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Aklant K. Bhowmick

3 papers here

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author2
  • middle author1

Across the 3 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA3
ORCID 0000-0002-7080-2864

identity via Semantic Scholar / OpenAlex

most citedRepresenting low mass black hole seeds in cosmological simulations: A new sub-grid stochastic seed model

2 citations · 4 across the 3 of their papers we have counts for

collaborators

3 papers

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 ∼102−106 M⊙​. However, the lowest mass seeds (≲103M⊙​) are inaccessible to most cosm…

astro-ph.GA2023★ 2 cited

Representing low mass black hole seeds in cosmological simulations: A new sub-grid stochastic seed model

Aklant K Bhowmick, Laura Blecha, Paul Torrey +5

The nature of the first seeds of supermassive black holes (SMBHs) is currently unknown, with postulated initial masses ranging from ∼105 M⊙​ to as low as $\sim10^2~M_{\…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.