Discontinuous Galerkin methods for general-relativistic hydrodynamics: formulation and application to spherically symmetric spacetimes
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[1] I. Hawke,et al. Numerical simulations of interfaces in relativistic hydrodynamics , 2009, 0909.4217.
[2] C. Palenzuela,et al. Evolutions of Magnetized and Rotating Neutron Stars , 2010, 1001.0575.
[3] Relativistic hydrodynamics on space - like and null surfaces: Formalism and computations of spherically symmetric space-times , 1999, gr-qc/9902018.
[4] Jan S. Hesthaven,et al. Discontinuous Galerkin method for the spherically reduced Baumgarte-Shapiro-Shibata-Nakamura system with second-order operators , 2010, 1008.1820.
[5] Timothy A. Davis,et al. An Unsymmetric-pattern Multifrontal Method for Sparse Lu Factorization , 1993 .
[6] Robert Michael Kirby,et al. Filtering in Legendre spectral methods , 2008, Math. Comput..
[7] L. Rezzolla,et al. Critical phenomena in neutron stars: I. Linearly unstable nonrotating models , 2010, 1007.2809.
[8] O. Zanotti,et al. ECHO: a Eulerian conservative high-order scheme for general relativistic magnetohydrodynamics and magnetodynamics , 2007, 0704.3206.
[9] Three-dimensional numerical general relativistic hydrodynamics. II. Long-term dynamics of single relativistic stars , 2001, gr-qc/0110047.
[10] R. LeVeque. Numerical methods for conservation laws , 1990 .
[11] J. Miralles,et al. Numerical relativistic hydrodynamics: Local characteristic approach. , 1991, Physical review. D, Particles and fields.
[12] Satoshi Matsuoka,et al. Proceedings of the Second International Symposium on Computing in Object-Oriented Parallel Environments , 1998 .
[13] Jinchao Xu,et al. A toy model for testing finite element methods to simulate extreme-mass-ratio binary systems , 2005, gr-qc/0507112.
[14] M. Aurada,et al. Convergence of adaptive BEM for some mixed boundary value problem , 2012, Applied numerical mathematics : transactions of IMACS.
[15] E. Toro. Riemann Solvers and Numerical Methods for Fluid Dynamics , 1997 .
[16] Claudio Canuto,et al. Spectral Methods: Evolution to Complex Geometries and Applications to Fluid Dynamics (Scientific Computation) , 2007 .
[17] B. Giacomazzo,et al. Accurate evolutions of inspiralling and magnetized neutron-stars: equal-mass binaries , 2010, 1009.2468.
[18] Erik Schnetter,et al. Recoil velocities from equal-mass binary-black-hole mergers. , 2007, Physical review letters.
[19] A. Patera. A spectral element method for fluid dynamics: Laminar flow in a channel expansion , 1984 .
[20] A new spherically symmetric general relativistic hydrodynamical code , 1995, astro-ph/9509121.
[21] M. Ansorg,et al. Highly accurate calculation of rotating neutron stars , 2001, astro-ph/0111080.
[22] The trumpet solution from spherical gravitational collapse with puncture gauges , 2010, 1012.3703.
[23] L. Baiotti,et al. Three-dimensional relativistic simulations of rotating neutron-star collapse to a Kerr black hole , 2004, gr-qc/0403029.
[24] Stephan Rosswog,et al. Conservative, special-relativistic smoothed particle hydrodynamics , 2009, J. Comput. Phys..
[25] Scott H. Hawley,et al. Evolutions in 3D numerical relativity using fixed mesh refinement , 2003, gr-qc/0310042.
[26] Chi-Wang Shu,et al. Discontinuous Galerkin Methods: Theory, Computation and Applications , 2011 .
[27] Michael Dumbser,et al. Very high order PNPM schemes on unstructured meshes for the resistive relativistic MHD equations , 2009, J. Comput. Phys..
[28] Timothy A. Davis,et al. A combined unifrontal/multifrontal method for unsymmetric sparse matrices , 1999, TOMS.
[29] Jerome Novak,et al. Combining spectral and shock-capturing methods: A new numerical approach for 3D relativistic core collapse simulations , 2004 .
[30] Simple equations for general relativistic hydrodynamics in spherical symmetry applied to neutron star collapse , 1991 .
[31] F. Curtis Michel,et al. Accretion of matter by condensed objects , 1971 .
[32] Eitan Tadmor,et al. Legendre pseudospectral viscosity method for nonlinear conservation laws , 1993 .
[33] R. F. Tooper. Adiabatic Fluid Spheres in General Relativity. , 1965 .
[34] G. G. Stokes. "J." , 1890, The New Yale Book of Quotations.
[35] A. Quarteroni,et al. Numerical Approximation of Partial Differential Equations , 2008 .
[36] Daoqi Yang,et al. C++ and Object-Oriented Numeric Computing for Scientists and Engineers , 2000, Springer New York.
[37] Douglas N. Arnold,et al. Unified Analysis of Discontinuous Galerkin Methods for Elliptic Problems , 2001, SIAM J. Numer. Anal..
[38] M. Berger,et al. Analysis of Slope Limiters on Irregular Grids , 2005 .
[39] Department of Physics,et al. WhiskyMHD: a new numerical code for general relativistic magnetohydrodynamics , 2007, gr-qc/0701109.
[40] Chi-Wang Shu,et al. Numerical Comparison of WENO Finite Volume and Runge–Kutta Discontinuous Galerkin Methods , 2001, J. Sci. Comput..
[41] S. Noble,et al. Type II critical phenomena of neutron star collapse , 2007, 0709.3527.
[42] Chi-Wang Shu,et al. High order finite difference and finite volume WENO schemes and discontinuous Galerkin methods for CFD , 2001 .
