DISSERTATION THULB JENA
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Description Einstein Dissertation eth 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. Collective MPG collaborative workspace: File change date and time Binary neutron star merger simulations. Captions Captions English Add a one-line explanation of what this file represents. Please consider to include the accepted manuscript version of your article into your thesis.
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Binary neutron star merger simulations – Digitale Bibliothek Thüringen
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Aprilabgedruckt in [http: Zitierform konnte nicht geladen werden. This algorithm allowed us to perform the most accurate simulations of the gravitational collapse of a rotating neutron star.
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Throughout the thesis we consider different configurations by varying the spin, the equation of state, and the mass-ratio. Aprilabgedruckt in Annalen der Physik Additionally, new numerical methods were implemented in the existing BAM code, most notably a refluxing algorithm which ensures mass conservation across mesh refinement boundaries.
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Files are available under licenses specified on their description page. Endnote help, individual and general introduction upon request. Furthermore, the effective-one-body model predicts quasi-universal relations, which we found also in full general relativistic jenna for the inspiral and even in the postmerger phase.
In addition to jrna 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.
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Thus, the usage of numerical methods is inevitable.