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Takashi Nakamura

8 papers hereh-index 448.3k citations515 works total

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

author position
  • sole author1
  • first author2
  • middle author4
  • last author1

Across the 8 of 8 papers where every author was matched, so the position is known.

fields
  • astro-ph4
  • astro-ph.HE1
  • gr-qc1
  • hep-ph1
  • nucl-th1
same name
  • Takashi Nakamura — 12 papers, h 83
  • Takashi Nakamura — 7 papers, h 23
  • Takashi Nakamura — 5 papers
  • Takashi Nakamura — 3 papers, h 17
  • Takashi Nakamura — 2 papers
  • Takashi Nakamura — 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
19982010
most citedExotic Quark Structure of Lambda(1405) in QCD Sum Rule

9 citations · 14 across the 4 of their papers we have counts for

collaborators
Showing astro-phShow all

4 papers · 1 filter

astro-ph2007★ 2 cited

Redshift Dependent Lag-Luminosity Relation in 565 BASTE Gamma Ray Bursts

Ryo Tsutsui, Takashi Nakamura, Daisuke Yonetoku +3

We compared redshifts zY​ from Yonetoku relation and zlag​ from the lag-luminosity relation for 565 BASTE GRBs and were surprised to find that the correlation is very low. As…

astro-ph2005

A Unified Model for Gamma-Ray Bursts

Ryo Yamazaki, Kunihito Ioka, Takashi Nakamura +1

A possible unified model of short and long gamma-ray bursts (GRBs), X-ray rich GRBs, and X-ray flashes is proposed. It is assumed that the jet of a GRB consists of many emitting su…

astro-ph2003

Near-Infrared Colors of Gamma-Ray Burst Afterglows and Cosmic Reionization History

Akio K. Inoue, Ryo Yamazaki, Takashi Nakamura

Using the near-infrared (NIR) observations of the afterglows of the high redshift ($5 \la z \la 25$) gamma-ray bursts (GRBs) which will be detected by the {\it Swift} satellite, we…

astro-ph1998

A Model for Non High Energy Gamma Ray Bursts and Sources of Ultra High Energy Cosmic Rays

Takashi Nakamura

As a progenitor of NHE (Non High Energy) GRBs, we propose a (C+O) star and a neutron star (black hole) close binary system. Since the (C+O) star is tidally locked, a new born pulsa…

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