activity
20162026
most citedThe Effect of Pair-Instability Mass Loss on Black Hole Mergers

382 citations · 909 across the 9 of their papers we have counts for

collaborators

11 papers

gr-qc2026

The Irreversible Depletion of Dark Matter Spikes by Extreme-Mass-Ratio Inspirals

Charlie Sharpe, Yonadav Barry Ginat, Thomas F. M. Spieksma +2

Dense dark matter spikes around massive black holes (MBHs) have been widely predicted to produce gravitational-wave dephasing in extreme-mass-ratio inspirals (EMRIs) that are poten…

astro-ph.HE2026

On the rates of binary star collisions around hypermassive black holes

Megha Sharma, Alexander Heger, Evgeni Grishin +1

Observations of the Milky Way show that galaxies have binary stars in their centres. Using Monte Carlo simulations, we model the population statistics of encounters of such binarie…

astro-ph.HE2026

Are most detected tidal disruption events partial?

Megha Sharma, Daniel J. Price, Alexander Heger +1

During a tidal disruption event (TDE), a star loses mass due to the tidal gravitational forces of the black hole. In a partial tidal disruption event, a stellar remnant is left beh…

astro-ph.IM2026

A benchmark for binary star interaction with a supermassive black hole in general relativity

Megha Sharma, Alexander Heger, Daniel J. Price +4

Most galaxies have supermassive black holes (SMBH) at their centres, surrounded by stars with binary systems also present in this environment. We use two schemes - post-Newtonian (…

astro-ph.HE2026

The deci-Hz gravitational wave signal from the collapse of rotating very massive stars

Bailey Sykes, Jade Powell, Bernhard Müller +1

We calculate the gravitational wave signal from the collapse of a rotating 300 star at the upper end of the pair-instability regime. The large-scale asymmetries that deve…

astro-ph.HE2025★ 3 cited

Crust composition and the Shallow Heat Source in KS 1731-260

R. Jain, E. F. Brown, H. Schatz +11

The presence of a strong shallow heat source of unknown origin in accreting neutron star crusts has been inferred by analyzing X-ray observations of their cooling in quiescence. We…

astro-ph.HE2024★ 11 cited

Neutron star kicks plus rockets as a mechanism for forming wide low-eccentricity neutron star binaries

Ryosuke Hirai, Philipp Podsiadlowski, Alexander Heger +1

Recent neutron star surface observations corroborate a long-standing theory that neutron stars may be accelerated over extended periods after their birth. We analyze how these prol…

astro-ph.HE2024★ 1 cited

Convection and the Core -mode in Proto-Compact Stars -- A detailed analysis

Pia Jakobus, Bernhard Mueller, Alexander Heger

We present a detailed analysis of the dynamics of proto-compact star (PCS) convection and the core -mode in core-collapse supernovae based on general relativistic 2D and…

astro-ph.SR2017★ 272 cited

Supernova Simulations from a 3D Progenitor Model -- Impact of Perturbations and Evolution of Explosion Properties

B. Müller, T. Melson, A. Heger +1

We study the impact of large-scale perturbations from convective shell burning on the core-collapse supernova explosion mechanism using three-dimensional (3D) multi-group neutrino…

astro-ph.HE2016★ 382 cited

The Effect of Pair-Instability Mass Loss on Black Hole Mergers

K. Belczynski, A. Heger, W. Gladysz +9

Mergers of two stellar origin black holes are a prime source of gravitational waves and are under intensive investigations. One crucial ingredient in their modeling has so far been…

astro-ph.SR2016★ 240 cited

A Simple Approach to the Supernova Progenitor-Explosion Connection

B. Müller, A. Heger, D. Liptai +1

We present a new approach to understand the landscape of supernova explosion energies, ejected nickel masses, and neutron star birth masses. In contrast to other recent parametric…