FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2110043261> ?p ?o ?g. }

• W2110043261 endingPage "1055" @default.
• W2110043261 startingPage "1033" @default.
• W2110043261 abstract "Core collapse supernovae are a promising source of detectable gravitational waves. Most of the existing (multidimensional) numerical simulations of core collapse in general relativity were done using approximations of the Einstein field equations. As recently shown by Dimmelmeier et al. (2002a, A&A, 388, 917), Dimmelmeier et al. (2002b, A&A, 393, 523), one of the most interesting such approximations is the so-called conformal flatness condition (CFC) of Isenberg, Wilson; and Mathews. Building on this previous work we present new results from numerical simulations of relativistic rotational core collapse in axisymmetry, with the aim of improving the dynamics and gravitational waveforms. The computer code used for these simulations models the evolution of the coupled system of metric and fluid equations using the formalism, specialized to a new framework for the gravitational field equations we call CFC+. In this approach we add new degrees of freedom to the original CFC equations, which extend them by terms of second post-Newtonian order. The resulting metric equations are still of elliptic type, but the number of equations is significantly augmented in comparison to the original CFC approach. The hydrodynamic evolution and the CFC spacetime metric are calculated with the code developed by Dimmelmeier et al.(2002a, A&A, 388, 917), which has been conveniently extended to account for the additional CFC+ equations. The corrections included in CFC+ are computed by solving a system of elliptic linear equations. The new formalism is assessed with time evolutions of both rotating neutron stars in equilibrium and gravitational core collapse of rotating polytropes. Gravitational wave signals for a comprehensive sample of collapse models are extracted using either the quadrupole formula or directly from the metric. We discuss our results on the dynamics and the gravitational wave emission through a detailed comparison between CFC and CFC+ simulations. The main conclusion is that, for the neutron star spacetimes analyzed in the present work, no significant differences are found among CFC, CFC+, and full general relativity, which highlights the suitability of the former." @default.
• W2110043261 created "2016-06-24" @default.
• W2110043261 creator A5009164035 @default.
• W2110043261 creator A5031691949 @default.
• W2110043261 creator A5043211610 @default.
• W2110043261 creator A5060655229 @default.
• W2110043261 creator A5081605513 @default.
• W2110043261 creator A5088644917 @default.
• W2110043261 creator A5088679659 @default.
• W2110043261 date "2005-08-12" @default.
• W2110043261 modified "2023-10-16" @default.
• W2110043261 title "CFC+: improved dynamics and gravitational waveforms from relativistic core collapse simulations" @default.
• W2110043261 cites W1573219113 @default.
• W2110043261 cites W1963750344 @default.
• W2110043261 cites W1966416137 @default.
• W2110043261 cites W1969992862 @default.
• W2110043261 cites W1971937909 @default.
• W2110043261 cites W1978976062 @default.
• W2110043261 cites W1979270702 @default.
• W2110043261 cites W1981857259 @default.
• W2110043261 cites W1983840127 @default.
• W2110043261 cites W1984873738 @default.
• W2110043261 cites W1987733395 @default.
• W2110043261 cites W1990262081 @default.
• W2110043261 cites W1991440291 @default.
• W2110043261 cites W2014678856 @default.
• W2110043261 cites W2020660424 @default.
• W2110043261 cites W2024195070 @default.
• W2110043261 cites W2026601534 @default.
• W2110043261 cites W2031569358 @default.
• W2110043261 cites W2032475606 @default.
• W2110043261 cites W2032734593 @default.
• W2110043261 cites W2045849629 @default.
• W2110043261 cites W2049955461 @default.
• W2110043261 cites W2073945818 @default.
• W2110043261 cites W2082914221 @default.
• W2110043261 cites W2089337959 @default.
• W2110043261 cites W2095216595 @default.
• W2110043261 cites W2099145118 @default.
• W2110043261 cites W2105635519 @default.
• W2110043261 cites W2119254801 @default.
• W2110043261 cites W2157515937 @default.
• W2110043261 cites W2163394719 @default.
• W2110043261 cites W2462804364 @default.
• W2110043261 cites W3100685757 @default.
• W2110043261 cites W3104382708 @default.
• W2110043261 cites W4211157367 @default.
• W2110043261 cites W4240909640 @default.
• W2110043261 doi "https://doi.org/10.1051/0004-6361:20042602" @default.
• W2110043261 hasPublicationYear "2005" @default.
• W2110043261 type Work @default.
• W2110043261 sameAs 2110043261 @default.
• W2110043261 citedByCount "44" @default.
• W2110043261 countsByYear W21100432612012 @default.
• W2110043261 countsByYear W21100432612013 @default.
• W2110043261 countsByYear W21100432612014 @default.
• W2110043261 countsByYear W21100432612016 @default.
• W2110043261 countsByYear W21100432612017 @default.
• W2110043261 countsByYear W21100432612018 @default.
• W2110043261 countsByYear W21100432612020 @default.
• W2110043261 crossrefType "journal-article" @default.
• W2110043261 hasAuthorship W2110043261A5009164035 @default.
• W2110043261 hasAuthorship W2110043261A5031691949 @default.
• W2110043261 hasAuthorship W2110043261A5043211610 @default.
• W2110043261 hasAuthorship W2110043261A5060655229 @default.
• W2110043261 hasAuthorship W2110043261A5081605513 @default.
• W2110043261 hasAuthorship W2110043261A5088644917 @default.
• W2110043261 hasAuthorship W2110043261A5088679659 @default.
• W2110043261 hasBestOaLocation W21100432611 @default.
• W2110043261 hasConcept C118396296 @default.
• W2110043261 hasConcept C121332964 @default.
• W2110043261 hasConcept C124017977 @default.
• W2110043261 hasConcept C127592171 @default.
• W2110043261 hasConcept C130187892 @default.
• W2110043261 hasConcept C14257148 @default.
• W2110043261 hasConcept C147452769 @default.
• W2110043261 hasConcept C190330329 @default.
• W2110043261 hasConcept C26405456 @default.
• W2110043261 hasConcept C2778530986 @default.
• W2110043261 hasConcept C2780791080 @default.
• W2110043261 hasConcept C33332235 @default.
• W2110043261 hasConcept C44715290 @default.
• W2110043261 hasConcept C44870925 @default.
• W2110043261 hasConcept C62520636 @default.
• W2110043261 hasConcept C74650414 @default.
• W2110043261 hasConceptScore W2110043261C118396296 @default.
• W2110043261 hasConceptScore W2110043261C121332964 @default.
• W2110043261 hasConceptScore W2110043261C124017977 @default.
• W2110043261 hasConceptScore W2110043261C127592171 @default.
• W2110043261 hasConceptScore W2110043261C130187892 @default.
• W2110043261 hasConceptScore W2110043261C14257148 @default.
• W2110043261 hasConceptScore W2110043261C147452769 @default.
• W2110043261 hasConceptScore W2110043261C190330329 @default.
• W2110043261 hasConceptScore W2110043261C26405456 @default.
• W2110043261 hasConceptScore W2110043261C2778530986 @default.
• W2110043261 hasConceptScore W2110043261C2780791080 @default.
• W2110043261 hasConceptScore W2110043261C33332235 @default.
• W2110043261 hasConceptScore W2110043261C44715290 @default.

• next