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GiRaFFE: an open-source general relativistic force-free electrodynamics code. (English) Zbl 1380.83003
83-08 Computational methods for problems pertaining to relativity and gravitational theory
83C22 Einstein-Maxwell equations
76W05 Magnetohydrodynamics and electrohydrodynamics
85A30 Hydrodynamic and hydromagnetic problems in astronomy and astrophysics
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[1] Abbott B P et al 2016 GW151226: observation of gravitational waves from a 22-solar-mass binary black hole coalescence Phys. Rev. Lett.116 241103
[2] Abbott B P et al 2016 Observation of gravitational waves from a binary black hole merger Phys. Rev. Lett.116 061102
[3] Alic D, Moesta P, Rezzolla L, Zanotti O and Jaramillo J L 2012 Accurate simulations of binary black-hole mergers in force-free electrodynamics Astrophys. J.754 36
[4] Arnowitt R, Deser S and Misner C W 1959 Dynamical structure and definition of energy in general relativity Phys. Rev.116 1322-30 · Zbl 0092.20704
[5] Balsara D and Spicer D S 1999 A staggered mesh algorithm using high order godunov fluxes to ensure solenoidal magnetic fields in magnetohydrodynamic simulations J. Comput. Phys.149 270292 · Zbl 0936.76051
[6] Belczynski K, Kalogera V and Bulik T 2002 A comprehensive study of binary compact objects as gravitational wave sources: evolutionary channels, rates, and physical properties Astrophys. J.572 407-31
[7] Berger E 2014 Short-duration gamma-ray bursts Annu. Rev. Astron. Astrophys.52 43-105
[8] Blandford R D and Znajek R L 1977 Electromagnetic extraction of energy from Kerr black holes Mon. Not. R. Astron. Soc.179 433
[9] Brown J D, Diener P, Sarbach O, Schnetter E and Tiglio M 2009 Turduckening black holes: an analytical and computational study Phys. Rev. D 79 044023
[10] Cao G, Zhang L and Sun S 2015 The spectral simulations of axisymmetric force-free pulsar magnetosphere Mon. Not. R. Astron. Soc.455 4267
[11] Cao G, Zhang L and Sun S 2016 An oblique pulsar magnetosphere with a plasma conductivity Mon. Not. R. Astron. Soc.461 1068
[12] Colella P and Woodward P R 1984 The piecewise parabolic method (PPM) for gas-dynamical simulations J. Comput. Phys.54 174-201 · Zbl 0531.76082
[13] Collaborative Effort 2011 Einstein Toolkit for Relativistic Astrophysics Astrophys. Source Code Libr. (http://ascl.net/1102.014)
[14] Connaughton V et al 2016 Fermi GBM observations of LIGO gravitational-wave event GW150914 Astrophys. J. Lett.826 L6
[15] Contopoulos I, Kazanas D and Fendt C 1999 The axisymmetric pulsar magnetosphere Astrophys. J.511 351
[16] Cook G B 2000 Initial data for numerical relativity Living Rev. Relativ.3 5
[17] Del Zanna L, Bucciantini N and Londrillo P 2003 An efficient shock-capturing central-type scheme for multidimensional relativistic flows. II. Magnetohydrodynamics Astron. Astrophys.400 397-413 · Zbl 1222.76122
[18] Drell S D, Foley H M and Ruderman M A 1965 Drag and propulsion of large satellites in the ionosphere: an Alfvén propulsion engine in space J. Geophys. Res.70 3131-45
[19] Etienne Z B, Paschalidis V, Haas R, Mösta P and Shapiro S L 2015 IllinoisGRMHD: an open-source, user-friendly GRMHD code for dynamical spacetimes Class. Quantum Grav.32 175009 · Zbl 1327.83153
[20] Etienne Z B, Paschalidis V, Liu Y T and Shapiro S L 2012 Relativistic magnetohydrodynamics in dynamical spacetimes: improved electromagnetic gauge condition for adaptive mesh refinement grids Phys. Rev. D 85 024013
[21] Farris B D, Gold R, Paschalidis V, Etienne Z B and Shapiro S L 2012 Binary black hole mergers in magnetized disks: simulations in full general relativity Phys. Rev. Lett.109 221102
[22] Goldreich P and Lynden-Bell D 1969 Io, a jovian unipolar inductor Astrophys. J.156 59-78
[23] Harten A, Lax P D and van Leer B J 1983 On upstream differencing and Godunov-type schemes for hyperbolic conservation laws SIAM Rev.25 35-61 · Zbl 0565.65051
[24] Husa S, Hinder I and Lechner C 2006 Kranc: a mathematica package to generate numerical codes for tensorial evolution equations Comput. Phys. Commun.174 983-1004 · Zbl 1196.68327
