dc.contributor.author | Ott, Christian David | |
dc.date.accessioned | 2010-10-12T18:23:23Z | |
dc.date.available | 2010-10-12T18:23:23Z | |
dc.date.issued | 2007 | |
dc.identifier.uri | http://hdl.handle.net/11858/00-1735-0000-0001-30E5-2 | |
dc.description.abstract | I perform and analyse the first ever calculations of rotating stellar iron core collapse in {3+1} general relativity that start out with presupernova models from stellar evolutionary calculations and include a microphysical finite-temperature nuclear equation of state, an approximate scheme for electron capture during collapse and neutrino pressure effects. Based on the results of these calculations, I obtain the to-date most realistic estimates for the gravitational wave signal from collapse, bounce and the early postbounce phase of core collapse supernovae. | |
dc.format.extent | 291 S | |
dc.format.mimetype | application/pdf | |
dc.language.iso | eng | |
dc.publisher | Univ. Potsdam | |
dc.rights.uri | http://e-docs.geo-leo.de/rights | |
dc.subject.ddc | 523 | |
dc.subject.gok | THU 162 | |
dc.subject.gok | TFA 000 | |
dc.title | Stellar iron core collapse in {3+1} general relativity and the gravitational wave signature of core-collapse supernovae | |
dc.type | monograph | |
dc.subject.gokverbal | Supernovae {Astronomie} | |
dc.subject.gokverbal | Relativistische Astrophysik, Gravitation | |
dc.identifier.doi | 10.23689/fidgeo-95 | |
dc.identifier.ppn | 527906093 | |
dc.type.version | publishedVersion | |
dc.relation.collection | Astronomie, Astrophysik, Weltraumforschung | |
dc.description.type | thesis | |