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Numerical Relativity Publications

Numerical Relativity Publications using Cactus Code
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[1] G. M. Manca, L. Baiotti, R. De Pietri, and L. Rezzolla. Dynamical non-axisymmetric instabilities in rotating relativistic stars, 2007.
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[2] M. Campanelli, C. O. Lousto, and Y. Zlochower. Spin-orbit interactions in black-hole binaries. page 9, August 2006.
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[3] M. Campanelli, C. O. Lousto, and Y. Zlochower. Spinning-black-hole binaries: The orbital hang up. Physical Review D, 74:041501, April 2006.
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[4] M. Campanelli, B. J. Kelly, and C. O. Lousto. The Lazarus Project. II. Spacelike extraction with the quasi-Kinnersley tetrad. Physical Review D, 73:064005, 2006.
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[5] Frank Löffler, Luciano Rezzolla, and Marcus Ansorg. Numerical evolutions of a black hole-neutron star system in full general relativity, 2006.
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[6] Luca Baiotti, Roberto De Pietri, Gian Mario Manca, and Luciano Rezzolla. Accurate simulations of the dynamical barmode instability in full General Relativity, 2006.
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[7] Peter Diener, Frank Herrmann, Denis Pollney, Erik Schnetter, Edward Seidel, Ryoji Takahashi, Jonathan Thornburg, and Jason Ventrella. Accurate evolution of orbiting binary black holes. Physical Review Letters, 96:121101, 2006.
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[8] Carlos F. Sopuerta, Ulrich Sperhake, and Pablo Laguna. Hydro-without-hydro framework for simulations of black hole-neutron star binaries. Classical and Quantum Gravity, 23:S579, 2006.
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[9] Ulrich Sperhake. Binary black-hole evolutions of excision and puncture data, 2006.
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[10] M. Campanelli, C. O. Lousto, and Y. Zlochower. The last orbit of binary black holes. Physical Review D, 73:061501, January 2006.
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[11] F. Herrmann, D. Shoemaker, and P. Laguna. Unequal-mass binary black hole inspirals, 2006.
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[12] Erik Schnetter, Peter Diener, Ernst Nils Dorband, and Manuel Tiglio. A multi-block infrastructure for three-dimensional time-dependent numerical relativity. Classical and Quantum Gravity, 23:S553, 2006.
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[13] Ke-Jian Jin and Wai-Mo Suen. Critical phenomena in head-on collisions of neutron stars. 2006.
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[14] Luca Baiotti and Luciano Rezzolla. Challenging the paradigm of singularity excision in gravitational collapse, 2006.
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[15] Erik Schnetter, Badri Krishnan, and Florian Beyer. Introduction to dynamical horizons in numerical relativity. Physical Review D, 74:024028, 2006.
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[16] Ernst Nils Dorband, Emanuele Berti, Peter Diener, Erik Schnetter, and Manuel Tiglio. A numerical study of the quasinormal mode excitation of kerr black holes. 2006.
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[17] M. Campanelli, C. O. Lousto, P. Marronetti, and Y. Zlochower. Accurate Evolutions of Orbiting Black-Hole Binaries Without Excision. Physical Review Letters, 96:111101, 2006.
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[18] Miguel Alcubierre, Bernd Brügmann, Peter Diener, Francisco Siddhartha Guzmán, Ian Hawke, Scott Hawley, Frank Herrmann, Michael Koppitz, Denis Pollney, Edward Seidel, and Jonathan Thornburg. Dynamical evolution of quasi-circular binary black hole data. Physical Review D, 72:044004 (14 pages), August 5 2005.
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[19] Y. Zlochower, J.G. Baker, M. Campanelli, and C.O. Lousto. Accurate black hole evolutions by fourth-order numerical relativity. Physical Review D, 72:024021, May 2005.
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[20] Miguel Alcubierre, Peter Diener, Francisco Siddhartha Guzmán, Scott Hawley, Michael Koppitz, Denis Pollney, and Edward Seidel. Shift Conditions for Orbiting Binaries in Numerical Relativity. in preparation, 2005.
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[21] Luca Baiotti, Ian Hawke, Luciano Rezzolla, and Erik Schnetter. Gravitational-wave emission from rotating gravitational collapse in three dimensions. Phys. Rev. Lett., 94:131101, 2005.
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[22] Burkhard Zink, Nikolaos Stergioulas, Ian Hawke, Christian D. Ott, Erik Schnetter, and Ewald Müller. Black hole formation through fragmentation of toroidal polytropes. 2005.
