Literature DB >> 28179823

Numerical Hydrodynamics and Magnetohydrodynamics in General Relativity.

José A Font1.   

Abstract

This article presents a comprehensive overview of numerical hydrodynamics and magneto-hydrodynamics (MHD) in general relativity. Some significant additions have been incorporated with respect to the previous two versions of this review (2000, 2003), most notably the coverage of general-relativistic MHD, a field in which remarkable activity and progress has occurred in the last few years. Correspondingly, the discussion of astrophysical simulations in general-relativistic hydrodynamics is enlarged to account for recent relevant advances, while those dealing with general-relativistic MHD are amply covered in this review for the first time. The basic outline of this article is nevertheless similar to its earlier versions, save for the addition of MHD-related issues throughout. Hence, different formulations of both the hydrodynamics and MHD equations are presented, with special mention of conservative and hyperbolic formulations well adapted to advanced numerical methods. A large sample of numerical approaches for solving such hyperbolic systems of equations is discussed, paying particular attention to solution procedures based on schemes exploiting the characteristic structure of the equations through linearized Riemann solvers. As previously stated, a comprehensive summary of astrophysical simulations in strong gravitational fields is also presented. These are detailed in three basic sections, namely gravitational collapse, black-hole accretion, and neutron-star evolutions; despite the boundaries, these sections may (and in fact do) overlap throughout the discussion. The material contained in these sections highlights the numerical challenges of various representative simulations. It also follows, to some extent, the chronological development of the field, concerning advances in the formulation of the gravitational field, hydrodynamics and MHD equations and the numerical methodology designed to solve them. To keep the length of this article reasonable, an effort has been made to focus on multidimensional studies, directing the interested reader to earlier versions of the review for discussions on one-dimensional works. ELECTRONIC SUPPLEMENTARY MATERIAL: Supplementary material is available for this article at 10.12942/lrr-2008-7.

Year:  2008        PMID: 28179823      PMCID: PMC5256108          DOI: 10.12942/lrr-2008-7

Source DB:  PubMed          Journal:  Living Rev Relativ        ISSN: 1433-8351            Impact factor:   40.429


  31 in total

1.  Relativistic Jets from Collapsars.

Authors: 
Journal:  Astrophys J       Date:  2000-03-10       Impact factor: 5.874

2.  Nonlinear r-modes in rapidly rotating relativistic stars.

Authors:  N Stergioulas; J A Font
Journal:  Phys Rev Lett       Date:  2001-02-12       Impact factor: 9.161

3.  Detecting energy emissions from a rotating black hole.

Authors:  Maurice H P M van Putten; Amir Levinson
Journal:  Science       Date:  2002-02-21       Impact factor: 47.728

4.  Numerical relativistic hydrodynamics: Local characteristic approach.

Authors: 
Journal:  Phys Rev D Part Fields       Date:  1991-06-15

5.  Dynamical determination of the innermost stable circular orbit of binary neutron stars.

Authors:  Pedro Marronetti; Matthew D Duez; Stuart L Shapiro; Thomas W Baumgarte
Journal:  Phys Rev Lett       Date:  2004-04-08       Impact factor: 9.161

6.  Universality and scaling in gravitational collapse of a massless scalar field.

Authors: 
Journal:  Phys Rev Lett       Date:  1993-01-04       Impact factor: 9.161

7.  Gravitational-wave emission from rotating gravitational collapse.

Authors: 
Journal:  Phys Rev Lett       Date:  1985-08-19       Impact factor: 9.161

8.  Challenging the paradigm of singularity excision in gravitational collapse.

Authors:  Luca Baiotti; Luciano Rezzolla
Journal:  Phys Rev Lett       Date:  2006-10-06       Impact factor: 9.161

9.  Formation of supermassive black holes through fragmentation of torodial supermassive stars.

Authors:  Burkhard Zink; Nikolaos Stergioulas; Ian Hawke; Christian D Ott; Erik Schnetter; Ewald Müller
Journal:  Phys Rev Lett       Date:  2006-04-26       Impact factor: 9.161

10.  Gravitational radiation from realistic relativistic stars: Odd-parity fluid perturbations.

Authors: 
Journal:  Phys Rev D Part Fields       Date:  1987-04-15
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  9 in total

Review 1.  Binary Neutron Star Mergers.

Authors:  Joshua A Faber; Frederic A Rasio
Journal:  Living Rev Relativ       Date:  2012-07-04       Impact factor: 40.429

Review 2.  Characteristic Evolution and Matching.

Authors:  Jeffrey Winicour
Journal:  Living Rev Relativ       Date:  2012-01-25       Impact factor: 40.429

Review 3.  Testing General Relativity with Low-Frequency, Space-Based Gravitational-Wave Detectors.

Authors:  Jonathan R Gair; Michele Vallisneri; Shane L Larson; John G Baker
Journal:  Living Rev Relativ       Date:  2013-09-12       Impact factor: 40.429

Review 4.  Dynamical Boson Stars.

Authors:  Steven L Liebling; Carlos Palenzuela
Journal:  Living Rev Relativ       Date:  2012-05-08       Impact factor: 40.429

Review 5.  Coalescence of Black Hole-Neutron Star Binaries.

Authors:  Masaru Shibata; Keisuke Taniguchi
Journal:  Living Rev Relativ       Date:  2011-08-29       Impact factor: 40.429

Review 6.  Rotating stars in relativity.

Authors:  Vasileios Paschalidis; Nikolaos Stergioulas
Journal:  Living Rev Relativ       Date:  2017-11-29       Impact factor: 40.429

Review 7.  Grid-based Methods in Relativistic Hydrodynamics and Magnetohydrodynamics.

Authors:  José María Martí; Ewald Müller
Journal:  Living Rev Comput Astrophys       Date:  2015-12-22

8.  Mapping nonlinear gravity into General Relativity with nonlinear electrodynamics.

Authors:  Victor I Afonso; Gonzalo J Olmo; Emanuele Orazi; Diego Rubiera-Garcia
Journal:  Eur Phys J C Part Fields       Date:  2018-10-27       Impact factor: 4.590

Review 9.  Dynamical boson stars.

Authors:  Steven L Liebling; Carlos Palenzuela
Journal:  Living Rev Relativ       Date:  2017-11-13       Impact factor: 40.429

  9 in total

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