Search Results - "Scheel, M. A"

General relativistic models of binary neutron stars in quasiequilibrium by Baumgarte, T. W., Cook, G. B., Scheel, M. A., Shapiro, S. L., Teukolsky, S. A.

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Stability of relativistic neutron stars in binary orbit by Baumgarte, T. W., Cook, G. B., Scheel, M. A., Shapiro, S. L., Teukolsky, S. A.

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Extending the lifetime of 3D black hole computations with a new hyperbolic system of evolution equations by Kidder, Lawrence E., Scheel, Mark A., Teukolsky, Saul A.

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Hot Hydrocarbon‐Solvent Slot‐Die Coating Enables High‐Efficiency Organic Solar Cells with Temperature‐Dependent Aggregation Behavior by Zhao, Heng, Naveed, Hafiz Bilal, Lin, Baojun, Zhou, Xiaobo, Yuan, Jian, Zhou, Ke, Wu, Hongbo, Guo, Renjun, Scheel, Manuel A., Chumakov, Andrei, Roth, Stephan V., Tang, Zheng, Müller‐Buschbaum, Peter, Ma, Wei

“…Organic solar cells (OSCs) have made rapid progress in terms of their development as a sustainable energy source. However, record‐breaking devices have not…”
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Binary Neutron Stars in General Relativity: Quasiequilibrium Models by Baumgarte, T. W., Cook, G. B., Scheel, M. A., Shapiro, S. L., Teukolsky, S. A.

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Numerical simulations of neutron star-black hole binaries in the near-equal-mass regime by Foucart, F, Duez, M. D, Kidder, L. E, Nissanke, S, Pfeiffer, H. P, Scheel, M. A

“…Phys. Rev. D 99, 103025 (2019) Simulations of neutron star-black hole (NSBH) binaries generally consider black holes with masses in the range $(5-10)M_\odot$,…”
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Stable Characteristic Evolution of Generic Three-Dimensional Single-Black-Hole Spacetimes by Gómez, R., Lehner, L., Marsa, R. L., Winicour, J., Abrahams, A. M., Anderson, A., Anninos, P., Baumgarte, T. W., Bishop, N. T., Brandt, S. R., Browne, J. C., Camarda, K., Choptuik, M. W., Cook, G. B., Correll, R., Evans, C. R., Finn, L. S., Fox, G. C., Haupt, T., Huq, M. F., Kidder, L. E., Klasky, S. A., Laguna, P., Landry, W., Lenaghan, J., Masso, J., Matzner, R. A., Mitra, S., Papadopoulos, P., Parashar, M., Rezzolla, L., Rupright, M. E., Saied, F., Saylor, P. E., Scheel, M. A., Seidel, E., Shapiro, S. L., Shoemaker, D., Smarr, L., Szilágyi, B., Teukolsky, S. A., van Putten, M. H. P. M., Walker, P., York, J. W.

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Boosted Three-Dimensional Black-Hole Evolutions with Singularity Excision by Cook, G. B., Huq, M. F., Klasky, S. A., Scheel, M. A., Abrahams, A. M., Anderson, A., Anninos, P., Baumgarte, T. W., Bishop, N. T., Brandt, S. R., Browne, J. C., Camarda, K., Choptuik, M. W., Correll, R. R., Evans, C. R., Finn, L. S., Fox, G. C., Gómez, R., Haupt, T., Kidder, L. E., Laguna, P., Landry, W., Lehner, L., Lenaghan, J., Marsa, R. L., Masso, J., Matzner, R. A., Mitra, S., Papadopoulos, P., Parashar, M., Rezzolla, L., Rupright, M. E., Saied, F., Saylor, P. E., Seidel, E., Shapiro, S. L., Shoemaker, D., Smarr, L., Suen, W. M., Szilágyi, B., Teukolsky, S. A., van Putten, M. H. P. M., Walker, P., Winicour, J., York, J. W.

