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20242026
most citedIntroducing the BRAHMA simulation suite: Signatures of low mass black hole seeding models in cosmological simulations

2 citations · 7 across the 13 of their papers we have counts for

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astro-ph.GA2024★ 1 cited

Signatures of black hole seeding in the local Universe: Predictions from the BRAHMA cosmological simulations

Aklant K Bhowmick, Laura Blecha, Paul Torrey +8

The first "seeds" of supermassive black holes (BHs) continue to be an outstanding puzzle, and it is currently unclear whether the imprints of early seed formation survive today. He…

astro-ph.GA2024★ 2 cited

Growth of high redshift supermassive black holes from heavy seeds in the BRAHMA cosmological simulations: Implications of overmassive black holes

Aklant K Bhowmick, Laura Blecha, Paul Torrey +6

JWST has recently revealed a large population of accreting black holes (BHs) in the early Universe. Even after accounting for possible systematic biases, the high-z $M_*-M_{\rm \rm…

astro-ph.HE2024★ 1 cited

Signatures of Circumbinary Disk Dynamics in Multi-Messenger Population Studies of Massive Black Hole Binaries

Magdalena Siwek, Luke Zoltan Kelley, Lars Hernquist

We investigate the effect of cutting-edge circumbinary disk (CBD) evolution models on massive black hole binary (MBHB) populations and the gravitational wave background (GWB). We s…

astro-ph.GA2024

AGN feedback in isolated galaxies with a SMUGGLE multiphase ISM

Aneesh Sivasankaran, Laura Blecha, Paul Torrey +6

Feedback from active galactic nuclei (AGN) can strongly impact the host galaxies by driving high-velocity winds that impart substantial energy and momentum to the interstellar medi…

astro-ph.GA2024★ 2 cited

Introducing the BRAHMA simulation suite: Signatures of low mass black hole seeding models in cosmological simulations

Aklant K. Bhowmick, Laura Blecha, Paul Torrey +6

The first "seeds" of supermassive black holes (BH) can range from . However, the lowest mass seeds () are inaccessible to most cosm…