activity
20212026
most citedGeneral-relativistic hydrodynamics of non-perfect fluids: 3+1 conservative formulation and application to viscous black-hole accretion

45 citations · 131 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.HE2026

Jet variability in small mass ratio supermassive black hole binaries

Jay V. Kalinani, Manuela Campanelli, Michail Chabanov +4

We present three-dimensional general relativistic magnetohydrodynamic simulations of a precessing supermassive black hole binary with mass ratio q=1/7, embedded in a circumbinary d…

astro-ph.HE2026

Detectability of bulk viscosity effects on post-merger gravitational wave signals from binary neutron star mergers

Zhenyu Zhu, Michail Chabanov, Richard O'Shaughnessy

We investigate bulk viscosity (BV) effects on post-merger gravitational wave (PMGW) signals from binary neutron star (BNS) mergers and their detectability using realistic equation…

astro-ph.HE2026

Magnetic Eruption and Nucleosynthesis in GRνMHD Simulations of Spinning Neutron Star Mergers

Allen Wen, Jay V. Kalinani, Michail Chabanov +3

We present three-dimensional general relativistic magnetohydrodynamics simulations of equal-mass binary neutron star mergers with varied neutron star spin configurations and second…

astro-ph.HE2025★ 3 cited

Long-term impact of the magnetic-field strength on the evolution and electromagnetic emission by neutron-star merger remnants

Jin-Liang Jiang, Harry Ho-Yin Ng, Michail Chabanov +1

Numerical simulations are essential to understand the complex physics accompanying the merger of binary systems of neutron stars. However, these simulations become computationally…

astro-ph.HE2025★ 9 cited

Relativistic gas accretion onto supermassive black Hole binaries from inspiral through merger

Lorenzo Ennoggi, Manuela Campanelli, Yosef Zlochower +8

Accreting supermassive black hole binaries are powerful multimessenger sources emitting both gravitational and EM radiation. Understanding the accretion dynamics of these systems a…

gr-qc2023★ 18 cited

Numerical modelling of bulk viscosity in neutron stars

Michail Chabanov, Luciano Rezzolla

The early post-merger phase of a binary neutron-star coalescence is shaped by characteristic rotational velocities as well as violent density oscillations and offers the possibilit…

gr-qc2023★ 27 cited

Impact of bulk viscosity on the post-merger gravitational-wave signal from merging neutron stars

Michail Chabanov, Luciano Rezzolla

In the violent post-merger of binary neutron-star mergers strong oscillations are present that impact the emitted gravitational-wave (GW) signal. The frequencies, temperatures and…

astro-ph.HE2022★ 29 cited

Crustal magnetic fields do not lead to large magnetic-field amplifications in binary neutron-star mergers

Michail Chabanov, Samuel D. Tootle, Elias R. Most +1

The amplification of magnetic fields plays an important role in explaining numerous astrophysical phenomena associated with binary neutron-star mergers, such as mass ejection and t…

gr-qc2021★ 45 cited

General-relativistic hydrodynamics of non-perfect fluids: 3+1 conservative formulation and application to viscous black-hole accretion

Michail Chabanov, Luciano Rezzolla, Dirk H. Rischke

We consider the relativistic hydrodynamics of non-perfect fluids with the goal of determining a formulation that is suited for numerical integration in special-relativistic and gen…