Reference Citation Analysis: Find an Article, Find a Category, Find a Journal, Find a Scholar

For: Buras R, Rampp M, Janka HT, Kifonidis K. Improved models of stellar core collapse and still no explosions: what is missing? Phys Rev Lett 2003;90:241101. [PMID: 12857181 DOI: 10.1103/physrevlett.90.241101] [Citation(s) in RCA: 5] [Impact Index Per Article: 0.2] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Subscribe] [Scholar Register] [Received: 03/07/2003] [Indexed: 05/24/2023]

For:	Buras R, Rampp M, Janka HT, Kifonidis K. Improved models of stellar core collapse and still no explosions: what is missing? Phys Rev Lett 2003;90:241101. [PMID: 12857181 DOI: 10.1103/physrevlett.90.241101] [Citation(s) in RCA: 5] [Impact Index Per Article: 0.2] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Subscribe] [Scholar Register] [Received: 03/07/2003] [Indexed: 05/24/2023]

Number

Cited by Other Article(s)

YAMADA S, NAGAKURA H, AKAHO R, HARADA A, FURUSAWA S, IWAKAMI W, OKAWA H, MATSUFURU H, SUMIYOSHI K. Physical mechanism of core-collapse supernovae that neutrinos drive. PROCEEDINGS OF THE JAPAN ACADEMY. SERIES B, PHYSICAL AND BIOLOGICAL SCIENCES 2024;100:190-233. [PMID: 38462501 PMCID: PMC11105976 DOI: 10.2183/pjab.100.015] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Received: 02/05/2023] [Accepted: 12/05/2023] [Indexed: 03/12/2024]

Nabi JU, Fayaz M. Gamma ray heating rates due to chromium isotopes in stellar core during late stages of high mass stars (>10M_⊙). EPJ WEB OF CONFERENCES 2017. [DOI: 10.1051/epjconf/201715401005] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/14/2022] Open

Font JA. Numerical Hydrodynamics and Magnetohydrodynamics in General Relativity. LIVING REVIEWS IN RELATIVITY 2008;11:7. [PMID: 28179823 PMCID: PMC5256108 DOI: 10.12942/lrr-2008-7] [Citation(s) in RCA: 16] [Impact Index Per Article: 1.0] [Reference Citation Analysis] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Accepted: 07/21/2008] [Indexed: 05/27/2023]

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.

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Schawinski K, Justham S, Wolf C, Podsiadlowski P, Sullivan M, Steenbrugge KC, Bell T, Röser HJ, Walker ES, Astier P, Balam D, Balland C, Carlberg R, Conley A, Fouchez D, Guy J, Hardin D, Hook I, Howell DA, Pain R, Perrett K, Pritchet C, Regnault N, Yi SK. Supernova Shock Breakout from a Red Supergiant. Science 2008;321:223-6. [DOI: 10.1126/science.1160456] [Citation(s) in RCA: 102] [Impact Index Per Article: 6.4] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/02/2022]

Affiliation(s)

