Area of research
Astronomy and Astrophysics · Atomic and Molecular Physics, and Optics
Research interest
Research interests include Physics, Gravitational wave, Waveform, Numerical relativity, Spins, and Binary black hole.
The SXS collaboration’s third catalog of binary black hole simulations
Multipolar effective-one-body waveforms for precessing binary black holes: Construction and validation
The SXS collaboration catalog of binary black hole simulations
On the properties of the massive binary black hole merger GW170729
Improved effective-one-body model of spinning, nonprecessing binary black holes for the era of gravitational-wave astrophysics with advanced detectors
Numerical relativity waveform surrogate model for generically precessing binary black hole mergers
Complete waveform model for compact binaries on eccentric orbits
Parameter estimation method that directly compares gravitational wave observations to numerical relativity
Effects of Neutron-Star Dynamic Tides on Gravitational Waveforms within the Effective-One-Body Approach
Fast and Accurate Prediction of Numerical Relativity Waveforms from Binary Black Hole Coalescences Using Surrogate Models
Post-merger evolution of a neutron star-black hole binary with neutrino transport
Approaching the Post-Newtonian Regime with Numerical Relativity: A Compact-Object Binary Simulation Spanning 350 Gravitational-Wave Cycles
Effective-one-body model for black-hole binaries with generic mass ratios and spins
Inspiral-merger-ringdown waveforms of spinning, precessing black-hole binaries in the effective-one-body formalism
Neutron star-black hole mergers with a nuclear equation of state and neutrino cooling: Dependence in the binary parameters
Catalog of 174 Binary Black Hole Simulations for Gravitational Wave Astronomy
Black-hole–neutron-star mergers at realistic mass ratios: Equation of state and spin orientation effects
BLACK HOLE-NEUTRON STAR MERGERS WITH A HOT NUCLEAR EQUATION OF STATE: OUTFLOW AND NEUTRINO-COOLED DISK FOR A LOW-MASS, HIGH-SPIN CASE
Final spin and radiated energy in numerical simulations of binary black holes with equal masses and equal, aligned or antialigned spins
First direct comparison of nondisrupting neutron star-black hole and binary black hole merger simulations
High-accuracy gravitational waveforms for binary black hole mergers with nearly extremal spins
Black hole-neutron star mergers for<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mn>10</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:msub><mml:mi>M</mml:mi><mml:mo>⊙</mml:mo></mml:msub></mml:math>black holes