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We review the current status of studies of the coalescence of binary neutron star systems.
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1977
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1977
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Lucy, L.B., “A numerical approach to the testing of the fission hypothesis”, Astron. J
1977
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1980
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1984
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Glendenning, N.K., “Neutron Stars Are Giant Hypernuclei?”, Astrophys. J
1985
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Hachisu, I., “A versatile method for obtaining structures of rapidly rotating stars”, Astrophys. J. Suppl. Ser
1986
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1986
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Chandrasekhar, S., Ellipsoidal figures of equilibrium
1987
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Komatsu, H., Eriguchi, Y. and Hachisu, I., “Rapidly rotating general relativistic stars – I. Numerical method and its application to uniformly rotating polytropes”, Mon. Not. R. Astron. Soc
1989
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Nakamura, T. and Oohara, K., “Gravitational Radiation From Coalescing Binary Neutron Stars. 2. Simulations Including Back Reaction Potential”, Prog. Theor. Phys
1989
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Oohara, K. and Nakamura, T., “Gravitational Radiation From A Coalescing Binary Neutron Star”, Prog. Theor. Phys
1989
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Pandharipande, V.R. and Ravenhall, D.G., “Hot Nuclear Matter”, in Soyeur, M., Flocard, H., Tamain, B. and Porneuf, M., eds., Nuclear Matter and Heavy Ion Collisions
1989
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Taylor, J.H. and Weisberg, J.M., “Further experimental tests of relativistic gravity using the binary pulsar PSR 1913+16”, Astrophys. J
1989
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Wilson, J.R. and Mathews, G.J., “Relativistic hydrodynamics”, in Evans, C.R., Finn, L.S. and Hobill, D.W., eds., Frontiers in Numerical Relativity
1989
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Winicour, J., “Disembodied boundary data for Einstein’s equations”, Phys. Rev. D
1989
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Blanchet, L., Damour, T. and Schäfer, G., “Post-Newtonian hydrodynamics and post-Newtonian gravitational wave generation for numerical relativity”, Mon. Not. R. Astron. Soc
1990
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Oohara, K. and Nakamura, T., “Gravitational Radiation From Coalescing Binary Neutron Stars. 3. Simulations From Equilibrium Model”, Prog. Theor. Phys
1990
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Bhattacharya, D. and van den Heuvel, E.P.J., “Formation and evolution of binary and millisecond radio pulsars”, Phys. Rept
1991
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Lattimer, J.M. and Swesty, F.D., “A Generalized equation of state for hot, dense matter”, Nucl. Phys. A
1991
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Mart, J. M., Ibáez, J. M. and Miralles, J. A., “Numerical relativistic hydrodynamics: Local characteristic approach”, Phys. Rev. D
1991
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Nakamura, T. and Oohara, K., “Gravitational radiation from coalescing binary neutron stars. 4: Tidal disruption”, Prog. Theor. Phys
1991
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Bildsten, L. and Cutler, C., “Tidal interactions of inspiraling compact binaries”, Astrophys. J
1992
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Cook, G.B., Shapiro, S.L. and Teukolsky, S.A., “Spin-up of a rapidly rotating star by angular momentum loss - Effects of general relativity”, Astrophys. J.j
1992
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Kochanek, C.S., “Coalescing binary neutron stars”, Astrophys. J
1992
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Monaghan, J.J., “Smoothed particle hydrodynamics”, Annu. Rev. Astron. Astrophys
1992
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Rasio, F.A. and Shapiro, S.L., “Hydrodynamical evolution of coalescing binary neutron stars”, Astrophys. J
1992
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Shibata, M., Nakamura, T. and Oohara, K., “Coalescence of spinning binary neutron stars of equal mass 3-D numerical simulations”, Prog. Theor. Phys
1992
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Lai, D., Rasio, F.A. and Shapiro, S.L., “Ellipsoidal figures of equilibrium - Compressible models”, Astrophys. J. Suppl. Ser