Kevin Schawinski Department of Physics, University of Oxford, Oxford OX1 3RH, UK St John's College Research Centre, University of Oxford, Oxford OX1 3JP, UK Max-Planck-Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, Germany Laboratoire de Physique Nucléaire et de Hautes Energies, CNRS-IN2P3 and Universités Paris VI and VII, 4 Place Jussieu, 75252 Paris Cedex 05, France Department of Physics and Astronomy, University of Victoria, Post Office Box 3055 STN CSC, Victoria, BC V8T 3P6, Canada
Stephen Justham Department of Physics, University of Oxford, Oxford OX1 3RH, UK St John's College Research Centre, University of Oxford, Oxford OX1 3JP, UK Max-Planck-Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, Germany Laboratoire de Physique Nucléaire et de Hautes Energies, CNRS-IN2P3 and Universités Paris VI and VII, 4 Place Jussieu, 75252 Paris Cedex 05, France Department of Physics and Astronomy, University of Victoria, Post Office Box 3055 STN CSC, Victoria, BC V8T 3P6, Canada
Christian Wolf Department of Physics, University of Oxford, Oxford OX1 3RH, UK St John's College Research Centre, University of Oxford, Oxford OX1 3JP, UK Max-Planck-Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, Germany Laboratoire de Physique Nucléaire et de Hautes Energies, CNRS-IN2P3 and Universités Paris VI and VII, 4 Place Jussieu, 75252 Paris Cedex 05, France Department of Physics and Astronomy, University of Victoria, Post Office Box 3055 STN CSC, Victoria, BC V8T 3P6, Canada
Philipp Podsiadlowski Department of Physics, University of Oxford, Oxford OX1 3RH, UK St John's College Research Centre, University of Oxford, Oxford OX1 3JP, UK Max-Planck-Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, Germany Laboratoire de Physique Nucléaire et de Hautes Energies, CNRS-IN2P3 and Universités Paris VI and VII, 4 Place Jussieu, 75252 Paris Cedex 05, France Department of Physics and Astronomy, University of Victoria, Post Office Box 3055 STN CSC, Victoria, BC V8T 3P6, Canada
Mark Sullivan Department of Physics, University of Oxford, Oxford OX1 3RH, UK St John's College Research Centre, University of Oxford, Oxford OX1 3JP, UK Max-Planck-Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, Germany Laboratoire de Physique Nucléaire et de Hautes Energies, CNRS-IN2P3 and Universités Paris VI and VII, 4 Place Jussieu, 75252 Paris Cedex 05, France Department of Physics and Astronomy, University of Victoria, Post Office Box 3055 STN CSC, Victoria, BC V8T 3P6, Canada
Katrien C. Steenbrugge Department of Physics, University of Oxford, Oxford OX1 3RH, UK St John's College Research Centre, University of Oxford, Oxford OX1 3JP, UK Max-Planck-Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, Germany Laboratoire de Physique Nucléaire et de Hautes Energies, CNRS-IN2P3 and Universités Paris VI and VII, 4 Place Jussieu, 75252 Paris Cedex 05, France Department of Physics and Astronomy, University of Victoria, Post Office Box 3055 STN CSC, Victoria, BC V8T 3P6, Canada
Tony Bell Department of Physics, University of Oxford, Oxford OX1 3RH, UK St John's College Research Centre, University of Oxford, Oxford OX1 3JP, UK Max-Planck-Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, Germany Laboratoire de Physique Nucléaire et de Hautes Energies, CNRS-IN2P3 and Universités Paris VI and VII, 4 Place Jussieu, 75252 Paris Cedex 05, France Department of Physics and Astronomy, University of Victoria, Post Office Box 3055 STN CSC, Victoria, BC V8T 3P6, Canada
Hermann-Josef Röser Department of Physics, University of Oxford, Oxford OX1 3RH, UK St John's College Research Centre, University of Oxford, Oxford OX1 3JP, UK Max-Planck-Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, Germany Laboratoire de Physique Nucléaire et de Hautes Energies, CNRS-IN2P3 and Universités Paris VI and VII, 4 Place Jussieu, 75252 Paris Cedex 05, France Department of Physics and Astronomy, University of Victoria, Post Office Box 3055 STN CSC, Victoria, BC V8T 3P6, Canada
Emma S. Walker Department of Physics, University of Oxford, Oxford OX1 3RH, UK St John's College Research Centre, University of Oxford, Oxford OX1 3JP, UK Max-Planck-Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, Germany Laboratoire de Physique Nucléaire et de Hautes Energies, CNRS-IN2P3 and Universités Paris VI and VII, 4 Place Jussieu, 75252 Paris Cedex 05, France Department of Physics and Astronomy, University of Victoria, Post Office Box 3055 STN CSC, Victoria, BC V8T 3P6, Canada
Pierre Astier Department of Physics, University of Oxford, Oxford OX1 3RH, UK St John's College Research Centre, University of Oxford, Oxford OX1 3JP, UK Max-Planck-Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, Germany Laboratoire de Physique Nucléaire et de Hautes Energies, CNRS-IN2P3 and Universités Paris VI and VII, 4 Place Jussieu, 75252 Paris Cedex 05, France Department of Physics and Astronomy, University of Victoria, Post Office Box 3055 STN CSC, Victoria, BC V8T 3P6, Canada
Dave Balam Department of Physics, University of Oxford, Oxford OX1 3RH, UK St John's College Research Centre, University of Oxford, Oxford OX1 3JP, UK Max-Planck-Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, Germany Laboratoire de Physique Nucléaire et de Hautes Energies, CNRS-IN2P3 and Universités Paris VI and VII, 4 Place Jussieu, 75252 Paris Cedex 05, France Department of Physics and Astronomy, University of Victoria, Post Office Box 3055 STN CSC, Victoria, BC V8T 3P6, Canada
Christophe Balland Department of Physics, University of Oxford, Oxford OX1 3RH, UK St John's College Research Centre, University of Oxford, Oxford OX1 3JP, UK Max-Planck-Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, Germany Laboratoire de Physique Nucléaire et de Hautes Energies, CNRS-IN2P3 and Universités Paris VI and VII, 4 Place Jussieu, 75252 Paris Cedex 05, France Department of Physics and Astronomy, University of Victoria, Post Office Box 3055 STN CSC, Victoria, BC V8T 3P6, Canada
