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researcher

P. Jaikumar

64 papers hereh-index 18955 citations100 works total

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

author position
  • sole author2
  • first author22
  • middle author8
  • last author28

Across the 60 of 64 papers where every author was matched, so the position is known.

fields
  • nucl-th20
  • hep-ph16
  • astro-ph10
  • astro-ph.HE9
  • gr-qc3
  • hep-th2
same name
  • P. Jaikumar — 1 paper, h 1
  • P. Jaikumar — 1 paper, h 2

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
20002026
most citedThe Strange Star Surface: A Crust with Nuggets

127 citations · 1.3k across the 64 of their papers we have counts for

collaborators
Showing 2006Show all

4 papers · 1 filter

nucl-th2006★ 44 cited

Nucleosynthesis in neutron-rich ejecta from quark-novae

Prashanth Jaikumar, Bradley S. Meyer, Kaori Otsuki +1

We explore heavy-element nucleosynthesis by rapid neutron capture (r-process) in the decompressing ejecta from the surface of a neutron star. The decompression is triggered by a vi…

astro-ph2006★ 8 cited

Quark Matter in Neutron Stars: An apercu

Prashanth Jaikumar, Sanjay Reddy, Andrew W. Steiner

The existence of deconfined quark matter in the superdense interior of neutron stars is a key question that has drawn considerable attention over the past few decades. Quark matter…

hep-ph2006★ 1 cited

Surface structure of Quark stars with magnetic fields

Prashanth Jaikumar

We investigate the impact of magnetic fields on the electron distribution in the electrosphere of quark stars. For moderately strong magnetic fields B∼1013G, quantization…

astro-ph2006★ 48 cited

Quark deconfinement in neutron star cores: The effects of spin-down

Jan Staff, Rachid Ouyed, Prashanth Jaikumar

We study the role of spin-down in driving quark deconfinement in the high density core of isolated neutron stars. Assuming spin-down to be solely due to magnetic braking, we obtain…

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