◍wovepaper
SearchResearchersInstitutions
Sign in
researcher

R. Prasad

4 papers hereh-index 8173 citations28 works total

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

author position
  • first author2
  • middle author1
  • last author1

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

fields
  • astro-ph.HE4
same name
  • R. Prasad — 13 papers, h 6
  • R. Prasad — 11 papers, h 20
  • R. Prasad — 5 papers, h 4
  • R. Prasad — 4 papers, h 5
  • R. Prasad — 4 papers, h 2
  • R. Prasad — 3 papers, h 25

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
20172021
most citedMultimessenger signal from phase transition of neutron star to quark star

7 citations · 7 across the 2 of their papers we have counts for

collaborators

4 papers

astro-ph.HE2021★ 7 cited

Multimessenger signal from phase transition of neutron star to quark star

Debojoti Kuzur, Ritam Mallick, Prasad R +1

Aim: To study the multimessenger nature of the signal that can result from the phase transition of a neutron star to a quark star and their corresponding astrophysical observations…

astro-ph.HE2020

Gravitational wave signature from phase transition of a combusting neutron star to quark star

Ritam Mallick, Shailendra Singh, R Prasad

Fluctuation at the neutron star center gives rise to a small deconfined quark core very close to the star center. The density discontinuity at the quark-hadron boundary initiates a…

astro-ph.HE2019

Gravitational waves from phase transition of NS to QS

Prasad R, Ritam Mallick

In this article, we perform a 2-d simulation of combustion of neutron star (NS) to hybrid star (HS). We assume that a sudden density fluctuation at the center of the NS initiates a…

astro-ph.HE2017

Dynamical phase transition in neutron stars

R Prasad, Ritam Mallick

In this work, we have studied the dynamical evolution of the shock front in a neutron star. The shock wave is expected to possess enough strength to ignite the nuclear matter there…

◍wovepaper

Papers, researchers and institutions, woven together.

Explore
  • Search
  • Researchers
  • Institutions
Account
  • Library
  • Chat
Data
  • arXiv.org
  • Semantic Scholar
  • OpenAlex
  • Latest RSS
AboutContactPrivacyDevelopersllms.txtopenapi.json
Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.