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[23] Edwin Evans, Sai Iyer, Erik Schnetter, Wai-Mo Suen, Jian Tao, Randy Wolfmeyer, and Hui-Min Zhang. Computational relativistic astrophysics with adaptive mesh refinement: Testbeds. Phys. Rev. D, 71:081301(R), 2005.
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[24] Jonathan Thornburg. Event and apparent horizon finders for 3+1 numerical relativity, 2005.
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[25] Erik Schnetter, Frank Herrmann, and Denis Pollney. Horizon pretracking. Phys. Rev. D, 71:044033, 2005.
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[26] Burkhard Zink, Nikolaos Stergioulas, Ian Hawke, Christian D. Ott, Erik Schnetter, and Ewald Müller. Black hole formation through fragmentation of toroidal polytropes. 2005.
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[27] I. Hawke, F. Löffler, and A. Nerozzi. Excision methods for high resolution shock capturing schemes applied to general relativistic hydrodynamics. Phys. Rev. D, 71:104006, 2005.
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[28] Andrea Nerozzi, Marco Bruni, Virginia Re, and Lior M Burko. Towards a Wave-extraction Method for Numerical Relativity: IV. Testing the Quasi-Kinnersley Method in the Bondi-Sachs framework, 2005.
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[29] Abhay Ashtekar and Gregory J Galloway. Some uniqueness results for dynamical horizons, 2005.
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[30] J. Balakrishna, R. Bondarescu, G. Daues, F. S. Guzmán, and E. Seidel. Evolution of 3D Boson Stars with Waveform Extraction. 2005. (Submitted).
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[31] Mark D Hannam. Quasi-circular orbits of conformal thin-sandwich puncture binary black holes. Physical Review D, 72:044025, 2005.
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[32] Pedro Marronetti. Hamiltonian relaxation. Classical and Quantum Gravity, 22:2433, 2005.
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[33] Peter Diener, Ernst Nils Dorband, Erik Schnetter, and Manuel Tiglio. New, efficient, and accurate high order derivative and dissipation operators satisfying summation by parts, and applications in three-dimensional multi-block evolutions, 2005.
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[34] Luca Baiotti, Ian Hawke, Pedro J. Montero, Frank Löffler, Luciano Rezzolla, Nikolaos Stergioulas, Jose A. Font, and Ed Seidel. Three-dimensional relativistic simulations of rotating neutron star collapse to a kerr black hole. Phys. Rev. D, 71:024035, 2005.
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[35] U Sperhake, B Kelly, P Laguna, K L Smith, and E Schnetter. Black hole head-on collisions and gravitational waves with fixed mesh-refinement and dynamic singularity excision. Physical Review D, 71:124042, 2005.
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[36] Erik Schnetter, Scott H. Hawley, and Ian Hawke. Evolutions in 3D numerical relativity using fixed mesh refinement. Class. Quantum Grav., 21(6):1465-1488, March 21 2004.
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[37] Harald Dimmelmeier, Jerome Novak, Jose A. Font, Jose M. Ibanez, and Ewald Müller. ``Mariage des Maillages'': A new numerical approach for 3D relativistic core collapse simulations. 2004.
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[38] Carsten Gundlach and Jose M. Martin-Garcia. Symmetric hyperbolicity and consistent boundary conditions for second-order Einstein equations. Phys. Rev., D70:044032, 2004.
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[39] Maria Babiuc, Bela Szilagyi, and Jeffrey Winicour. Some mathematical problems in numerical relativity, 2004.
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[40] Bernd Reimann and Bernd Brügmann. Maximal slicing for puncture evolutions of Schwarzschild and Reissner - Nordstrom black holes. Phys. Rev. D, 69:044006, 2004.
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[41] Miguel Alcubierre, Bernd Brügmann, Peter Diener, Frank Herrmann, Denis Pollney, Edward Seidel, and Ryoji Takahashi. Testing excision techniques for dynamical 3D black hole evolutions. submitted to Phys. Rev. D, 2004.
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[42] J. Baker, M. Campanelli, C. O. Lousto, and R. Takahashi. Coalescence remnant of spinning binary black holes. Phys. Rev., D69:027505, 2004.
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[43] C. Bona, T. Ledvinka, C. Palenzuela, and M. Zacek. A symmetry-breaking mechanism for the Z4 general-covariant evolution system. Phys. Rev. D, 69:064036, 2004.
