| Автор | Alessandro Drago |
| Автор | Ubaldo Tambini |
| Дата выпуска | 1999-05-01 |
| dc.description | We study the equation of state (EOS) of quark matter at finite temperature, using a confinement model in which chiral symmetry remains broken in the deconfined phase. Using the Walecka model to describe the hadronic phase, a deconfinement transition at densities slightly larger than nuclear matter saturation density takes place in pre-supernova matter. The presence of a mixed-phase region softens the EOS and open the possibility of a direct explosion. At larger densities the EOS is stiff enough to support a neutron star compatible with observations. |
| Формат | application.pdf |
| Издатель | Institute of Physics Publishing |
| Название | Finite temperature quark matter and supernova explosion |
| Тип | paper |
| DOI | 10.1088/0954-3899/25/5/302 |
| Electronic ISSN | 1361-6471 |
| Print ISSN | 0954-3899 |
| Журнал | Journal of Physics G: Nuclear and Particle Physics |
| Том | 25 |
| Первая страница | 971 |
| Последняя страница | 979 |
| Аффилиация | Alessandro Drago; Dipartimento di Fisica, Università di Ferrara, and INFN, Sezione di Ferrara, Via Paradiso 12, Ferrara 44100, Italy |
| Аффилиация | Ubaldo Tambini; Dipartimento di Fisica, Università di Ferrara, and INFN, Sezione di Ferrara, Via Paradiso 12, Ferrara 44100, Italy |
| Выпуск | 5 |
