Matches in SemOpenAlex for { <https://semopenalex.org/work/W2002144102> ?p ?o ?g. }
- W2002144102 abstract "Numerical simulations of binary black holes---an important predictive tool for the detection of gravitational waves---are computationally expensive, especially for binaries with high mass ratios or with rapidly spinning constituent holes. Existing codes for evolving binary black holes rely on explicit timestepping methods, for which the timestep size is limited by the smallest spatial scale through the Courant-Friedrichs-Lewy condition. Binary inspiral typically involves spatial scales (the spatial resolution required by a small or rapidly spinning hole) which are orders of magnitude smaller than the relevant (orbital, precession, and radiation-reaction) timescales characterizing the inspiral. Therefore, in explicit evolutions of binary black holes, the timestep size is typically orders of magnitude smaller than the relevant physical timescales. Implicit timestepping methods allow for larger timesteps, and they often reduce the total computational cost (without significant loss of accuracy) for problems dominated by spatial rather than temporal error, such as for binary-black-hole inspiral in corotating coordinates. However, fully implicit methods can be difficult to implement for nonlinear evolution systems like the Einstein equations. Therefore, in this paper we explore implicit-explicit (IMEX) methods and use them for the first time to evolve black-hole spacetimes. Specifically, as a first step toward IMEX evolution of a full binary-black-hole spacetime, we develop an IMEX algorithm for the generalized harmonic formulation of the Einstein equations and use this algorithm to evolve stationary and perturbed single-black-hole spacetimes. Numerical experiments explore the stability and computational efficiency of our method." @default.
- W2002144102 created "2016-06-24" @default.
- W2002144102 creator A5045624486 @default.
- W2002144102 creator A5064280165 @default.
- W2002144102 creator A5075664699 @default.
- W2002144102 date "2011-10-12" @default.
- W2002144102 modified "2023-10-14" @default.
- W2002144102 title "Implicit-explicit evolution of single black holes" @default.
- W2002144102 cites W1970213140 @default.
- W2002144102 cites W1972645024 @default.
- W2002144102 cites W1976906776 @default.
- W2002144102 cites W1978595411 @default.
- W2002144102 cites W1989170879 @default.
- W2002144102 cites W1991962363 @default.
- W2002144102 cites W2012004405 @default.
- W2002144102 cites W2027658685 @default.
- W2002144102 cites W2033442379 @default.
- W2002144102 cites W2035880798 @default.
- W2002144102 cites W2040114992 @default.
- W2002144102 cites W2040167847 @default.
- W2002144102 cites W2045467243 @default.
- W2002144102 cites W2048444320 @default.
- W2002144102 cites W2072642665 @default.
- W2002144102 cites W2078437593 @default.
- W2002144102 cites W2089021822 @default.
- W2002144102 cites W2092791625 @default.
- W2002144102 cites W2094258223 @default.
- W2002144102 cites W2095258875 @default.
- W2002144102 cites W2096804551 @default.
- W2002144102 cites W2103931654 @default.
- W2002144102 cites W2104853465 @default.
- W2002144102 cites W2122049987 @default.
- W2002144102 cites W2123597888 @default.
- W2002144102 cites W2137082582 @default.
- W2002144102 cites W2139494815 @default.
- W2002144102 cites W2146272509 @default.
- W2002144102 cites W2155426846 @default.
- W2002144102 cites W2163352838 @default.
- W2002144102 cites W2175135350 @default.
- W2002144102 cites W2179614604 @default.
- W2002144102 cites W3099915293 @default.
- W2002144102 cites W3102065489 @default.
- W2002144102 cites W3102806891 @default.
- W2002144102 cites W3103497273 @default.
- W2002144102 cites W3106379197 @default.
- W2002144102 cites W4238420140 @default.
- W2002144102 cites W4243158510 @default.
- W2002144102 doi "https://doi.org/10.1103/physrevd.84.084023" @default.
- W2002144102 hasPublicationYear "2011" @default.
- W2002144102 type Work @default.
- W2002144102 sameAs 2002144102 @default.
- W2002144102 citedByCount "11" @default.
- W2002144102 countsByYear W20021441022012 @default.
- W2002144102 countsByYear W20021441022013 @default.
- W2002144102 countsByYear W20021441022014 @default.
- W2002144102 countsByYear W20021441022015 @default.
- W2002144102 countsByYear W20021441022016 @default.
- W2002144102 countsByYear W20021441022017 @default.
- W2002144102 countsByYear W20021441022018 @default.
- W2002144102 countsByYear W20021441022019 @default.
- W2002144102 countsByYear W20021441022022 @default.
- W2002144102 crossrefType "journal-article" @default.
- W2002144102 hasAuthorship W2002144102A5045624486 @default.
- W2002144102 hasAuthorship W2002144102A5064280165 @default.
- W2002144102 hasAuthorship W2002144102A5075664699 @default.
- W2002144102 hasBestOaLocation W20021441021 @default.
- W2002144102 hasConcept C104954878 @default.
- W2002144102 hasConcept C11413529 @default.
- W2002144102 hasConcept C121332964 @default.
- W2002144102 hasConcept C121864883 @default.
- W2002144102 hasConcept C130187892 @default.
- W2002144102 hasConcept C190330329 @default.
- W2002144102 hasConcept C31258907 @default.
- W2002144102 hasConcept C32602459 @default.
- W2002144102 hasConcept C33923547 @default.
- W2002144102 hasConcept C41008148 @default.
- W2002144102 hasConcept C44715290 @default.
- W2002144102 hasConcept C44870925 @default.
- W2002144102 hasConcept C48372109 @default.
- W2002144102 hasConcept C50341732 @default.
- W2002144102 hasConcept C62520636 @default.
- W2002144102 hasConcept C74172769 @default.
- W2002144102 hasConcept C74650414 @default.
- W2002144102 hasConcept C89305328 @default.
- W2002144102 hasConcept C94375191 @default.
- W2002144102 hasConceptScore W2002144102C104954878 @default.
- W2002144102 hasConceptScore W2002144102C11413529 @default.
- W2002144102 hasConceptScore W2002144102C121332964 @default.
- W2002144102 hasConceptScore W2002144102C121864883 @default.
- W2002144102 hasConceptScore W2002144102C130187892 @default.
- W2002144102 hasConceptScore W2002144102C190330329 @default.
- W2002144102 hasConceptScore W2002144102C31258907 @default.
- W2002144102 hasConceptScore W2002144102C32602459 @default.
- W2002144102 hasConceptScore W2002144102C33923547 @default.
- W2002144102 hasConceptScore W2002144102C41008148 @default.
- W2002144102 hasConceptScore W2002144102C44715290 @default.
- W2002144102 hasConceptScore W2002144102C44870925 @default.
- W2002144102 hasConceptScore W2002144102C48372109 @default.
- W2002144102 hasConceptScore W2002144102C50341732 @default.
- W2002144102 hasConceptScore W2002144102C62520636 @default.