · The Astrophysical Journal · 1998 · 2.2K citations · Full text
Baryon- and Lepton-Nonconserving Processes
Steven Weinberg · Physical Review Letters · 1979 · 2.2K citations
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Center for Astrophysics Harvard & Smithsonian, United States
19 publications · 6.2K citations
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Center for Astrophysics Harvard & Smithsonian, United States
18 publications · 6.1K citations
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Centre National de la Recherche Scientifique
Paris, France
35 h-index
446 publications
17.6K citations
University of California, Berkeley
Berkeley, United States
32 h-index
66 publications
7.9K citations
University of Cambridge
Cambridge, United Kingdom
31 h-index
121 publications
7.9K citations

Durham University
Durham, United Kingdom
30 h-index
107 publications
14K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
28 h-index
73 publications
24.8K citations
Heidelberg University
Heidelberg, Germany
28 h-index
201 publications
13.9K citations
Max Planck Institute for Astrophysics
Garching, Germany
28 h-index
79 publications
9.9K citations
Max Planck Institute for Astronomy
Heidelberg, Germany
28 h-index
59 publications
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ApJ · 104 publications · 15.7K citations
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PRL · 34 publications · 5.2K citations
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