Driving Processes
Driving Processes is a theoretical construct in astrophysics that identifies the physical mechanisms responsible for sustaining pulsational instabilities in stars through the periodic conversion of thermal energy into mechanical work.
154
Publications
7.7K
Citations
516
Authors
286
Institutions
Publications per year
2017–2026
47
Parents
154
Three Detailed Fluctuation Theorems
Massimiliano Esposito, Christian Van den Broeck · Physical Review Letters · 2010 · 411 citations · Full text
Observation of a Dissipative Time Crystal
Hans Keßler, Phatthamon Kongkhambut, Christoph Georges et al. · Physical Review Letters · 2021 · 248 citations · Full text
Observation of a prethermal discrete time crystal
A. Kyprianidis, Francisco Machado, W. Morong et al. · Science · 2021 · 209 citations · Full text
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286
University of California, Berkeley
Berkeley, United States
5 h-index
8 publications
1.3K citations
Universität Hamburg
Hamburg, Germany
5 h-index
14 publications
1.6K citations

Centre National de la Recherche Scientifique
Paris, France
5 h-index
10 publications
689 citations
Université de Montréal
Montreal, Canada
4 h-index
5 publications
172 citations
Harvard University
Cambridge, United States
4 h-index
9 publications
877 citations
University College London
London, United Kingdom
4 h-index
8 publications
446 citations
Ludwig-Maximilians-Universität München
Munich, Germany
4 h-index
7 publications
147 citations
University of Augsburg
Augsburg, Germany
4 h-index
10 publications
652 citations
1–8 of 286
PRL · 12 publications · 1.4K citations
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PRE · 8 publications · 282 citations
8
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7 publications · 308 citations
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PRB · 6 publications · 142 citations
6
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PRA · 6 publications · 135 citations
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