Ray Carlberg Department of Physics, University of Oxford, Oxford OX1 3RH, UK St John's College Research Centre, University of Oxford, Oxford OX1 3JP, UK Max-Planck-Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, Germany Laboratoire de Physique Nucléaire et de Hautes Energies, CNRS-IN2P3 and Universités Paris VI and VII, 4 Place Jussieu, 75252 Paris Cedex 05, France Department of Physics and Astronomy, University of Victoria, Post Office Box 3055 STN CSC, Victoria, BC V8T 3P6, Canada
Alex Conley Department of Physics, University of Oxford, Oxford OX1 3RH, UK St John's College Research Centre, University of Oxford, Oxford OX1 3JP, UK Max-Planck-Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, Germany Laboratoire de Physique Nucléaire et de Hautes Energies, CNRS-IN2P3 and Universités Paris VI and VII, 4 Place Jussieu, 75252 Paris Cedex 05, France Department of Physics and Astronomy, University of Victoria, Post Office Box 3055 STN CSC, Victoria, BC V8T 3P6, Canada
Dominique Fouchez Department of Physics, University of Oxford, Oxford OX1 3RH, UK St John's College Research Centre, University of Oxford, Oxford OX1 3JP, UK Max-Planck-Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, Germany Laboratoire de Physique Nucléaire et de Hautes Energies, CNRS-IN2P3 and Universités Paris VI and VII, 4 Place Jussieu, 75252 Paris Cedex 05, France Department of Physics and Astronomy, University of Victoria, Post Office Box 3055 STN CSC, Victoria, BC V8T 3P6, Canada
Julien Guy Department of Physics, University of Oxford, Oxford OX1 3RH, UK St John's College Research Centre, University of Oxford, Oxford OX1 3JP, UK Max-Planck-Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, Germany Laboratoire de Physique Nucléaire et de Hautes Energies, CNRS-IN2P3 and Universités Paris VI and VII, 4 Place Jussieu, 75252 Paris Cedex 05, France Department of Physics and Astronomy, University of Victoria, Post Office Box 3055 STN CSC, Victoria, BC V8T 3P6, Canada
Delphine Hardin Department of Physics, University of Oxford, Oxford OX1 3RH, UK St John's College Research Centre, University of Oxford, Oxford OX1 3JP, UK Max-Planck-Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, Germany Laboratoire de Physique Nucléaire et de Hautes Energies, CNRS-IN2P3 and Universités Paris VI and VII, 4 Place Jussieu, 75252 Paris Cedex 05, France Department of Physics and Astronomy, University of Victoria, Post Office Box 3055 STN CSC, Victoria, BC V8T 3P6, Canada
Isobel Hook Department of Physics, University of Oxford, Oxford OX1 3RH, UK St John's College Research Centre, University of Oxford, Oxford OX1 3JP, UK Max-Planck-Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, Germany Laboratoire de Physique Nucléaire et de Hautes Energies, CNRS-IN2P3 and Universités Paris VI and VII, 4 Place Jussieu, 75252 Paris Cedex 05, France Department of Physics and Astronomy, University of Victoria, Post Office Box 3055 STN CSC, Victoria, BC V8T 3P6, Canada
D. Andrew Howell Department of Physics, University of Oxford, Oxford OX1 3RH, UK St John's College Research Centre, University of Oxford, Oxford OX1 3JP, UK Max-Planck-Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, Germany Laboratoire de Physique Nucléaire et de Hautes Energies, CNRS-IN2P3 and Universités Paris VI and VII, 4 Place Jussieu, 75252 Paris Cedex 05, France Department of Physics and Astronomy, University of Victoria, Post Office Box 3055 STN CSC, Victoria, BC V8T 3P6, Canada
Reynald Pain Department of Physics, University of Oxford, Oxford OX1 3RH, UK St John's College Research Centre, University of Oxford, Oxford OX1 3JP, UK Max-Planck-Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, Germany Laboratoire de Physique Nucléaire et de Hautes Energies, CNRS-IN2P3 and Universités Paris VI and VII, 4 Place Jussieu, 75252 Paris Cedex 05, France Department of Physics and Astronomy, University of Victoria, Post Office Box 3055 STN CSC, Victoria, BC V8T 3P6, Canada
Kathy Perrett Department of Physics, University of Oxford, Oxford OX1 3RH, UK St John's College Research Centre, University of Oxford, Oxford OX1 3JP, UK Max-Planck-Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, Germany Laboratoire de Physique Nucléaire et de Hautes Energies, CNRS-IN2P3 and Universités Paris VI and VII, 4 Place Jussieu, 75252 Paris Cedex 05, France Department of Physics and Astronomy, University of Victoria, Post Office Box 3055 STN CSC, Victoria, BC V8T 3P6, Canada
Chris Pritchet Department of Physics, University of Oxford, Oxford OX1 3RH, UK St John's College Research Centre, University of Oxford, Oxford OX1 3JP, UK Max-Planck-Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, Germany Laboratoire de Physique Nucléaire et de Hautes Energies, CNRS-IN2P3 and Universités Paris VI and VII, 4 Place Jussieu, 75252 Paris Cedex 05, France Department of Physics and Astronomy, University of Victoria, Post Office Box 3055 STN CSC, Victoria, BC V8T 3P6, Canada
Nicolas Regnault Department of Physics, University of Oxford, Oxford OX1 3RH, UK St John's College Research Centre, University of Oxford, Oxford OX1 3JP, UK Max-Planck-Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, Germany Laboratoire de Physique Nucléaire et de Hautes Energies, CNRS-IN2P3 and Universités Paris VI and VII, 4 Place Jussieu, 75252 Paris Cedex 05, France Department of Physics and Astronomy, University of Victoria, Post Office Box 3055 STN CSC, Victoria, BC V8T 3P6, Canada
Sukyoung K. Yi Department of Physics, University of Oxford, Oxford OX1 3RH, UK St John's College Research Centre, University of Oxford, Oxford OX1 3JP, UK Max-Planck-Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, Germany Laboratoire de Physique Nucléaire et de Hautes Energies, CNRS-IN2P3 and Universités Paris VI and VII, 4 Place Jussieu, 75252 Paris Cedex 05, France Department of Physics and Astronomy, University of Victoria, Post Office Box 3055 STN CSC, Victoria, BC V8T 3P6, Canada

