| dc.contributor.author |
Boden, Andreas |
|
| dc.contributor.author |
Doneva, Daniela D. |
|
| dc.contributor.author |
Kokkotas, Kostas D. |
|
| dc.date.accessioned |
2019-04-09T13:32:29Z |
|
| dc.date.available |
2019-04-09T13:32:29Z |
|
| dc.date.issued |
2019-04 |
|
| dc.identifier.other |
1668927489 |
|
| dc.identifier.uri |
http://hdl.handle.net/10900/87660 |
|
| dc.identifier.uri |
http://nbn-resolving.de/urn:nbn:de:bsz:21-dspace-876608 |
de_DE |
| dc.identifier.uri |
http://dx.doi.org/10.15496/publikation-29046 |
|
| 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 |
ConferencePaper |
de_DE |
| utue.publikation.fachbereich |
Informatik |
de_DE |
| utue.publikation.fakultaet |
7 Mathematisch-Naturwissenschaftliche Fakultät |
de_DE |
| utue.opus.portal |
bwhpc5 |
de_DE |
