Gravitational waves from binary compact star mergers in the context of strange matter
- n this article we will focus on the appearance of the hadron-quark phase transition and the formation of strange matter in the interior region of the hypermassive neutron star and its conjunction with the spectral properties of the emitted gravitational waves (GWs). A strong hadron-quark phase transition might give rise to a mass-radius relation with a twin star shape and we will show in this article that a twin star collapse followed by a twin star oscillation is feasible. If such a twin star collapse would happen during the postmerger phase it will be imprinted in the GW-signal.
Author: | Matthias HanauskeGND, Zekiye Simay Yilmaz, Christina Mitropoulos, Luciano RezzollaORCiDGND, Horst StöckerORCiDGND |
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URN: | urn:nbn:de:hebis:30:3-718573 |
DOI: | https://doi.org/10.1051/epjconf/201817120004 |
ISSN: | 2100-014X |
Parent Title (English): | EPJ Web of Conferences |
Publisher: | EDP Sciences |
Place of publication: | Les Ulis |
Document Type: | Article |
Language: | English |
Date of Publication (online): | 2018/02/02 |
Date of first Publication: | 2018/02/02 |
Publishing Institution: | Universitätsbibliothek Johann Christian Senckenberg |
Contributing Corporation: | International Conference on Strangeness in Quark Matter (17. : 2017 : Utrecht) |
Release Date: | 2023/02/06 |
Volume: | 171 |
Issue: | 20004 |
Page Number: | 4 |
HeBIS-PPN: | 505769328 |
Institutes: | Physik / 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 - Namensnennung 4.0 |