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S. D. Mink

4 papers hereh-index 131.2k citations26 works total

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

author position
  • middle author1
  • last author1

Across the 2 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR3
  • astro-ph.HE1
same name
  • S. D. Mink — 47 papers, h 53
  • S. D. Mink — 3 papers, h 1
  • S. D. Mink — 1 paper, h 3

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

most citedSensitivity of the lower-edge of the pair instability black hole mass gap to the treatment of time dependent convection

89 citations · 195 across the 4 of their papers we have counts for

collaborators

3 papers

astro-ph.HE2025★ 9 cited

A fundamental limit to how close binary systems can get via stable mass transfer shapes the properties of binary black hole mergers

Jakub Klencki, Philipp Podsiadlowski, Norbert Langer +4

Mass transfer in binary systems is the key process in the formation of various classes of objects, including merging binary black holes (BBHs) and neutron stars. Orbital evolution…

astro-ph.SR2025★ 8 cited

Binary mass transfer in 3D: Mass Transfer Rate and Morphology

T. Ryu, R. Sari, S. E. de Mink +6

Mass transfer is crucial in binary evolution, yet its theoretical treatment has long relied on analytic models whose key assumptions remain debated. We present a direct and systema…

astro-ph.SR2020★ 89 cited

Sensitivity of the lower-edge of the pair instability black hole mass gap to the treatment of time dependent convection

M. Renzo, R. J. Farmer, S. Justham +3

Gravitational-wave detections are now probing the black hole (BH) mass distribution, including the predicted pair-instability mass gap. These data require robust quantitative predi…

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