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 |