| Автор | B Kampfer |
| Дата выпуска | 1983-12-01 |
| dc.description | Estimates of the bombarding energies necessary to reach the quark-gluon phase in heavy-ion collisions are presented within a hydrodynamical framework. At intermediate energies (3-7 GeV/nucleon) the quark-gluon matter formed is predicted to be rather cool (below 100 MeV), i.e. much colder than nuclear matter without phase transitions. Further, the consequences of first-order phase transitions from the neutron matter to pion-condensed matter and quark matter are discussed for neutron stars. Quark matter does not fulfil the conditions for the existence of a third stable branch, e.g. stars with quark cores. Because of observational constraints on neutron-star masses, pion condensation is restricted to a narrow first-order phase transition at best. Due to this restriction the rapid growth of a pion-condensed core in a neutron star cannot appear as a supernova-like event as suggested in earlier work. |
| Формат | application.pdf |
| Издатель | Institute of Physics Publishing |
| Название | Phase transitions in dense nuclear matter and consequences for neutron stars |
| Тип | paper |
| DOI | 10.1088/0305-4616/9/12/009 |
| Print ISSN | 0305-4616 |
| Журнал | Journal of Physics G: Nuclear Physics |
| Том | 9 |
| Первая страница | 1487 |
| Последняя страница | 1496 |
| Аффилиация | B Kampfer; Zentralinst. fur Kernforschung Rossendorf, Dresden, East Germany |
| Выпуск | 12 |