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[44] U Sperhake, K L Smith, B Kelly, P Laguna, and D Shoemaker. Impact of densitized lapse slicings on evolutions of a wobbling black hole. Physical Review D, 69:024012, 2004.
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[45] Miguel Alcubierre, Gabrielle Allen, Thomas W. Baumgarte, Carles Bona, David Fiske, Tom Goodale, Francisco Siddhartha Guzmán, Ian Hawke, Scott Hawley, Sascha Husa, Michael Koppitz, Christiane Lechner, Lee Lindblom, Denis Pollney, David Rideout, Marcelo Salgado, Erik Schnetter, Edward Seidel, Hisa aki Shinkai, Deirdre Shoemaker, Bela Szilagyi, Ryoji Takahashi, and Jeffrey Winicour. Towards standard testbeds for numerical relativity. Class. Quantum Grav., 21(2):589-613, 2004.
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[46] Manuel Tiglio, Luis Lehner, and David Neilsen. 3d simulations of einstein's equations: symmetric hyperbolicity, live gauges and dynamic control of the constraints. Physical Review D, 70:104018, 2004.
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[47] Bernd Reimann and Bernd Brügmann. Late time analysis for maximal slicing of Reissner-Nordstrom puncture evolutions. Phys. Rev. D, 69:124009, 2004.
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[48] David R Fiske. Toward making the constraint hypersurface an attractor in free evolution. Physical Review D, 69:047501, 2004.
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[49] Jonathan Thornburg. A Fast Apparent-Horizon Finder for 3-Dimensional Cartesian Grids in Numerical Relativity. Class. Quantum Grav., 21(2):743-766, January 2004.
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[50] C. Gundlach and J.M. Martin-Garcia. Symmetric hyperbolic form of systems of second-order evolution equations subject to constraints. Phys. Rev., D70:044031, 2004.
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[51] Luis Lehner, David Neilsen, Oscar Reula, and Manuel Tiglio. The discrete energy method in numerical relativity: Towards long-term stability. Classical and Quantum Gravity, 21:5819, 2004.
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[52] Sascha Husa, Ian Hinder, and Christiane Lechner. Kranc: a mathematica application to generate numerical codes for tensorial evolution equations. 2004.
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[53] Miguel Alcubierre, Alejandro Corichi, Jose A. Gonzalez, Dario Nu nez, and Marcelo Salgado. A hyperbolic slicing condition adapted to killing fields and densitized lapses. Class. Quantum Grav., 20(18):3951-3968, September 2003.
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[54] Mark Miller and Wai-Mo Suen. Towards a realistic neutron star binary inspiral, 2003.
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[55] Sascha Husa and Christiane Lechner. Computer algebra applications for numerical relativity. 2003.
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[56] Erik Schnetter. Finding apparent horizons and other two-surfaces of constant expansion. Class. Quantum Grav., 20(22):4719-4737, 2003.
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[57] W Tichy, B Brügmann, M Campanelli, and P Diener. Binary black hole initial data for numerical general relativity based on post-newtonian data. Physical Review D, 67:064008, 2003.
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[58] Bela Szilagyi and Jeffrey Winicour. Well-posed initial-boundary evolution in general relativity. Physical Review D, 68:041501, 2003.
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[59] Miguel Alcubierre, Bernd Brügmann, Peter Diener, Michael Koppitz, Denis Pollney, Edward Seidel, and Ryoji Takahashi. Gauge conditions for long-term numerical black hole evolutions without excision. Phys. Rev. D, 67:084023, 2003.
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[60] Michael Koppitz, Miguel Alcubierre, Bernd Brügmann, Ian Hawke, Denis Pollney, and Edward Seidel. Numerical evolutions of quasi-stationary black hole initial data. 2003. in preparation.
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[61] L. Baiotti, I. Hawke, P. Montero, and L. Rezzolla. A new three-dimensional general-relativistic hydrodynamics code. In R. Capuzzo-Dolcetta, editor, Computational Astrophysics in Italy: Methods and Tools, volume 1, page 327, Trieste, 2003. Mem. Soc. Astron. It. Suppl.
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[62] J. A. Font. Numerical hydrodynamics in general relativity. Liv. Rev. Relativ., 6:4, 2003.
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[63] Edwin Evans, A. Gopakumar, Philip Gressman, Sai Iyer, Mark Miller, Wai-Mo Suen, and Hui-Min Zhang. Head-on/Near Head-on Collisions of Neutron Stars With a Realistic EOS. Phys. Rev., D67:104001, 2003.
