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D. Misra

16 papers hereh-index 11391 citations20 works total

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

author position
  • first author3
  • middle author13

Across the 16 of 16 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE12
  • astro-ph.SR3
  • astro-ph.GA1
same name
  • D. Misra — 6 papers, h 8
  • D. Misra — 6 papers, h 3
  • D. Misra — 2 papers, h 17
  • D. Misra — 1 paper, h 32
  • D. Misra — 1 paper, h 0
  • D. Misra — 1 paper, h 1

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

activity
20202025
most citedThe impact of mass-transfer physics on the observable properties of field binary black hole populations

156 citations · 558 across the 16 of their papers we have counts for

collaborators
Showing 2020Show all

3 papers · 1 filter

astro-ph.HE2020★ 35 cited

The role of core-collapse physics in the observability of black-hole neutron-star mergers as multi-messenger sources

Jaime Román-Garza, Simone S. Bavera, Tassos Fragos +10

Recent detailed 1D core-collapse simulations have brought new insights on the final fate of massive stars, which are in contrast to commonly used parametric prescriptions. In this…

astro-ph.HE2020★ 156 cited

The impact of mass-transfer physics on the observable properties of field binary black hole populations

Simone S. Bavera, Tassos Fragos, Michael Zevin +13

We study the impact of mass-transfer physics on the observable properties of binary black hole populations formed through isolated binary evolution. We investigate the impact of ma…

astro-ph.HE2020★ 56 cited

The origin of pulsating ultra-luminous X-ray sources: Low- and intermediate-mass X-ray binaries containing neutron star accretors

Devina Misra, Tassos Fragos, Thomas Tauris +2

Ultra-luminous X-ray sources (ULXs) are those X-ray sources located away from the centre of their host galaxy with luminosities exceeding the Eddington limit of a stellar-mass blac…

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