TY  - JOUR
A1  - Schramm, Stefan
A1  - Steinheimer, Jan
A1  - Dexheimer, Verônica Antocheviz
A1  - Mukherjee, Ayon
T1  - Modeling hybrid stars and hot matter
T2  - Nuclear Physics A
N2  - 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.
KW  - neutron star
KW  - hybrid star
KW  - phase transition
KW  - hyperons
Y1  - 2019
UR  - http://publikationen.ub.uni-frankfurt.de/frontdoor/index/index/docId/77575
UR  - https://nbn-resolving.org/urn:nbn:de:hebis:30:3-775758
SN  - 0375-9474
VL  - 982
SP  - 887
EP  - 890
PB  - Elsevier
CY  - Amsterdam
ER  -