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[64] N. Stergioulas and I. Hawke. Equilibrium and pulsations of rotating stars in numerical relativity. In K. D. Kokkotas and N. Stergioulas, editors, Recent Developments in Gravity, Proceedings of the 10th Hellenic Relativity Conference, page 185, Singapore, 2003. World Scientific.
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[65] J. Baker, M. Campanelli, C. O. Lousto, and R. Takahashi. The final plunge of spinning binary black holes. 2003.
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[66] S. Brandt, K. Camarda, E. Seidel, and R. Takahashi. Three dimensional distorted black holes. Class. Quantum Grav., 20:1-20, 2003.
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[67] D Shoemaker, K Smith, U Sperhake, P Laguna, E Schnetter, and D Fiske. Moving black holes via singularity excision. Classical and Quantum Gravity, 20:3729, 2003.
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[68] M W Choptuik, L Lehner, I Olabarrieta, R Petryk, F Pretorius, and H Villegas. Towards the final fate of an unstable black string. Physical Review D, 68:044001, 2003.
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[69] M. Alcubierre, A. Corichi, J.A. Gonzalez, D. Nu nez, and M. Salgado. Hyperbolicity of the KST formulation of Einstein's equations coupled to a modified Bona-Masso slicing condition. Phys. Rev. D, 67:104021, 2003.
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[70] Miguel Alcubierre, John Baker, , Bernd Brügmann, Manuela Campanelli, Peter Diener, Frank Herrmann, Carlos O. Lousto, Denis Pollney, and Edward Seidel. Gravitational waveforms from black hole collisions. 2003. in preparation.
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[71] Yosef Zlochower, Roberto Gómez, Sascha Husa, Luis Lehner, and Jeffrey Winicour. Mode coupling in the nonlinear response of black holes. Physical Review D, 68:084014, 2003.
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[72] P. Diener. A new general purpose event horizon finder for 3D numerical spacetimes. Class. Quantum Grav., 20(22):4901-4917, 2003.
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[73] J Baker, M Campanelli, C O Lousto, and R Takahashi. Modeling gravitational radiation from coalescing binary black holes. Physical Review D, 65:124012, 2002.
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[74] B. D. Baker. Binary black holes in quasi-stationary circular orbits. 2002.
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[75] Hisa aki Shinkai and Gen Yoneda. Re-formulating the einstein equations for stable numerical simulations: Formulation problem in numerical relativity, 2002.
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[76] D. N. Vulcanov. Doing numerical cosmology with the cactus code, 2002.
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[77] Dumitru N Vulcanov and Miguel Alcubierre. Testing the Cactus Code on Exact Solutions of the Einstein Field Equations. International Journal of Modern Physics C, 13(6):805-822, 2002.
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[78] Jose. A. Font, Tom Goodale, Sai Iyer, Mark Miller, Luciano Rezzolla, Edward Seidel, Nikolaos Stergioulas, Wai-Mo Suen, and Malcolm Tobias. Three-dimensional general relativistic hydrodynamics. II. Long-term dynamics of single relativistic stars. Phys. Rev. D, 65:084024, 2002.
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[79] Miguel Alcubierre, F Siddhartha Guzmán, Tonatiuh Matos, Dario Nu nez, L Arturo Urena-Lopez, and Petra Wiederhold. Galactic collapse of scalar field dark matter. Class. Quantum Grav., 19(19):5017-5024, 2002.
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[80] Philip Gressman, Lap-Ming Lin, Wai-Mo Suen, N Stergioulas, and John L Friedman. Nonlinear r-modes in neutron stars: Instability of an unstable mode. Physical Review D, 66:041303R, 2002.
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[81] M. Bondarescu, M. Alcubierre, and E. Seidel. Isometric embeddings of black hole horizons in three-dimensional flat space. Class. Quantum Grav., 19(2):375-392, January 2002.
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[82] Sascha Husa. Problems and successes in the numerical approach to the conformal field equations. LECT.NOTES PHYS., 604:239, 2002.
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[83] John Baker, Manuela Campanelli, and Carlos O. Lousto. The Lazarus project: A pragmatic approach to binary black hole evolutions. Phys. Rev. D, 65:044001, 2002.
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[84] Nikolaos Stergioulas and Jose A Font. Nonlinear r-modes in rapidly rotating relativistic stars. Physical Review Letters, 86:1148, 2001.