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Gravitational Wave Extraction and Outer Boundary Conditions by Perturbative Matching by Abrahams, A. M., Rezzolla, L., Rupright, M. E., Anderson, A., Anninos, P., Baumgarte, T. W., Bishop, N. T., Brandt, S. R., Browne, J. C., Camarda, K., Choptuik, M. W., Cook, G. B., Correll, R. R., Evans, C. R., Finn, L. S., Fox, G. C., Gómez, R., Haupt, T., Huq, M. F., Kidder, L. E., Klasky, S. A., Laguna, P., Landry, W., Lehner, L., Lenaghan, J., Marsa, R. L., Masso, J., Matzner, R. A., Mitra, S., Papadopoulos, P., Parashar, M., Saied, F., Saylor, P. E., Scheel, M. A., Seidel, E., Shapiro, S. L., Shoemaker, D., Smarr, L., Szilágyi, B., Teukolsky, S. A., van Putten, M. H. P. M., Walker, P., Winicour, J., York, J. W.

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In Situ Study of FePt Nanoparticles‐Induced Morphology Development during Printing of Magnetic Hybrid Diblock Copolymer Films by Cao, Wei, Yin, Shanshan, Bitsch, Martin, Liang, Suzhe, Plank, Martina, Opel, Matthias, Scheel, Manuel A., Gallei, Markus, Janka, Oliver, Schwartzkopf, Matthias, Roth, Stephan V., Müller‐Buschbaum, Peter

“…The development of magnetic hybrid films containing diblock copolymers (DBCs) and magnetic nanoparticles (NPs) by printing is a highly promising method for…”
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Equilibrium and stability of relativistic cylindrical polytropes by SCHEEL, M. A, SHAPIRO, S. L, TEUKOLSKY, S. A

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A multidomain spectral method for solving elliptic equations by Pfeiffer, Harald P., Kidder, Lawrence E., Scheel, Mark A., Teukolsky, Saul A.

“…We present a new solver for coupled nonlinear elliptic partial differential equations (PDEs). The solver is based on pseudo-spectral collocation with domain…”
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Numerical evolution of black holes with a hyperbolic formulation of general relativity by Scheel, Mark A., Baumgarte, Thomas W., Cook, Gregory B., Shapiro, Stuart L., Teukolsky, Saul A.

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Dynamical gauge conditions for the Einstein evolution equations by Lindblom, Lee, Scheel, Mark A.

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Black hole evolution by spectral methods by Kidder, Lawrence, Scheel, Mark, Teukolsky, Saul, Carlson, Eric, Cook, Gregory

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Energy norms and the stability of the Einstein evolution equations by Lindblom, Lee, Scheel, Mark A.

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Waveform propagation in black hole spacetimes: Evaluating the quality of numerical solutions by Rezzolla, L., Abrahams, A. M., Baumgarte, T. W., Cook, G. B., Scheel, M. A., Shapiro, S. L., Teukolsky, S. A.

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General Relativistic Models of Binary Neutron Stars in Quasiequilibrium by Baumgarte, T. W, Cook, G. B, Scheel, M. A, Shapiro, S. L, Teukolsky, S. A

“…Phys. Rev. D 57, 7299 (1998) We perform fully relativistic calculations of binary neutron stars in corotating, circular orbit. While Newtonian gravity allows…”
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The Stability of Relativistic Neutron Stars in Binary Orbit by Baumgarte, T. W, Cook, G. B, Scheel, M. A, Shapiro, S. L, Teukolsky, S. A

“…Phys.Rev. D57 (1998) 6181-6184 We analyze the stability of relativistic, quasi-equilibrium binary neutron stars in synchronous circular orbit. We explore…”
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Binary Neutron Stars in General Relativity: Quasi-Equilibrium Models by Baumgarte, T. W, Cook, G. B, Scheel, M. A, Shapiro, S. L, Teukolsky, S. A

“…Phys.Rev.Lett. 79 (1997) 1182-1185 We perform fully relativistic calculations of binary neutron stars in quasi-equilibrium circular orbits. We integrate…”
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