| dc.date.accessioned | 2019-08-26T13:08:42Z | |
| dc.date.accessioned | 2022-10-18T22:29:14Z | |
| dc.date.available | 2019-08-26T13:08:42Z | |
| dc.date.available | 2022-10-18T22:29:14Z | |
| dc.date.created | 2019-08-26T13:08:42Z | |
| dc.date.issued | 2019 | |
| dc.identifier | http://hdl.handle.net/10533/236498 | |
| dc.identifier | 1150847 | |
| dc.identifier | WOS:000468591100037 | |
| dc.identifier.uri | https://repositorioslatinoamericanos.uchile.cl/handle/2250/4467832 | |
| dc.description.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. Keywords. Author Keywords:hadrons; neutron star; thermal field theory | |
| dc.relation | https://www.researchgate.net/publication/329734929_Pions_near_condensation_under_compact_star_conditions | |
| dc.relation | 10.1002/asna.201913585 | |
| dc.relation | info:eu-repo/grantAgreement//1150847 | |
| dc.relation | info:eu-repo/semantics/dataset/hdl.handle.net/10533/93477 | |
| dc.relation | instname: Conicyt | |
| dc.relation | reponame: Repositorio Digital RI2.0 | |
| dc.rights | http://creativecommons.org/licenses/by-nc-nd/3.0/cl/ | |
| dc.rights | info:eu-repo/semantics/openAccess | |
| dc.rights | info:eu-repo/semantics/openAccess | |
| dc.rights | Attribution-NonCommercial-NoDerivs 3.0 Chile | |
| dc.title | Pions near condensation under compact star conditions | |
| dc.type | Articulo | |