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[85] M. Alcubierre, W. Benger, B. Brügmann, G. Lanfermann, L. Nerger, E. Seidel, and R. Takahashi. 3D Grazing Collision of Two Black Holes. Phys. Rev. Lett., 87:271103, 2001.
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[86] C O Lousto. Perturbative evolution of nonlinear initial data for binary black holes: Zerilli vs. teukolsky. Physical Review D, 63:047504, 2001.
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[87] C. Gundlach and J.M. Martin-Garcia. Gauge-invariant and coordinate-independent perturbations of stellar collapse ii: matching to the exterior. Phys. Rev. D, 64:024012, 2001.
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[88] M. Alcubierre and B. Brügmann. Simple excision of a black hole in 3+1 numerical relativity. Phys. Rev. D, 63:104006, 2001.
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[89] J. Baker, B. Brügmann, Manuela Campanelli, C. O. Lousto, and R. Takahashi. Plunge waveforms from inspiralling binary black holes. Phys. Rev. Lett., 87:121103, 2001.
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[90] M. Alcubierre, S. Brandt, B. Brügmann, D. Holz, E. Seidel, R. Takahashi, and J. Thornburg. Symmetry without symmetry: Numerical simulation of axisymmetric systems using Cartesian grids. Int. J. Mod. Phys. D, 10(3):273-289, 2001.
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[91] Miguel Alcubierre, Bernd Brügmann, Denis Pollney, Edward Seidel, and Ryoji Takahashi. Black hole excision for dynamic black holes. Phys. Rev. D, 64:061501(R), 2001.
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[92] Miguel Alcubierre, Bernd Brügmann, Denis Pollney, Edward Seidel, and Ryoji Takahashi. Black Hole Excision for Dynamic Black Holes. Physical Review D, 64:061501, 2001.
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[93] Mark Miller, Wai-Mo Suen, and Malcolm Tobias. The shapiro conjecture: Prompt or delayed collapse in the head-on collision of neutron stars? Physical Review D, 63:121501, 2001.
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[94] M. Alcubierre, S. Brandt, B. Brügmann, C. Gundlach, J. Massó, E. Seidel, and P. Walker. Test-beds and applications for apparent horizon finders in numerical relativity. Class. Quantum Grav., 17:2159-2190, 2000.
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[95] S Brandt, J A Font, J M Ibanez, J Massó, and E Seidel. Numerical evolution of matter in dynamical axisymmetric black hole spacetimes. i. methods and tests. Computer Physics Communications, 124:169, 2000.
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[96] J. A. Font, M. Miller, W. M. Suen, and M. Tobias. Three-dimensional numerical general relativistic hydrodynamics: Formulations, methods, and code tests. Phys. Rev. D, 61:044011, 2000.
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[97] Miguel Alcubierre, Bernd Brügmann, Thomas Dramlitsch, Jose A Font, Philippos Papadopoulos, Edward Seidel, Nikolaos Stergioulas, and Ryoji Takahashi. Towards a stable numerical evolution of strongly gravitating systems in general relativity: The conformal treatments. Physical Review D, 62:044034, 2000.
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[98] John Baker, Bernd Brügmann, Manuela Campanelli, and Carlos O. Lousto. Gravitational waves from black hole collisions via an eclectic approach. Class. Quantum Grav., 17:L149-L156, 2000.
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[99] M. Alcubierre, G. Allen, B. Brügmann, G. Lanfermann, E. Seidel, W.-M. Suen, and M. Tobias. Gravitational collapse of gravitational waves in 3D numerical relativity. Phys. Rev. D, 61:041501 (R), 2000.
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[100] Steve Brandt, Randall Correll, Roberto Gómez, Mijan Huq, Pablo Laguna, Luis Lehner, Pedro Marronetti, Richard A Matzner, David Neilsen, Jorge Pullin, Erik Schnetter, Deirdre Shoemaker, and Jeffrey Winicour. Grazing collisions of black holes via the excision of singularities. Physical Review Letters, 85:5496, 2000.
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[101] P. Diener, N. Jansen, A. Khokhlov, and I. Novikov. Adaptive mesh refinement approach to construction of initial data for black hole collisions. Class. Quantum Grav., 17:435-451, 2000.
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[102] C. Gundlach and J.M. Martin-Garcia. Gauge-invariant and coordinate-independent perturbations of stellar collapse i: the interior. Phys. Rev. D, 61:08024, 2000.
