Pions near condensation under compact star conditions
Abstract
The behavior of pions is studied in systems where their normal leptonic decay is forbidden. When thermal fluctuations are present, a low decay rate results, and as a consequence of lepton recombination, the number of pions remains almost unaltered. Compact star conditions are favorable for the formation of such intermediate state of charged pions: near condensation and almost stable, leading to a continuum source of antineutrinos. In particular, protoneutron stars could be a scenario where this state of matter is relevant.
Más información
Título según WOS: | Pions near condensation under compact star conditions |
Título según SCOPUS: | Pions near condensation under compact star conditions |
Título de la Revista: | ASTRONOMISCHE NACHRICHTEN |
Volumen: | 340 |
Número: | 01-mar |
Editorial: | WILEY-V C H VERLAG GMBH |
Fecha de publicación: | 2019 |
Página de inicio: | 184 |
Página final: | 188 |
Idioma: | English |
DOI: |
10.1002/asna.201913585 |
Notas: | ISI, SCOPUS |