activity
20052021
most citedSelf-interaction spin effects in inspiralling compact binaries

142 citations · 298 across the 13 of their papers we have counts for

collaborators

13 papers

gr-qc2021★ 1 cited

Spin precession of binary neutron stars with magnetic dipole moments

Balázs Mikóczi

Spin precession equations including the spin-orbit (SO), spin-spin (SS), quadrupole-monopole (QM) and magnetic dipole-magnetic dipole (DD) leading-order interactions are derived fo…

gr-qc2016★ 32 cited

Spin supplementary conditions for spinning compact binaries

Balázs Mikóczi

We consider different spin supplementary conditions (SSC) for a spinning compact binary with the leading-order spin-orbit (SO) interaction. The Lagrangian of the binary system can…

gr-qc2015★ 17 cited

Eccentric first post-Newtonian waveforms for compact binaries in frequency domain with Hansen coefficients

Balázs Mikóczi, Péter Forgács, Mátyás Vasúth

The inspiral and merger of supermassive black hole binary systems with high orbital eccentricity are among the promising sources of the advanced gravitational wave observatories. I…

gr-qc2012★ 51 cited

Parameter estimation for inspiraling eccentric compact binaries including pericenter precession

Balázs Mikóczi, Bence Kocsis, Péter Forgács +1

Inspiraling supermassive black hole binary systems with high orbital eccentricity are important sources for space-based gravitational wave (GW) observatories like the Laser Interfe…

gr-qc2009★ 5 cited

Secular momentum transport by gravitational waves from spinning compact binaries

Zoltán Keresztes, Balázs Mikóczi, László Á. Gergely +1

We present a closed system of coupled first order differential equations governing the secular linear momentum loss of a compact binary due to emitted gravitational waves, with the…

gr-qc2009★ 1 cited

Renormalized spin coefficients in the accumulated orbital phase for unequal mass black hole binaries

László Á. Gergely, Peter L. Biermann, Balázs Mikóczi +1

We analyze galactic black hole mergers and their emitted gravitational waves. Such mergers have typically unequal masses with mass ratio of the order 1/10. The emitted gravitationa…