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researcher

B. K. Sharma

4 papers hereh-index 2150 citations10 works total

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

author position
  • first author1
  • middle author2
  • last author1

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

fields
  • nucl-th3
  • astro-ph.HE1
same name
  • B. K. Sharma — 10 papers, h 11
  • B. K. Sharma — 1 paper, h 13
  • B. K. Sharma — 1 paper, h 6
  • B. K. Sharma — 1 paper, h 2
  • B. K. Sharma — 1 paper, h 11

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
20152026
most citedUnified equation of state for neutron stars on a microscopic basis

160 citations · 177 across the 4 of their papers we have counts for

collaborators

4 papers

nucl-th2026

Radial oscillations of pulsating neutron stars: The UCIa equation-of-state case

G. Panotopoulos, A. Övgün, T. Iqbal +2

Radial oscillations provide a clean dynamical test of the high-density stiffness of neutron-star equations of state. We study spherically symmetric pulsations of nonrotating relati…

astro-ph.HE2025

Implications of σ-cut potential on Antikaon condensates in neutron stars

Prashant Thakur, Yashmitha Kumaran, Lakshana Sudarsan +3

We investigate the properties of neutron stars with antikaon condensation in the framework of the Relativistic Mean-Field (RMF) model with a σ-cut potential. The well-known RMF m…

nucl-th2024★ 17 cited

Feasibility of dark matter admixed neutron star based on recent observational constraints

Prashant Thakur, Tuhin Malik, Arpan Das +3

The equation of state (EOS) for neutron stars is modeled using the Relativistic Mean Field (RMF) approach with a mesonic nonlinear (NL) interaction, a modified sigma cut potential…

nucl-th2015★ 160 cited

Unified equation of state for neutron stars on a microscopic basis

B. K. Sharma, M. Centelles, X. Vinas +2

We derive a new equation of state (EoS) for neutron stars (NS) from the outer crust to the core based on modern microscopic Brueckner-Hartree-Fock (BHF) calculations using the Argo…

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