[25] Komissarov S S 2002 Time-dependent, force-free, degenerate electrodynamics Mon. Not. R. Astron. Soc.336 759
[26] Komissarov S S 2004 Electrodynamics of black hole magnetospheres Mon. Not. R. Astron. Soc.350 407
[27] Komissarov S S 2005 Observations of the Blandford-Znajek and the MHD penrose processes in computer simulations of black hole magnetospheres Mon. Not. R. Astron. Soc.359 801
[28] Komissarov S S 2006 Simulations of the axisymmetric magnetospheres of neutron stars Mon. Not. R. Astron. Soc.367 19
[29] Kranc: Kranc assembles numerical code http://kranccode.org/
[30] Lehner L, Palenzuela C, Liebling S L, Thompson C and Hanna C 2012 Intense electromagnetic outbursts from collapsing hypermassive neutron stars Phys. Rev. D 86 104035
[31] McKinney J C 2006 General relativistic force-free electrodynamics: a new code and applications to black hole magnetospheres Mon. Not. R. Astron. Soc.367 1797
[32] McKinney J C 2006 Relativistic force-free electrodynamic simulations of neutron star magnetospheres Mon. Not. R. Astron. Soc.368 L30
[33] McKinney J C and Gammie C F 2004 A measurement of the electromagnetic luminosity of a Kerr black hole Astrophys. J.611 977
[34] McWilliams S T and Levin J 2011 Electromagnetic extraction of energy from black-hole-neutron-star binaries Astrophys. J.742 90
[35] Nakar E 2007 Short-hard gamma-ray bursts Phys. Rep.442 166-236
[36] Nathanail A and Contopoulos I 2014 Black hole magnetospheres Astrophys. J.788 186
[37] Palenzuela C, Bona C, Lehner L and Reula O 2011 Robustness of the Blanford-Znajek mechanism Class. Quantum Grav.28 4007
[38] Palenzuela C, Garrett T, Lehner L and Liebling S L 2010 Magnetospheres of black hole systems in force-free plasma Phys. Rev. D 82 044045
[39] Palenzuela C, Lehner L and Liebling S L 2010 Dual jets from binary black holes Science329 927
[40] Parfrey K, Beloborodov A M and Hui L 2012 Introducing PHAEDRA: a new spectral code for simulations of relativistic magnetospheres Mon. Not. R. Astron. Soc.423 1416
[41] Paschalidis V 2017 General relativistic simulations of compact binary mergers as engines of short gamma-ray bursts Class. Quantum Grav.34 084002 · Zbl 1368.83044
[42] Paschalidis V, Etienne Z B and Shapiro S L 2013 General-relativistic simulations of binary black hole-neutron stars: precursor electromagnetic signals Phys. Rev. D 88 021504
[43] Paschalidis V, Ruiz M and Shapiro S L 2015 Relativistic simulations of black hole-neutron star coalescence: the jet emerges Astrophys. J. Lett.806 L14
[44] Paschalidis V and Shapiro S L 2013 A new scheme for matching general relativistic ideal magnetohydrodynamics to its force-free limit Phys. Rev. D 88 104031
[45] Petri J 2016 General-relativistic force-free pulsar magnetospheres Mon. Not. R. Astron. Soc.455 3779
[46] Petri J 2016 Strongly magnetized rotating dipole in general relativity Astron. Astrophys.594 A112
[47] Ruiz M, Lang R N, Paschalidis V and Shapiro S L 2016 Binary neutron star mergers: a jet engine for short gamma-ray bursts Astrophys. J. Lett.824 L6
[48] Schnetter E, Hawley S and Hawke I 2016 Carpet: adaptive mesh refinement for the cactus framework Astrophys. Source Code Libr. (http://ascl.net/1611.016)
[49] Spitkovsky A 2006 Time-dependent force-free pulsar magnetospheres: axisymmetric and oblique rotators Astrophys. J.648 L51
[50] Stone J M and Pringle J E 2001 Magnetohydrodynamical non-radiative accretion flows in two dimensions Mon. Not. R. Astron. Soc.322 461-72
[51] Thorne K S, Price R H and MacDonald D A 1986 Black Holes: the Membrane Paradigm (New Haven, CT: Yale University Press) · Zbl 1374.83002
[52] Tóth G 2000 The ∇⋅B=0 constraint in shock-capturing magnetohydrodynamics codes J. Comput. Phys.161 605-52 · Zbl 0980.76051
[53] Wald R M 1974 Black hole in a uniform magnetic field Phys. Rev. D 10 1680
[54] Zhang F, McWilliams S T and Pfeiffer H P 2015 Stability of exact force-free electrodynamic solutions and scattering from spacetime curvature Phys. Rev. D 92 024049
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