1993
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Lai, D., Rasio, F.A. and Shapiro, S.L., “Hydrodynamic instability and coalescence of close binary systems”, Astrophys. J. Lett
1993
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Oohara, K. and Nakamura, T., “Gravitational radiation from coalescing binary neutron stars. 5. PostNewtonian calculation”, Prog. Theor. Phys
1993
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Cook, G.B., Shapiro, S.L. and Teukolsky, S.A., “Rapidly rotating neutron stars in general relativity: Realistic equations of state”, Astrophys. J
1994
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Davies, M.B., Benz, W., Piran, T. and Thielemann, F.K., “Merging neutron stars. I. Initial results for coalescence of noncorotating systems”, Astrophys. J
1994
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Lai, D., Rasio, F.A. and Shapiro, S.L., “Equilibrium, stability and orbital evolution of close binary systems”, Astrophys. J
1994
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Lai, D., Rasio, F.A. and Shapiro, S.L., “Hydrodynamic instability and coalescence of binary neutron stars”, Astrophys. J
1994
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Lai, D., Rasio, F.A. and Shapiro, S.L., “Hydrodynamics of rotating stars and close binary interactions: Compressible ellipsoid models”, Astrophys. J
1994
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Rasio, F.A. and Shapiro, S.L., “Hydrodynamics of binary coalescence. 1. Polytropes with stiff equations of state”, Astrophys. J
1994
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Xing, Z.-G., Centrella, J.M. and McMillan, S.L.W., “Gravitational radiation from coalescing binary neutron stars”, Phys. Rev. D
1994
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Kettner, C., Weber, F., Weigel, M.K. and Glendenning, N.K., “Structure and stability of strange and charm stars at finite temperatures”, Phys. Rev. D
1995
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Lai, D. and Shapiro, S.L., “Gravitational radiation from rapidly rotating nascent neutron stars”, Astrophys. J
1995
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Prakash, M., Cooke, J.R. and Lattimer, J.M., “Quark - hadron phase transition in protoneutron stars”, Phys. Rev. D
1995
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Rasio, F.A. and Shapiro, S.L., “Hydrodynamics of binary coalescence. II. Polytropes with Γ = 5 / 3 \Gamma=5/3 ”, Astrophys. J
1995
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Shibata, M. and Nakamura, T., “Evolution of three-dimensional gravitational waves: Harmonic slicing case”, Phys. Rev. D
1995
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Wilson, J.R. and Mathews, G.J., “Instabilities in Close Neutron Star Binaries”, Phys. Rev. Lett
1995
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Janka, H.-T. and Ruffert, M., “Can neutrinos from neutron star mergers power gamma-ray bursts?”, Astron. Astrophys
1996
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Ruffert, M.H., Janka, H.-T. and Schäfer, G., “Coalescing neutron stars: A Step towards physical models. 1: Hydrodynamic evolution and gravitational wave emission”, Astron. Astrophys
1996
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Shibata, M., “Instability of synchronized binary neutron stars in the first post-Newtonian approximation of general relativity”, Prog. Theor. Phys
1996
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Wilson, J.R., Mathews, G.J. and Marronetti, P., “Relativistic numerical model for close neutron star binaries”, Phys. Rev. D
1996
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Xing, Z.-G., Centrella, J.M. and McMillan, S.L.W., “Gravitational radiation from the coalescence of binary neutron stars: Effects due to the equation of state, spin, and mass ratio”, Phys. Rev. D
1996
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Balberg, S. and Gal, A., “An Effective equation of state for dense matter with strangeness”, Nucl. Phys. A
1997
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Baumgarte, T.W., Cook, G.B., Scheel, M.A., Shapiro, S.L. and Teukolsky, S.A., “Binary neutron stars in general relativity: Quasiequilibrium models”, Phys. Rev. Lett
1997
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Lombardi Jr, J.C., Rasio, F.A. and Shapiro, S.L., “PostNewtonian models of binary neutron stars”, Phys. Rev. D
1997
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Mathews, G.J. and Wilson, J.R., “Binary induced neutron star compression, heating, and collapse”, Astrophys. J
1997
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New, K.C.B. and Tohline, J.E., “The Relative stability against merger of close, compact binaries”, Astrophys. J
1997
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Ruffert, M., Janka, H.-T., Takahashi, K. and Schäfer, G., “Coalescing neutron stars: A Step towards physical models. 2. Neutrino emission, neutron tori, and gamma-ray bursts”, Astron. Astrophys
1997
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Ruffert, M., Rampp, M. and Janka, H.-T., “Coalescing neutron stars: Gravitational waves from polytropic models”, Astron. Astrophys
1997
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Shibata, M., “Numerical study of synchronized binary neutron stars in the postNewtonian approximation of general relativity”, Phys. Rev. D
1997
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Shibata, M., Oohara, K. and Nakamura, T., “Numerical study on the hydrodynamic instability of binary stars in the first post-Newtonian approximation of general relativity”, Prog. Theor. Phys
1997
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Shibata, M. and Taniguchi, K., “Solving the Darwin problem in the first postNewtonian approximation of general relativity: Compressible model”, Phys. Rev. D
1997
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Akmal, A., Pandharipande, V.R. and Ravenhall, D.G., “The Equation of state of nucleon matter and neutron star structure”, Phys. Rev. C
1998
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Baumgarte, T.W., Cook, G.B., Scheel, M.A., Shapiro, S.L. and Teukolsky, S.A., “General relativistic models of binary neutron stars in quasiequilibrium”, Phys. Rev. D
1998
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Mathews, G.J., Marronetti, P. and Wilson, J.R., “Relativistic hydrodynamics in close binary systems: Analysis of neutron star collapse”, Phys. Rev. D
1998
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Portegies Zwart, S.F., “Gamma-ray binaries: Stable mass transfer from neutron star to black hole”, Astrophys. J. Lett
1998
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Shen, H., Toki, H., Oyamatsu, K. and Sumiyoshi, K., “Relativistic equation of state of nuclear matter for supernova and neutron star”, Nucl. Phys. A
1998
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1998
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Shibata, M., Baumgarte, T.W. and Shapiro, S.L., “Stability of coalescing binary stars against gravitational collapse: Hydrodynamical simulations”, Phys. Rev. D
1998
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Taniguchi, K., Asada, H. and Shibata, M., “Irrotational and incompressible ellipsoids in the first postNewtonian approximation of general relativity”, Prog. Theor. Phys
1998
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Uryū, K. and Eriguchi, Y., “Stationary states of irrotational binary neutron star systems and their evolution due to gravitational wave emission”, Mon. Not. R. Astron. Soc. Lett
1998
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Uryū, K. and Eriguchi, Y., “Stationary structures of irrotational binary systems: Models for close binary systems of compact stars”, Astrophys. J. Suppl. Ser
1998
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Baumgarte, T.W. and Shapiro, S.L., “On the numerical integration of Einstein’s field equations”, Phys. Rev. D
1999
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Bonazzola, S., Gourgoulhon, E. and Marck, J.-A., “Numerical models of irrotational binary neutron stars in general relativity”, Phys. Rev. Lett
1999
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Buonanno, A. and Damour, T., “Effective one-body approach to general relativistic two-body dynamics”, Phys. Rev. D
1999
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1999
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Flanagan, É.É., “Possible explanation for star-crushing effect in binary neutron star simulations”, Phys. Rev. Lett
1999
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Freiburghaus, C., Rosswog, S. and Thielemann, F.-K., “R-Process in Neutron Star Mergers”, Astrophys. J. Lett
1999
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Friedrich, H. and Nagy, G., “The Initial boundary value problem for Einstein’s vacuum field equations”, Commun.Math.Phys
1999
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1999
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Janka, H.-T., Eberl, T., Ruffert, M. and Fryer, C.L., “Black hole: Neutron star mergers as central engines of gamma-ray bursts”, Astrophys. J. Lett
1999
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Lee, W.H. and Kluźniak, W., “Newtonian hydrodynamics of the coalescence of black holes with neutron stars. 1. Tidally locked binaries with a stiff equation of state”, Astrophys. J
1999
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Lee, W.H. and Kluźniak, W., “Newtonian hydrodynamics of the coalescence of black holes with neutron stars. II. Tidally locked binaries with a soft equation of state”, Mon. Not. R. Astron. Soc
1999
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Marronetti, P., Mathews, G.J. and Wilson, J.R., “Irrotational binary neutron stars in quasiequilibrium”, Phys. Rev. D
1999
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Ruffert, M. and Janka, H.-T., “Gamma-ray bursts from accreting black holes in neutron star mergers”, Astron. Astrophys
1999
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Shibata, M., “3-D numerical simulation of black hole formation using collisionless particles: Triplane symmetric case”, Prog. Theor. Phys
1999
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Shibata, M., “Fully general relativistic simulation of merging binary clusters: Spatial gauge condition”, Prog. Theor. Phys
1999
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1999
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Baumgarte, T.W., Shapiro, S.L. and Shibata, M., “On the maximum mass of differentially rotating neutron stars”, Astrophys. J. Lett
2000
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2000
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2000
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Mathews, G.J. and Wilson, J.R., “Revised relativistic hydrodynamical model for neutron star binaries”, Phys. Rev. D
2000
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2000
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2000
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2000
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Uryū, K., Shibata, M. and Eriguchi, Y., “Properties of general relativistic, irrotational binary neutron stars in close quasiequilibrium orbits: Polytropic equations of state”, Phys. Rev. D
2000
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Usui, F., Uryū, K. and Eriguchi, Y., “A New numerical scheme to compute 3-D configurations of quasiequilibrium compact stars in general relativity: Application to synchronously rotating binary star systems”, Phys. Rev. D
2000
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Ayal, S., Piran, T., Oechslin, R., Davies, M.B. and Rosswog, S., “PostNewtonian SPH”, Astrophys. J
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2001
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Faber, J.A., Rasio, F.A. and Manor, J.B., “PostNewtonian SPH calculations of binary neutron star coalescence. 2. Binary mass ratio, equation of state, and spin dependence”, Phys. Rev. D
2001
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Gourgoulhon, E., Grandclément, P., Taniguchi, K., Marck, J.-A. and Bonazzola, S., “Quasiequilibrium sequences of synchronized and irrotational binary neutron stars in general relativity: 1. Method and tests”, Phys. Rev. D
2001
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Rosswog, S., Freiburghaus, C. and Thielemann, F.K., “Nucleosynthesis calculations for the ejecta of neutron star coalescences”, Nucl. Phys. A
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Ruffert, M. and Janka, H.-T., “Coalescing neutron stars - a step towards physical models III. Improved numerics and different neutron star masses and spins s”, Astron. Astrophys
2001
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Saijo, M., Shibata, M., Baumgarte, T.W. and Shapiro, S.L., “Dynamical bar instability in rotating stars: Effect of general relativity”, Astrophys. J
2001
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Baker, J., Campanelli, M. and Lousto, C. O., “The Lazarus project: A Pragmatic approach to binary black hole evolutions”, Phys. Rev. D
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Taniguchi, K. and Shibata, M., “Binary Neutron Stars in Quasi-equilibrium”, Astrophys. J. Suppl. Ser
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Closest in time.
“Einstein Toolkit”. URL (accessed 30 March 2012): http://www.einsteintoolkit.org
2012
Closest in time.
2012
Closest in time.
2012
Closest in time.
2012
Closest in time.
“HAD: the hyper AMR driver”. URL (accessed 20 March 2012): http://relativity.phys.lsu.edu/~matt/had.html
2012
Closest in time.
“LORENE: Langage Objet pour la RElativité NumériquE”. URL (accessed 30 March 2012): http://www.lorene.obspm.fr
2012
Closest in time.
“The Cactus Code”. URL (accessed 30 March 2012): http://www.cactuscode.org/
2012
Closest in time.