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researcher

A. Panday

7 papers hereh-index 6168 citations14 works total

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

author position
  • middle author1

Across the 1 of 7 papers where every author was matched, so the position is known.

fields
  • nucl-ex4
  • hep-ex2
  • nucl-th1
same name
  • A. Panday — 3 papers, h 1
  • A. Panday — 1 paper, h 0
  • A. Panday — 1 paper, h 1
  • A. Panday — 1 paper, h 0
  • A. Panday — 1 paper, h 0
  • A. Panday — 1 paper, h 1

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
20242026
most citedMeasuring spin correlation between quarks during QCD confinement

14 citations · 14 across the 2 of their papers we have counts for

collaborators
Showing nucl-exShow all

4 papers · 1 filter

nucl-ex2025

Onset of Constituent Quark Number Scaling in Heavy-Ion Collisions at RHIC

STAR Collaboration, B. E. Aboona, J. Adam +355

Partonic collectivity is one of the necessary signatures for the formation of quark-gluon plasma in high-energy nuclear collisions. Number of constituent quarks (NCQ) scaling has b…

nucl-ex2025

Light Nuclei Femtoscopy and Baryon Interactions in 3 GeV Au+Au Collisions at RHIC

The STAR Collaboration

We report the measurements of proton-deuteron (p-d) and deuteron-deuteron (d-d) correlation functions in Au+Au collisions at sNN​​ = 3 GeV using fixed-targ…

nucl-ex2024

Imaging Shapes of Atomic Nuclei in High-Energy Nuclear Collisions

STAR Collaboration

Atomic nuclei are self-organized, many-body quantum systems bound by strong nuclear forces within femtometer-scale space. These complex systems manifest a variety of shapes, tradit…

nucl-ex2024

Production of Protons and Light Nuclei in Au+Au Collisions at sNN​​ = 3 GeV with the STAR Detector

STAR Collaboration, M. I. Abdulhamid, B. E. Aboona +349

We report the systematic measurement of protons and light nuclei production in Au+Au collisions at sNN​​ = 3 GeV by the STAR experiment at the Relativistic Heavy…

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