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Dasgupta B, Dighe A. Phase effects in neutrino conversions during a supernova shock wave. Int J Clin Exp Med 2007. [DOI: 10.1103/physrevd.75.093002] [Citation(s) in RCA: 44] [Impact Index Per Article: 2.6] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/07/2022]

Todd-Rutel BG, Piekarewicz J. Neutron-rich nuclei and neutron stars: a new accurately calibrated interaction for the study of neutron-rich matter. PHYSICAL REVIEW LETTERS 2005;95:122501. [PMID: 16197069 DOI: 10.1103/physrevlett.95.122501] [Citation(s) in RCA: 31] [Impact Index Per Article: 1.6] [Reference Citation Analysis] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 04/11/2005] [Indexed: 05/04/2023]

Nuclear Astrophysicsand Nuclei Far from Stability. ACTA ACUST UNITED AC 2004. [DOI: 10.1007/978-3-540-44490-9_11] [Citation(s) in RCA: 2] [Impact Index Per Article: 0.1] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register]

Jachowicz N, Vantournhout K, Ryckebusch J, Heyde K. Identifying neutrinos and antineutrinos in neutral-current scattering reactions. PHYSICAL REVIEW LETTERS 2004;93:082501. [PMID: 15447177 DOI: 10.1103/physrevlett.93.082501] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.1] [Reference Citation Analysis] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 02/26/2004] [Indexed: 05/24/2023]

Scheck L, Plewa T, Janka HT, Kifonidis K, Müller E. Pulsar recoil by large-scale anisotropies in supernova explosions. PHYSICAL REVIEW LETTERS 2004;92:011103. [PMID: 14753979 DOI: 10.1103/physrevlett.92.011103] [Citation(s) in RCA: 4] [Impact Index Per Article: 0.2] [Reference Citation Analysis] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 07/18/2003] [Indexed: 05/24/2023]

Hix WR, Messer OEB, Mezzacappa A, Liebendörfer M, Sampaio J, Langanke K, Dean DJ, Martínez-Pinedo G. Consequences of nuclear electron capture in core collapse supernovae. PHYSICAL REVIEW LETTERS 2003;91:201102. [PMID: 14683349 DOI: 10.1103/physrevlett.91.201102] [Citation(s) in RCA: 7] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 04/25/2003] [Indexed: 05/24/2023]

Fryer CL, New KCB. Gravitational Waves from Gravitational Collapse. LIVING REVIEWS IN RELATIVITY 2003;6:2. [PMID: 28163639 PMCID: PMC5253977 DOI: 10.12942/lrr-2003-2] [Citation(s) in RCA: 5] [Impact Index Per Article: 0.2] [Reference Citation Analysis] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Accepted: 01/13/2003] [Indexed: 05/27/2023]