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researcher

R. Moradi

50 papers hereh-index 15615 citations83 works total

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

author position
  • first author7
  • middle author36
  • last author3

Across the 46 of 50 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE42
  • gr-qc5
  • astro-ph.IM3
same name
  • R. Moradi — 13 papers, h 4
  • R. Moradi — 3 papers, h 2
  • R. Moradi — 2 papers, h 16
  • R. Moradi — 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
20132026
most citedOn the classification of GRBs and their occurrence rates

76 citations · 723 across the 50 of their papers we have counts for

collaborators
Showing 2021Show all

4 papers · 1 filter

astro-ph.HE2021★ 22 cited

Nature of the ultrarelativistic prompt emission phase of GRB 190114C

R. Moradi, J. A. Rueda, R. Ruffini +7

We address the physical origin of the ultrarelativistic prompt emission (UPE) phase of GRB 190114C observed in the interval 1.9-3.99 s, by the Fermi-GBM in 10 keV-10 MeV . Thanks t…

gr-qc2021★ 15 cited

Is the remnant of GW190425 a strange quark star?

J. Sedaghat, S. M. Zebarjad, G. H. Bordbar +2

This study investigates the effects of different QCD models on the structure of strange quark stars (SQS). In these models, the running coupling constant has a finite value in the…

astro-ph.HE2021★ 1 cited

X-ray and GeV afterglows and sub-TeV emission of GRB 180720B

R. Moradi, Liang Li, J. A. Rueda +3

GRB 180720B, observed by {\it Fermi}-GBM, with redshift z=0.653, isotropic energy Eiso​=5.92×1053 erg, and X-ray afterglow observed by the XRT onboard the Neil G…

astro-ph.HE2021★ 24 cited

The morphology of the X-ray afterglows and of the jetted GeV emission in long GRBs

R. Ruffini, R. Moradi, J. A. Rueda +14

We recall evidence that long gamma-ray bursts (GRBs) have binary progenitors and give new examples. Binary-driven hypernovae (BdHNe) consist of a carbon-oxygen core (CO$_{\rm core}…

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