activity
20092023
most citedAbout 30% of Sun-like Stars Have Kepler-like Planetary Systems: A Study of their Intrinsic Architecture

263 citations · 2.8k across the 46 of their papers we have counts for

collaborators
Showing astro-ph.HEShow all

9 papers · 1 filter

astro-ph.HE2022

Eccentric Mergers of Intermediate-Mass Black Holes from Evection Resonances in AGN Disks

Diego J. Muñoz, Nicholas C. Stone, Cristobal Petrovich +1

We apply the theory of nonlinear resonance capture to the problem of a black hole binary (BHB) orbiting a supermassive black hole (SMBH) while embedded in the accretion disk of an…

astro-ph.HE2019★ 30 cited

Compact-Object Mergers in the Galactic Center: Evolution in Triaxial Clusters

Mathew W. Bub, Cristobal Petrovich

There is significant observational evidence that a large fraction of galactic centers, including those in the Milky Way and M31, host a supermassive black hole (SMBH) embedded in a…

astro-ph.HE2018★ 118 cited

The impact of vector resonant relaxation on the evolution of binaries near a massive black hole: implications for gravitational wave sources

Adrian S. Hamers, Ben Bar-Or, Cristobal Petrovich +1

Binaries within the sphere of influence of a massive black hole (MBH) in galactic nuclei are susceptible to the Lidov-Kozai (LK) mechanism, which can drive orbits to high eccentric…

astro-ph.HE2017★ 91 cited

Precessional dynamics of black hole triples: binary mergers with near-zero effective spin

Fabio Antonini, Carl L. Rodriguez, Cristobal Petrovich +1

The binary black hole mergers detected by Advanced LIGO/Virgo have shown no evidence of large black hole spins. However, because LIGO/Virgo best measures the effective combination…

astro-ph.HE2017★ 181 cited

Greatly enhanced merger rates of compact-object binaries in non-spherical nuclear star clusters

Cristobal Petrovich, Fabio Antonini

The Milky Way and a significant fraction of galaxies are observed to host a central Massive Black Hole (MBH) embedded in a non-spherical nuclear star cluster. We study the secular…

astro-ph.HE2010★ 9 cited

Long-period thermal oscillations in superfluid millisecond pulsars

Cristobal Petrovich, Andreas Reisenegger

In previous papers, we have shown that, as the rotation of a neutron star slows down, it will be internally heated as a consequence of the progressively changing mix of particles (…

astro-ph.HE2010

Rotochemical heating with a density-dependent superfluid energy gap in neutron stars

Nicolás González-Jiménez, Cristóbal Petrovich, Andreas Reisenegger

When a rotating neutron star loses angular momentum, the reduction of the centrifugal force makes it contract. This perturbs each fluid element, raising the local pressure and orig…

astro-ph.HE2010

Rotochemical heating in millisecond pulsars with Cooper pairing

Cristobal Petrovich, Andreas Reisenegger

When a rotating neutron star loses angular momentum, the reduction in the centrifugal force makes it contract. This perturbs each fluid element, raising the local pressure and orig…

astro-ph.HE2009★ 34 cited

Rotochemical heating in millisecond pulsars: modified Urca reactions with uniform Cooper pairing gaps

Cristobal Petrovich, Andreas Reisenegger

Context: When a rotating neutron star loses angular momentum, the reduction in the centrifugal force makes it contract. This perturbs each fluid element, raising the local pressure…