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[103] J. Baker, S. R. Brandt, M. Campanelli, C. O. Lousto, E. Seidel, and R. Takahashi. Nonlinear and perturbative evolution of distorted black holes: Odd-parity modes. Phys. Rev. D, 62:127701, 2000.
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[104] M. Alcubierre, G. Allen, B. Brügmann, E. Seidel, and W.-M. Suen. Towards an understanding of the stability properties of the 3+1 evolution equations in general relativity. Phys. Rev. D, 62:124011, 2000.
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[105] J. Baker, S. R. Brandt, M. Campanelli, C. O. Lousto, E. Seidel, and R. Takahashi. Nonlinear and perturbative evolution of distorted black holes: Odd-parity modes. Phys. Rev., D62:127701, 2000.
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[106] J. Baker and M. Campanelli. Making use of geometrical invariants in black hole collisions. Phys. Rev. D, 62:127501, 2000.
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[107] B. Brügmann. Numerical relativity in 3+1 dimensions. Ann. Phys. (Leipzig), 9:227-246, 2000.
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[108] Miguel Alcubierre, Gabrielle Allen, Bernd Brügmann, Gerd Lanfermann, Edward Seidel, Wai-Mo Suen, and Malcolm Tobias. Gravitational collapse of gravitational waves in 3d numerical relativity. Physical Review D, 61:041501, 2000.
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[109] C. Gundlach. Critical phenomena in gravitational collapse. Living Rev. Rel., 2:4, 1999.
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[110] Edward Seidel and Wai-Mo Suen. Numerical relativity as a tool for computational astrophysics. J. Comp. Appl. Math., 109:493, 1999.
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[111] A. Arbona, C. Bona, J. Massó, and J. Stela. Robust evolution system for Numerical Relativity. Phys. Rev. D, 60:104014, 1999.
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[112] Edward Seidel. Technologies for Collaborative, Large Scale Simulation in Astrophysics and a General Toolkit for solving PDE's in Science and Engineering. In T. Plesser and P. Wittenburg, editors, Forschung und wissenschaftliches Rechnen. Max-Planck-Gesselschaft, München, 1999.
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[113] J. Baker and R. Puzio. A new method for solving the initial value problem with application to multiple black holes. Phys. Rev. D, 59:044030, 1999.
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[114] J. Massó, E. Seidel, Wai-Mo Suen, and P. Walker. Event horizons in numerical relativity. II. Analyzing the horizon. Phys. Rev. D, 59:064015, 1999.
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[115] M. Alcubierre, B. Brügmann, M. Miller, and W.-M. Suen. A conformal hyperbolic formulation of the Einstein equations. Phys. Rev. D, 60:064017, 1999.
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[116] Edward Seidel. Black Hole Coalescence and Mergers: Review, Status, and ``Where are We Heading?''. Prog. Theor. Phys. Suppl., 136:87-106, 1999.
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[117] C. Gundlach and P. Walker. Causal differencing of flux-conservative equations applied to black hole spacetimes. Class. Quantum Grav., 16:991-1010, 1999.
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[118] C. Gundlach. Pseudo-spectral apparent horizon finders: An efficient new algorithm. Phys. Rev. D, 57:863-875, 1998.
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[119] Carsten Gundlach. Angular momentum at the black hole threshold. Phys. Rev. D, 57:R7080, 1998.
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[120] C. Gundlach. Nonspherical perturbations of critical collapse and cosmic censorship. Phys. Rev. D, 57:R7075, 1998.
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[121] Edward Seidel. A numerical approach to black holes. In F. Hehl, editor, Bad Honnef Meeting on Black Holes. Springer-Verlag, 1998.
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[122] Carsten Gundlach. Nonspherical perturbations of critical collapse and cosmic censorship. 1998.
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[123] Carles Bona, Joan Massó, Edward Seidel, and Paul Walker. Three dimensional numerical relativity with a hyperbolic formulation. 1998.
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[124] Carsten Gundlach. Critical phenomena in gravitational collapse. Adv. Theor. Math. Phys, 2:1, 1998.
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[125] Edward Seidel. Numerical relativity: Towards simulations of 3D black hole coalescence, 1998.
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[126] C. Gundlach and J. Pullin. Instability of free evolution in double null coordinates. Class. Quantum Grav., 14:991, 1997.
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[127] C. Gundlach. Understanding critical collapse of a scalar field. Phys. Rev. D, 55:695, 1997.
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[128] Peter Diener, Ryoji Takahashi, Denis Pollney, and Edward Seidel. The Evolution of 3D Rotating Distorted Black Holes. in preparation.
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