Daniel Hemberger, Ph.D. - Publications

Affiliations: 
Cornell University, Ithaca, NY, United States 
 Astronomy California Institute of Technology, Pasadena, CA 
Area:
Gravitational Physics/Theoretical Astrophysics

12 high-probability publications. We are testing a new system for linking publications to authors. You can help! If you notice any innacuracies, please sign in and mark papers as correct or incorrect matches. If you identify any major omissions or other inaccuracies in the publication list, please let us know.

Year Citation  Score
2015 Blackman J, Field SE, Galley CR, Szilágyi B, Scheel MA, Tiglio M, Hemberger DA. Fast and Accurate Prediction of Numerical Relativity Waveforms from Binary Black Hole Coalescences Using Surrogate Models. Physical Review Letters. 115: 121102. PMID 26430979 DOI: 10.1103/PhysRevLett.115.121102  0.8
2015 Lovelace G, Scheel MA, Owen R, Giesler M, Katebi R, Szilágyi B, Chu T, Demos N, Hemberger DA, Kidder LE, Pfeiffer HP, Afshari N. Nearly extremal apparent horizons in simulations of merging black holes Classical and Quantum Gravity. 32. DOI: 10.1088/0264-9381/32/6/065007  0.8
2015 Scheel MA, Giesler M, Hemberger DA, Lovelace G, Kuper K, Boyle M, Szilágyi B, Kidder LE. Improved methods for simulating nearly extremal binary black holes Classical and Quantum Gravity. 32. DOI: 10.1088/0264-9381/32/10/105009  0.8
2014 Taracchini A, Buonanno A, Pan Y, Hinderer T, Boyle M, Hemberger DA, Kidder LE, Lovelace G, Mroué AH, Pfeiffer HP, Scheel MA, Szilágyi B, Taylor NW, Zenginoglu A. Effective-one-body model for black-hole binaries with generic mass ratios and spins Physical Review D - Particles, Fields, Gravitation and Cosmology. 89. DOI: 10.1103/PhysRevD.89.061502  0.8
2014 Hinder I, Buonanno A, Boyle M, Etienne ZB, Healy J, Johnson-Mcdaniel NK, Nagar A, Nakano H, Pan Y, Pfeiffer HP, Pürrer M, Reisswig C, Scheel MA, Schnetter E, Sperhake U, ... ... Hemberger DA, et al. Error-analysis and comparison to analytical models of numerical waveforms produced by the NRAR Collaboration Classical and Quantum Gravity. 31. DOI: 10.1088/0264-9381/31/2/025012  0.8
2013 Mroué AH, Scheel MA, Szilágyi B, Pfeiffer HP, Boyle M, Hemberger DA, Kidder LE, Lovelace G, Ossokine S, Taylor NW, Zenginoğlu A, Buchman LT, Chu T, Foley E, Giesler M, et al. Catalog of 174 binary black hole simulations for gravitational wave astronomy. Physical Review Letters. 111: 241104. PMID 24483642 DOI: 10.1103/PhysRevLett.111.241104  0.8
2013 Le Tiec A, Buonanno A, Mroué AH, Pfeiffer HP, Hemberger DA, Lovelace G, Kidder LE, Scheel MA, Szilágyi B, Taylor NW, Teukolsky SA. Periastron advance in spinning black hole binaries: Gravitational self-force from numerical relativity Physical Review D - Particles, Fields, Gravitation and Cosmology. 88. DOI: 10.1103/PhysRevD.88.124027  0.8
2013 Hinderer T, Buonanno A, Mroué AH, Hemberger DA, Lovelace G, Pfeiffer HP, Kidder LE, Scheel MA, Szilagyi B, Taylor NW, Teukolsky SA. Periastron advance in spinning black hole binaries: Comparing effective-one-body and numerical relativity Physical Review D - Particles, Fields, Gravitation and Cosmology. 88. DOI: 10.1103/PhysRevD.88.084005  0.8
2013 Hemberger DA, Lovelace G, Loredo TJ, Kidder LE, Scheel MA, Szilágyi B, Taylor NW, Teukolsky SA. Final spin and radiated energy in numerical simulations of binary black holes with equal masses and equal, aligned or antialigned spins Physical Review D - Particles, Fields, Gravitation and Cosmology. 88. DOI: 10.1103/PhysRevD.88.064014  0.8
2013 Hemberger DA, Scheel MA, Kidder LE, Szilágyi B, Lovelace G, Taylor NW, Teukolsky SA. Dynamical excision boundaries in spectral evolutions of binary black hole spacetimes Classical and Quantum Gravity. 30. DOI: 10.1088/0264-9381/30/11/115001  0.8
2011 Hemberger D, Walsh JA. Fractals in the 3-body problem via symplectic integration The Beauty of Fractals: Six Different Views. 75-94. DOI: 10.1017/CBO9780883859711.007  0.8
2008 Hemberger DA, Stinebring DR. Time variability of interstellar scattering and improvements to pulsar timing Astrophysical Journal. 674: L37-L40. DOI: 10.1086/528985  0.8
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