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Debanjan Sengupta

3 papers here

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

author position
  • first author1
  • middle author2

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

fields
  • astro-ph.EP3
ORCID 0000-0003-0801-3159
same name
  • Debanjan Sengupta — 2 papers, h 4

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 citedA solution for the density dichotomy problem of Kuiper Belt objects with multi-species streaming instability and pebble accretion

1 citations · 1 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.EP2024

Magnetically Driven Turbulence in the Inner Regions of Protoplanetary Disks

David G. Rea, Jacob B. Simon, Daniel Carrera +5

Given the important role turbulence plays in the settling and growth of dust grains in protoplanetary disks, it is crucial that we determine whether these disks are turbulent and t…

astro-ph.EP2024

Length and Velocity Scales in Protoplanetary Disk Turbulence

Debanjan Sengupta, Jeffrey N. Cuzzi, Orkan M. Umurhan +1

In the theory of protoplanetary disk turbulence, a widely adopted \emph{ansatz}, or assumption, is that the turnover frequency of the largest turbulent eddy, ΩL​, is the local Ke…

astro-ph.EP2024★ 1 cited

A solution for the density dichotomy problem of Kuiper Belt objects with multi-species streaming instability and pebble accretion

Manuel H. Cañas, Wladimir Lyra, Daniel Carrera +6

Kuiper belt objects show an unexpected trend, whereby large bodies have increasingly higher densities, up to five times greater than their smaller counterparts. Current explanation…

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