<> "The repository administrator has not yet configured an RDF license."^^ . <> . . "Statistical modeling of the progenitor evolution and formation of neutron stars and stellar-mass black holes"^^ . "In this thesis, methods are elaborated for constructing efficient, scalable predictive models of stellar evolution, of core collapse supernova (CCSN) outcomes and of the\r\ngravitational wave (GW) emission from binary neutron star (NS) merger remnants, with supervised machine learning techniques. Aided by the predictive models, the following central scientific findings are made. The final fates of massive single and binary-stripped stars undergoing iron core collapse are not only encoded in the pre-SN progenitor structure, but broadly pre-determined already at the end of core helium burning (CHeB). The CCSN model developed in this work is in agreement with estimates of carbon-oxygen core masses ($M_{CO}$) of several observed SN progenitors, which other CCSN recipes typically used in rapid binary population synthesis codes cannot explain. In order to partially address the missing red supergiant problem by failed SNe, stellar evolution models are constrained to have a $M_{CO}$ and a central carbon mass fraction at the end of CHeB within a confined region of parameter space. A NS is the more likely (guaranteed for $M_{CO} \\lesssim 6 \\, M_\\odot$ , and at 85-90 % probability otherwise) compact remnant left behind a successful SN, while fallback black hole formation can under certain pre-SN conditions be excluded. When two\r\nNSs merge, the GW signal of the merger remnant can be reconstructed at advanced LIGO sensitivity up to a source luminosity distance of approximately 12 Mpc. A less massive NS binary at a softer equation of state (EOS) can lead to a similar peak oscillation frequency of the merger remnant as a more massive binary at a stiffer\r\nEOS."^^ . "2025" . . . . . . . "Kiril"^^ . "Maltsev"^^ . "Kiril Maltsev"^^ . . . . . . "Statistical modeling of the progenitor evolution and formation of neutron stars and stellar-mass black holes (PDF)"^^ . . . "Maltsev_PhDthesis.pdf"^^ . . . "Statistical modeling of the progenitor evolution and formation of neutron stars and stellar-mass black holes (Other)"^^ . . . . . . "indexcodes.txt"^^ . . . "Statistical modeling of the progenitor evolution and formation of neutron stars and stellar-mass black holes (Other)"^^ . . . . . . "lightbox.jpg"^^ . . . "Statistical modeling of the progenitor evolution and formation of neutron stars and stellar-mass black holes (Other)"^^ . . . . . . "preview.jpg"^^ . . . "Statistical modeling of the progenitor evolution and formation of neutron stars and stellar-mass black holes (Other)"^^ . . . . . . "medium.jpg"^^ . . . "Statistical modeling of the progenitor evolution and formation of neutron stars and stellar-mass black holes (Other)"^^ . . . . . . "small.jpg"^^ . . "HTML Summary of #36020 \n\nStatistical modeling of the progenitor evolution and formation of neutron stars and stellar-mass black holes\n\n" . "text/html" . . . "310 Statistik"@de . "310 General statistics"@en . . . "520 Astronomie"@de . "520 Astronomy and allied sciences"@en . . . "530 Physik"@de . "530 Physics"@en . .