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S. Chowdhury

9 papers hereh-index 449 citations13 works total

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

author position
  • sole author1
  • first author5
  • middle author3

Across the 9 of 9 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR4
  • gr-qc4
  • astro-ph.HE1
same name
  • S. Chowdhury — 33 papers, h 13
  • S. Chowdhury — 24 papers, h 10
  • S. Chowdhury — 20 papers, h 13
  • S. Chowdhury — 18 papers, h 7
  • S. Chowdhury — 17 papers, h 13
  • S. Chowdhury — 15 papers, h 5

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
20182023
most citedModified gravity in the interior of population II stars

18 citations · 67 across the 9 of their papers we have counts for

collaborators
Showing gr-qcShow all

4 papers · 1 filter

gr-qc2023

Anisotropies and modified gravity theories in stellar and substellar objects

Shaswata Chowdhury

In several classes of modified gravity theories, extra degrees of freedom are not completely screened in the interiors of stellar and substellar objects. In such theories, the hydr…

gr-qc2023

Tidal disruption of white dwarfs in a modified gravity theory with SPH

Debojyoti Garain, Pritam Banerjee, Shaswata Chowdhury +1

Low energy imprints of modifications to general relativity are often found in pressure balance equations inside stars. These modifications are then amenable to tests via astrophysi…

gr-qc2022★ 1 cited

Equilibrium of slowly rotating polytropes in modified theories of gravity

Shaswata Chowdhury, Pritam Banerjee, Aneta Wojnar

A general formalism to find the density profile of a slowly rotating stellar object in modified gravity is presented. We derive a generic Lane-Emden equation and its analytical sol…

gr-qc2020★ 18 cited

Modified gravity in the interior of population II stars

Shaswata Chowdhury, Tapobrata Sarkar

We study the effects of a beyond-Horndeski theory of modified gravity in the interior of a population II star. We consider a simple phenomenological model of a 1.1M⊙​ star…

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