Modeling hybrid stars and hot matter
- The core of neutron stars consists of extremely dense matter at relatively low temperatures. In such an environment the appearance of exotic strongly interacting particles beyond nucleons appears quite natural. In this context we consider hybrid stars that, in addition to nucleons and hyperons, also contain quarks as further degrees of freedom. We investigate the impact of quarks on the properties of these compact stars. In addition, we discuss new constraints on such objects arising from the recently measured gravitational wave signal of two merging neutron stars.
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| Author: | Stefan SchrammGND, Jan SteinheimerORCiDGND, Verônica Antocheviz DexheimerORCiDGND, Ayon MukherjeeORCiDGND |
|---|---|
| URN: | urn:nbn:de:hebis:30:3-775758 |
| DOI: | https://doi.org/10.1016/j.nuclphysa.2018.09.067 |
| ISSN: | 0375-9474 |
| Parent Title (English): | Nuclear Physics A |
| Publisher: | Elsevier |
| Place of publication: | Amsterdam |
| Document Type: | Article |
| Language: | English |
| Date of Publication (online): | 2019/01/22 |
| Date of first Publication: | 2019/01/22 |
| Publishing Institution: | Universitätsbibliothek Johann Christian Senckenberg |
| Release Date: | 2023/10/12 |
| Tag: | hybrid star; hyperons; neutron star; phase transition |
| Volume: | 982 |
| Page Number: | 4 |
| First Page: | 887 |
| Last Page: | 890 |
| HeBIS-PPN: | 517297825 |
| Institutes: | Physik |
| Wissenschaftliche Zentren und koordinierte Programme / Frankfurt Institute for Advanced Studies (FIAS) | |
| Dewey Decimal Classification: | 5 Naturwissenschaften und Mathematik / 53 Physik / 530 Physik |
| Sammlungen: | Universitätspublikationen |
| Licence (German): |  Creative Commons - CC BY-NC-ND - Namensnennung - Nicht kommerziell - Keine Bearbeitungen 4.0 International |
