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Please refer to the checklist of the ThuLB for your publishing options. In particular, we present the first consistent, constraint solved simulations of spinning binary neutron stars in full general relativity and the highest mass ratios simulated to date. Binary neutron star merger simulations. Structured data Items portrayed in this file depicts P File change date and time Also, an international tutor service from and for doctoral candidates and postdocs is available to support you taking your first steps in Jena.
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This algorithm allowed us to perform the most accurate simulations of the gravitational collapse of a rotating neutron star.
Binary neutron star merger simulations – Digitale Bibliothek Thüringen
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This page was last edited on 12 Februaryat In addition to pure numerical waveform modeling, we used high-resolution simulations to validate an improved tidal effective-one-body model and show that the new formalism can predict the waveform accurately up to the moment of merger.
Aprilabgedruckt in [http: Introduction to the Web of Science: Binary neutron star mergers are associated with a variety of observable phenomena in the gravitational and electromagnetic spectra and are of great importance in a number of different physical subjects, e. Date 30 April Source http: