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Literature Catalog: Stellar CollapseAlso sorted by dateLast updated January 14, 2005. Arnaud, N. and Barsuglia, M. and Bizouard, M. and Brisson, V. and Cavalier, F. and Davier, M. and Hello, P. and Kreckelbergh, S. and Porter, E.K., Detection of a close supernova gravitational wave burst in a network of interferometers, neutrino and optical detectors, Astroparticle Physics 21, 201 (2004) Bonazzola, S. and Frieben, J. and Gourgoulhon, E. " Spontaneous symmetry breaking of rapidly rotating stars in general relativity: influence of the 3Dshift vector," Astron. Astrophys., 331, 280 (1997). Bonazzola, S. and Frieben, J. and Gourgoulhon, E. " Spontaneous Symmetry Breaking of Rapidly Rotating Stars in General Relativity," ApJ, 460, 379 (1996). Bonazzola, S. and Marck, J. A. " Efficiency of gravitational radiation from axisymmetric and 3D stellar collapse. I  Polytropic case," Astron. Astrophys., 267, 623 (1993). Brown, J. D. " Rotational instabilities in postcollapse stellar cores," AIP Conference Proc., Vol. 575, Astrophysical sources for groundbased gravitational wave detectors, pg. 234 (2001) Ed. Centrella, J. M. New York, USA. American Institute of Physics, Melville. Burman, R.R. and Blair, D.G. and Woodings, S.J. " Calculating the cosmic background of supernovagenerated gravitational radiation," in 'Recent developments in theoretical and experimental general relativity, gravitation, and relativistic field theories', eds. T. Piran and R. Ruffini, World Scientific Publishers, 1092 (1999) Burrows, A. and Hayes, J. " Pulsar recoil and gravitational radiation due to axisymmetrical stellar collapse and explosion," Phys. Rev. Lett., 76, 352 (1996). CerdaDuran, P. and Faye, G. and Dimmelmeier, H. and Font, J.A. and Ibanez, J.M. and Mueller, E. and Schaefer, G., CFC+: Improved dynamics and gravitational waveforms from relativistic core collapse simulations Astron. Astrophys., submitted; and astroph Dimmelmeier, H. and Novak, J. and Font, J.A. and Ibanez, J.M. and Mueller, E., Mariage des Maillages: A new numerical approach for 3D relativistic core collapse simulations Phys. Rev. D, submitted; and astroph Dimmelmeier, H. and Font, J. A. and Müller, E. " Relativistic simulations of rotational core collapse. I. Methods, initial models, and code tests," Astron. Astrophys., 388, 917 (2002). Dimmelmeier, H. and Font, J. A. and Müller, E. " Relativistic simulations of rotational core collapse. II. Collapse dynamics and gravitational radiation," Astron. Astrophys., 393, 523 (2002). Dimmelmeier, H. and Font, J. A. and Müller, E. " Gravitational waves from relativistic rotational core collapse," ApJ 560, L163L166. (2001). Epstein, R. " The generation of gravitational radiation by escaping supernova neutrinos," ApJ., 223, 1037 (1978). Evans, C. R. "An approach for calculating axisymmetric gravitational collapse," in Dynamical spacetimes and numerical relativity, pg. 3, (1986). Ed. Centrella, J. M. Cambridge, U. K. Cambridge University Press. Ferrari, V. and Matarrese, S. and Schneider, R. " Gravitational wave background from a cosmological population of corecollapse supernovae", Mon.Not.Roy.Astron.Soc., 3037, 247257 (1999). Finn, L. S. and Evans, C. R. " Determining gravitational radiation from Newtonian selfgravitating systems," ApJ, 351, 588 (1990). Finn, L. S. "Supernovae, gravitational radiation, and the quadrupole formula," in Frontiers in numerical relativity, pg. 126 (1989). Eds. Evans, C. R. and Finn, S. L. and Hobill, D. W. Cambridge, U. K. Cambridge University Press. Fryer, C.L. and Holz, D.E. and Hughes, S.A., Gravitational Waves from Stellar Collapse: Correlations to Explosion Asymmetries, ApJ 609, 288 (2004) Fryer, C.L. and Warren, M.S. and Holz, D.E. and Hughes, S.A. and Dupuis, R., Gravitational waves from core collapse, in "GravitationalWave Detection", eds. M.Cruise and P.Saulson, proceedings of the SPIE, Vol.4856, 123 (2003) Fryer, C.L. and Holz, D.E. and Hughes, S.A. and Warren, M.S. " Stellar collapse and gravitational waves" astroph/0211609 Fryer, C. and Holz, D. E. and Hughes, S. A. " Gravitational wave emission from core collapse of massive stars," ApJ, 565, 430 (2002). Houser, J.L. " Instabilities in Stiff Stellar Cores: The Gravitational Radiation Reaction," in 'Gravitational Waves', Third Edoardo Amaldi Conference, ed. S. Meshkov, AIP Conference Proceedings, Vol.523, 51 (2000). Houser, J.L. " The effect of rotation on the gravitational radiation and dynamical stability of stiff stellar cores," Mon. Not. Roy. Astronom. Soc., 299, 1069 (1998). Houser, J. L. and Centrella, J. M. and Smith, S. C. " Gravitational radiation from nonaxisymmetric instability in a rotating star," Phys. Rev. Lett., 72, 1314 (1994). Howell, E. and Coward, D. and Burman, R. and Blair, D. and Gilmore, J., The gravitational wave background from neutron star birth throughout the cosmos, Mon. Not. Roy. Astron. Soc. 351, 1237 (2004) Imamura, J.N. and Pickett, B.K. and Durisen, R.H., " The Nonlinear Evolution of Massive Stellar Core Collapses That 'Fizzle' " ApJ 587, 341 (2003) Kobayashi, S., Meszaros, P. " Polarized gravitational waves from gammaray bursts," ApJ, 585, L89 (2003). Kotake, K. and Yamada, S. and Sato, K. and Sumiyoshi, K. and Ono, H. and Suzuki, H., Gravitational Radiation from Rotational Core Collapse: Effects of Magnetic Fields and Realistic Equation of States, Phys. Rev. D69, 124004 (2004) Kotake, K. and Yamada, S. and Sato, K., " Gravitational radiation from axisymmetric rotational core collapse", Phys.Rev.D, 68, 44023 (2003) Loveridge, L. C., Gravitational waves from a pulsar kick caused by neutrino conversions Phys. Rev. D69, 024008 (2004) Loveridge, L.C., Gravitational Waves from a Pulsar Kick Caused by Neutrino Conversions, Phys.Rev. D69, 024008 (2004) Mönchmeyer, R. and Schäfer, G. and Mueller, E. and Kates, R. E. " Gravitational waves from the collapse of rotating stellar cores," Astron. Astrophys. 246, 417 (1991). Mezzacappa, A., The Road to Prediction: Toward Gravitational Wave Signatures from Core Collapse Supernovae, AIP Conf. Proc. 686 , 29 (2003), Mueller, E. and Rampp, M. and Buras, R. and Janka, H.T. and Shoemaker, D.H., Toward Gravitational Wave Signals from Realistic CoreCollapse Supernova Models, ApJ 603, 221 (2004) Mueller, E. "Simulation of astrophysical fluid flow," in Computational methods for astrophysical fluid flow, SaasFee Advanced Course 27, 343 (1998) Eds. Steiner, O. and Gautschy, A. Berlin, Germany. Springer. Mueller, E. and Janka, H.T. " Gravitational radiation from convective instabilities in type II supernova explosions," Astron. Astrophys., 317, 140 (1997). Mueller, E. "Gravitational Waves from Core Collapse Supernovae," in Astrophysical Sources of Gravitational Radiation, pg. 273 1995. Eds. Marck, J.A. and Lasota, J.P. Cambridge, UK.Cambridge University Press. Mueller, E. " Gravitational radiation from collapsing rotating stellar cores," Astron. Astrophys., 114, 53 (1982). Mueller, E. and Hillebrandt, W. " The collapse of rotating stellar cores," Astron. Astrophys., 103, 358 (1981). Nakamura, T. and Oohara, K. and Kojima, Y. "General relativistic collapse to black holes and gravitational waves from black holes," Prog. Theor. Phys., 90, 1 (1987). Nakamura, T. "General relativistic collapse of accreting neutron stars with rotation," Prog. Theor. Phys., 70, 1144 (1983). Nakamura, T. "General relativistic collapse of axially symmetric stars leading to the formation of rotating black holes," Prog. Theor. Phys., 65, 1876 (1981). Nazin, S.N. and Potsnov, K.A. " High neutron star birth velocities and gravitational radiation during supernova explosions," Astron. Astrophys., 317, L79 (1997). New, K.C.B. " Gravitational Waves from Gravitational Collapse", Living Reviews in Relativity, 6 (2003) New, K. C. B. and Centrella, J. M. and Tohline, J. E. " Gravitational waves from longduration simulations of the dynamical bar instability," Phys. Rev. D. 62. 064019.(2000). Novak, J. and Ibanez, J.M., " Gravitational Waves from the Collapse and Bounce of a Stellar Core in TensorScalar Gravity" ApJ 533, 392 (2000) Ott, C.D. and Burrows, A. and Livne, E. and Walder, R., Gravitational Waves from Axisymmetric, Rotating Stellar Core Collapse, ApJ 600, 834 (2004) Rampp, M. and Mueller, E. and Ruffert, M. " Simulations of nonaxisymmetric rotational core collapse," Astron. Astrophys, 332, 969 (1998). Saenz, R. A. and Shapiro, S. L. " Gravitational radiation from stellar core collapse. III. Damped ellipsiodal oscillations," ApJ, 244, 1033 (1981). Saenz, R. A. and Shapiro, S. L. " Gravitational radiation from stellar core collapse: Ellipsiodal models," ApJ, 221, 286 (1978). Saijo, M. and Shibata, M. and Baumgarte, T. W. and Shapiro, S. L. " Dynamical Bar Instability in Rotating Stars: Effect of General Relativity," ApJ, 548, 919, (2001). Santostasi, G. and Johnson, W. and Frank, J., Detectability of Gravitational Waves from SN1987A, ApJ 586, 1191 (2003) Schneider, R. and Ferrara, A. and Ciardi, B. and Ferrari, V. and Matarrese, S. " Gravitational wave signals from the collapse of the first stars", Mon.Not.Roy.Astron.Soc., 317, 385390 (2000). Seidel, E. "Gravitational radiation from evenparity perturbations of stellar collapse: Mathematical formalism and numerical methods," Phys. Rev. D. 42, 1884 (1990). Seidel, E. and Moore, T. " Gravitational radiation from realistic relativistic stars: Oddparity fluid perturbations," Phys. Rev. D., 35, 2287 (1987). Shibata, M. and Sekiguchi, Y., Threedimensional simulations of stellar core collapse in full general relativity: Nonaxisymmetric dynamical instabilities Phys. Rev. D, submitted; and astroph Shibata, M. and Sekiguchi, Y., Gravitational waves from axisymmetric rotating stellar core collapse to a neutron star in full general relativity Phys. Rev. D69, 084024 (2004) Shibata, M., Axisymmetric general relativistic hydrodynamics: Longterm evolution of neutron stars and stellar collapse to neutron stars and black holes, Phys. Rev. D67, 024033 (2003), Shibata, M. and Baumgarte, T. W. and Shapiro, S. L. " Stability and collapse of rapidly rotating, supramassive neutron stars: 3D simulations in general relativity," Phys. Rev. D. 61. 044012. (2000). Shibata, M. " Axisymmetric simulations of rotating stellar collapse in full general relativity  Criteria for prompt collapse to black holes," Prog. Theor. Phys. 104, 325 (2000). Shibata, M. and Baumgarte, T. W. and Shapiro, S. L. " The BarMode Instability in Differentially Rotating Neutron Stars: Simulations in Full General Relativity," ApJ 542, 453 (2000). Smith, S. C. and Houser, J. L. and Centrella, J. M. " Simulations of nonaxisymmetric instability in a rotating star: A comparison between Eulerian and Smooth Particle Hydrodynamics," ApJ, 458, 236 (1996). Stark, R. F. and Piran, T. "A general relativistic code for rotating axisymmetric configurations and gravitational radiation: Numerical methods and tests," Comp. Phys. Rep., 5, 221 (1987). Stark, R. F. and Piran, T. " Gravitationalwave emission from rotating gravitational collapse," Phys. Rev. Lett., 55, 891 (1985). Turner, M. S. " Gravitational radiation from supernova neutrino bursts," Nature, 274, 565 (1978). van Putten, M.H. and Levinson, A. and Lee, H.K. and Regimbau, T. and Punturo, M. and Harry, G.M., "Gravitational radiation from gammaray burstsupernovae as observational opportunities for LIGO and VIRGO" Phys. Rev. D69, 044007 (2004) van Putten, M.H.P.M. " LIGO/VIRGO searches for gravitational radiation in hypernovae," ApJ, 575, L71 (2002). Wheeler, J. C. and Yi, I. and Höflich, P. and Wang, L. " Asymmetric supernovae, pulsars, magnetars, and gammaray bursts," ApJ, 537, 810 (2000). Wilson, J. R. "A numerical method for relativistic hydrodynamics," in Sources of gravitational radiation, pg. 423, 1979. Eds. Smarr, L. L. Cambridge, U. K. Cambridge University Press. Wilson, J. R. " A numerical study of gravitational stellar collapse," ApJ, 163, 209 (1971). Yamada, S. and Sawai, H., Numerical Study on the Rotational Collapse of Strongly Magnetized Cores of Massive Stars ApJ 608, 907 (2004) Yamada, S. and Sato, K. " Gravitational radiation from rotational collapse of a supernova core," ApJ, 450, 245 (1995). Zwerger, T. and Müller, E. " Dynamics and gravitational wave signature of axisymmetric rotational core collapse," Astron. Astrophys., 320, 209 (1997).