[43] W. Marsden. I and J , 2012 .
[44] Gui-Qiang G. Chen,et al. Gauss‐Green theorem for weakly differentiable vector fields, sets of finite perimeter, and balance laws , 2007, 0709.3673.
[45] Timothy A. Davis,et al. A column pre-ordering strategy for the unsymmetric-pattern multifrontal method , 2004, TOMS.
[46] José A. Font,et al. Numerical Hydrodynamics and Magnetohydrodynamics in General Relativity , 2008, Living reviews in relativity.
[47] L. Rezzolla,et al. Computations of primordial black-hole formation , 2004, gr-qc/0412063.
[48] Parviz Moin,et al. Assessment of high-resolution methods for numerical simulations of compressible turbulence with shock waves , 2010, J. Comput. Phys..
[49] Challenging the paradigm of singularity excision in gravitational collapse. , 2006, Physical review letters.
[50] J. Novak,et al. Spectral Methods for Numerical Relativity , 2007, Living reviews in relativity.
[51] James R. Wilson. Numerical Study of Fluid Flow in a Kerr Space , 1972 .
[52] Relativistic simulations of rotational core collapse I. Methods, initial models, and code tests , 2002, astro-ph/0204288.
[53] Hermano Frid,et al. Extended Divergence-Measure Fields and the Euler Equations for Gas Dynamics , 2003 .
[54] E. Gourgoulhon. 1D numerical relativity applied to neutron star collapse , 1992 .
[55] W. Kastaun. High-resolution shock capturing scheme for ideal hydrodynamics in general relativity optimized for quasistationary solutions , 2006 .
[56] Dusan Agrez,et al. Dynamics of the frequency estimation in the frequency domain , 2007, Proceedings of the 21st IEEE Instrumentation and Measurement Technology Conference (IEEE Cat. No.04CH37510).
[57] Kenzo Watanabe,et al. スイッチド・キャパシタディジタル容量ブリッジ(IEEE Transactions on Instrumentation and Measurement,Vol.IM-33,December,1984) , 1985 .
[58] William J. Rider,et al. Revisiting Wall Heating , 2000 .
[59] P. Cerdá-Durán. Numerical viscosity in hydrodynamics simulations in general relativity , 2009, 0912.1774.
[60] E. Gourgoulhon,et al. Relativistic formalism to compute quasiequilibrium configurations of nonsynchronized neutron star binaries , 1997 .
[61] R. Haber,et al. A spacetime discontinuous Galerkin method for scalar conservation laws , 2004 .
[62] Zhi J. Wang,et al. Spectral (Finite) Volume Method for Conservation Laws on Unstructured Grids. Basic Formulation , 2002 .
[63] Abraham Robinson,et al. COMMUNICATIONS ON PURE AND APPLIED MATHEMATICS , 1956 .
[64] Lilia Krivodonova,et al. Limiters for high-order discontinuous Galerkin methods , 2007, J. Comput. Phys..
[65] Quasi-radial modes of rotating stars in general relativity , 1999, astro-ph/9908359.
[66] Chi-Wang Shu,et al. High Order Strong Stability Preserving Time Discretizations , 2009, J. Sci. Comput..
[67] B. M. Fulk. MATH , 1992 .
[68] D. Arnold. An Interior Penalty Finite Element Method with Discontinuous Elements , 1982 .
[70] Smoothed particle hydrodynamics simulations of ultrarelativistic shocks with artificial viscosity , 1999, astro-ph/9904070.
[71] D. Gottlieb,et al. The CFL condition for spectral approximations to hyperbolic initial-boundary value problems. , 1991 .
[72] Mark Sussman,et al. Tracking discontinuities in hyperbolic conservation laws with spectral accuracy , 2007, J. Comput. Phys..
[73] Relativistic radiative transfer for spherical flows , 1994, astro-ph/9406055.
[74] Nonlinear radial oscillations of neutron stars , 2009, 0906.3088.
[75] C. Canuto. Spectral methods in fluid dynamics , 1991 .
[76] Gerhard Zumbusch,et al. Finite element, discontinuous Galerkin, and finite difference evolution schemes in spacetime , 2009, 0901.0851.
[77] W. F. Noh. Errors for calculations of strong shocks using an artificial viscosity and artificial heat flux , 1985 .
[78] E. Müller,et al. Numerical Hydrodynamics in Special Relativity , 1999, Living reviews in relativity.
[79] Masaru Shibata,et al. Collapse of magnetized hypermassive neutron stars in general relativity. , 2006 .
[80] B. Giacomazzo,et al. Accurate evolutions of inspiralling neutron-star binaries: assessment of the truncation error , 2009, 0901.4955.
[81] Harald P. Pfeiffer,et al. Evolving black hole-neutron star binaries in general relativity using pseudospectral and finite difference methods , 2008, 0809.0002.
[82] H. Huynh,et al. Accurate Monotonicity-Preserving Schemes with Runge-Kutta Time Stepping , 1997 .
[83] Yousef Saad,et al. Iterative methods for sparse linear systems , 2003 .
[84] Richard H. White,et al. Hydrodynamic Calculations of General-Relativistic Collapse , 1966 .
[85] Miguel A. Aloy,et al. THE MISSING LINK: MERGING NEUTRON STARS NATURALLY PRODUCE JET-LIKE STRUCTURES AND CAN POWER SHORT GAMMA-RAY BURSTS , 2011, 1101.4298.
[86] Carlos F. Sopuerta,et al. Finite element computation of the gravitational radiation emitted by a pointlike object orbiting a nonrotating black hole , 2005, gr-qc/0512028.
[87] David L. Meier. Multidimensional Astrophysical Structural and Dynamical Analysis. I. Development of a Nonlinear Finite Element Approach , 1999 .