Neutron star oscillations. Linking gravitational waves to microphysics

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Show simple item record Boden, Andreas Doneva, Daniela D. Kokkotas, Kostas D. 2019-04-09T13:32:29Z 2019-04-09T13:32:29Z 2019-04
dc.identifier.other 1668927489
dc.identifier.uri de_DE
dc.description.abstract Fast rotating isolated neutron stars are strong sources of gravitational waves when deformed. One possible source of such a deformation is the occurrence of unstable oscillation modes in the star. Their properties strongly depend on the equation of state, describing the behavior of matter at extremely high densities. A future detection of gravitational waves from rotating neutron stars can thus provide insights not only for relativistic astrophysics, but for nuclear physics as well. en
dc.language.iso en de_DE
dc.publisher Universität Tübingen de_DE
dc.publisher Universität Tübingen de_DE
dc.subject.classification Hochleistungsrechnen de_DE
dc.subject.ddc 004 de_DE
dc.subject.other High Performance Computing en
dc.subject.other bwHPC Symposium de_DE
dc.subject.other HPC en
dc.subject.other Astrophysics en
dc.subject.other GR en
dc.subject.other Neutron Stars en
dc.title Neutron star oscillations. Linking gravitational waves to microphysics en
dc.type InProceedings (Aufsatz / Paper einer Konferenz etc.) de_DE
utue.publikation.fachbereich Informatik de_DE
utue.publikation.fakultaet 7 Mathematisch-Naturwissenschaftliche Fakultät de_DE
utue.opus.portal bwhpc5 de_DE


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