activity
20162026
most citedPost-Newtonian dynamical modeling of supermassive black holes in galactic-scale simulations

79 citations · 820 across the 41 of their papers we have counts for

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Showing 2024Show all

9 papers · 1 filter

astro-ph.GA2024

MAGICS II. Seed black holes stripped of their surrounding stars do not sink

Yihao Zhou, Diptajyoti Mukherjee, Nianyi Chen +7

MBH seed mergers are expected to be among the loudest sources of gravitational waves detected by the Laser Interferometer Space Antenna (LISA), providing a unique window into the b…

astro-ph.GA2024★ 9 cited

Identifying supermassive black hole recoil in elliptical galaxies

Alexander Rawlings, Atte Keitaanranta, Max Mattero +8

We study stellar core growth in simulations of merging massive () elliptical galaxies by a supermassive black hole (SMBH) displaced by gravitatio…

astro-ph.GA2024★ 14 cited

The formation, evolution and disruption of star clusters with improved gravitational dynamics in simulated dwarf galaxies

Natalia Lahén, Antti Rantala, Thorsten Naab +3

So far, even the highest resolution galaxy formation simulations with gravitational softening have failed to reproduce realistic life cycles of star clusters. We present the first…

astro-ph.CO2024★ 17 cited

Structure formation with primordial black holes: collisional dynamics, binaries, and gravitational waves

M. Sten Delos, Antti Rantala, Sam Young +1

Primordial black holes (PBHs) could compose the dark matter content of the Universe. We present the first simulations of cosmological structure formation with PBH dark matter that…

astro-ph.GA2024

The importance of nuclear star clusters for massive black hole growth and nuclear star formation in simulated low-mass galaxies

Christian Partmann, Thorsten Naab, Natalia Lahén +5

Observed low-mass galaxies with nuclear star clusters (NSCs) can host accreting massive black holes (MBH). We present simulations of dwarf galaxies ($M_{\mathrm{baryon}} \sim 0.6 -…

astro-ph.GA2024★ 12 cited

The supermassive black hole merger driven evolution of high-redshift red nuggets into present-day cored early-type galaxies

Antti Rantala, Alexander Rawlings, Thorsten Naab +2

Very compact ( kpc) massive quiescent galaxies (red nuggets) are more abundant in the high-redshift Universe (-) than today. Their size evolution…