Curran D. Muhlberger, Ph.D.
Affiliations: | Cornell University, Ithaca, NY, United States |
Area:
Gravitational Physics/Theoretical AstrophysicsGoogle:
"Curran Muhlberger"Mean distance: 12.78
Parents
Sign in to add mentorSaul Arno Teukolsky | grad student | 2014 | Cornell | |
(Numerical simulations of generally relativistic hydrodynamic systems.) |
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Publications
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Deaton MB, Duez MD, Foucart F, et al. (2016) ERRATUM: “BLACK HOLE–NEUTRON STAR MERGERS WITH A HOT NUCLEAR EQUATION OF STATE: OUTFLOW AND NEUTRINO-COOLED DISK FOR A LOW-MASS, HIGH-SPIN CASE” (2013, ApJ, 776, 47) The Astrophysical Journal. 824: 62 |
Tacik N, Foucart F, Pfeiffer HP, et al. (2016) Erratum: Binary neutron stars with arbitrary spins in numerical relativity [Phys. Rev. D92, 124012 (2015)] Physical Review D. 94 |
Haas R, Ott CD, Szilagyi B, et al. (2016) Simulations of inspiraling and merging double neutron stars using the Spectral Einstein Code Physical Review D. 93 |
Barkett K, Scheel MA, Haas R, et al. (2016) Gravitational waveforms for neutron star binaries from binary black hole simulations Physical Review D - Particles, Fields, Gravitation and Cosmology. 93 |
Tacik N, Foucart F, Pfeiffer HP, et al. (2016) Initial data for black hole–neutron star binaries, with rotating stars Classical and Quantum Gravity. 33: 225012 |
Tacik N, Foucart F, Pfeiffer HP, et al. (2015) Binary neutron stars with arbitrary spins in numerical relativity Physical Review D - Particles, Fields, Gravitation and Cosmology. 92 |
Muhlberger CD, Nouri FH, Duez MD, et al. (2014) Magnetic effects on the low- T/ |W | instability in differentially rotating neutron stars Physical Review D - Particles, Fields, Gravitation and Cosmology. 90 |
Deaton MB, Foucart F, Duez MD, et al. (2014) Neutrino-Driven Outflows From Realistic Black Hole-Neutron Star Mergers Bulletin of the American Physical Society. 2014 |
Deaton MB, Duez MD, Foucart F, et al. (2013) Black hole-neutron star mergers with a hot nuclear equation of state: Outflow and neutrino-cooled disk for a low-mass, high-spin case Astrophysical Journal. 776 |