Supernova constraints on dark flavored sectors

Autor: Robert Ziegler, Jorge Terol-Calvo, Laura Tolos, Jorge Martin Camalich

Publikováno v: Digital.CSIC. Repositorio Institucional del CSIC
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Physical Review D, 103 (12), Art.-Nr.: L121301
Physical Review
Physical Review D

Proto-neutron stars forming a few seconds after core-collapse supernovae are hot and dense environments where hyperons can be efficiently produced by weak processes. By making use of various state-of-the-art supernova simulations combined with the pr

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::36b09fedc53cfa155fc681159674fdad
https://doi.org/10.1103/physrevd.103.l121301