M. Hashimoto

877 total citations
30 papers, 585 citations indexed

About

M. Hashimoto is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Geophysics. According to data from OpenAlex, M. Hashimoto has authored 30 papers receiving a total of 585 indexed citations (citations by other indexed papers that have themselves been cited), including 28 papers in Astronomy and Astrophysics, 12 papers in Nuclear and High Energy Physics and 6 papers in Geophysics. Recurrent topics in M. Hashimoto's work include Gamma-ray bursts and supernovae (16 papers), Astrophysical Phenomena and Observations (9 papers) and Pulsars and Gravitational Waves Research (8 papers). M. Hashimoto is often cited by papers focused on Gamma-ray bursts and supernovae (16 papers), Astrophysical Phenomena and Observations (9 papers) and Pulsars and Gravitational Waves Research (8 papers). M. Hashimoto collaborates with scholars based in Japan, United States and Canada. M. Hashimoto's co-authors include K. Nomoto, Nikos Prantzos, K. Nomoto, M. Rayet, M. Arnould, F.‐K. Thielemann, K. Arai, M. Ono, Toshikazu Shigeyama and D. Sugimoto and has published in prestigious journals such as Nature, Physical Review Letters and The Astrophysical Journal.

In The Last Decade

M. Hashimoto

30 papers receiving 568 citations

Peers — A (Enhanced Table)

Peers by citation overlap · career bar shows stage (early→late) cites · hero ref

Name h Career Trend Papers Cites
M. Hashimoto Japan 12 470 325 53 42 39 30 585
K. Nomoto Japan 18 763 1.6× 420 1.3× 54 1.0× 58 1.4× 31 0.8× 35 897
M. F. El Eid Lebanon 12 454 1.0× 272 0.8× 39 0.7× 29 0.7× 36 0.9× 38 542
D. K. Nadyozhin Russia 16 799 1.7× 475 1.5× 13 0.2× 31 0.7× 43 1.1× 54 914
Stéphane Schanne France 4 407 0.9× 314 1.0× 32 0.6× 82 2.0× 11 0.3× 11 553
K. Farouqi Germany 14 677 1.4× 481 1.5× 77 1.5× 46 1.1× 47 1.2× 32 837
M. Jaeger Germany 7 252 0.5× 385 1.2× 112 2.1× 165 3.9× 16 0.4× 11 537
L. Piersanti Italy 15 959 2.0× 285 0.9× 29 0.5× 40 1.0× 65 1.7× 41 1.0k
V. E. Barnard United States 9 457 1.0× 290 0.9× 61 1.2× 80 1.9× 89 2.3× 10 620
Marius Eichler Germany 8 370 0.8× 310 1.0× 39 0.7× 22 0.5× 22 0.6× 13 505
Oliver Just Germany 18 967 2.1× 619 1.9× 19 0.4× 16 0.4× 49 1.3× 29 1.2k

Countries citing papers authored by M. Hashimoto

Since Specialization
Citations

This map shows the geographic impact of M. Hashimoto's research. It shows the number of citations coming from papers published by authors working in each country. You can also color the map by specialization and compare the number of citations received by M. Hashimoto with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites M. Hashimoto more than expected).

Fields of papers citing papers by M. Hashimoto

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by M. Hashimoto. Nodes represent research fields, and links connect fields that are likely to share authors. Colored nodes show fields that tend to cite the papers produced by M. Hashimoto. The network helps show where M. Hashimoto may publish in the future.

Co-authorship network of co-authors of M. Hashimoto

This figure shows the co-authorship network connecting the top 25 collaborators of M. Hashimoto. A scholar is included among the top collaborators of M. Hashimoto based on the total number of citations received by their joint publications. Widths of edges represent the number of papers authors have co-authored together. Node borders signify the number of papers an author published with M. Hashimoto. M. Hashimoto is excluded from the visualization to improve readability, since they are connected to all nodes in the network.

All Works

20 of 20 papers shown
1.
Kase, Ryotaro, et al.. (2021). Neutron star cooling in modified gravity theories. Progress of Theoretical and Experimental Physics. 2021(9). 7 indexed citations
2.
Hayakawa, Takehito, Myung-Ki Cheoun, Motohiko Kusakabe, et al.. (2018). Short-Lived Radioisotope Tc98 Synthesized by the Supernova Neutrino Process. Physical Review Letters. 121(10). 102701–102701. 15 indexed citations
3.
Liu, Helei, et al.. (2018). Quiescent luminosities of accreting neutron stars-possibility of neutrino losses due to strong pion condensations. International Journal of Modern Physics E. 27(8). 1850067–1850067. 9 indexed citations
4.
Ono, M., Shigehiro Nagataki, M. Hashimoto, et al.. (2015). MATTER MIXING IN CORE-COLLAPSE SUPERNOVA EJECTA: LARGE DENSITY PERTURBATIONS IN THE PROGENITOR STAR?. The Astrophysical Journal. 808(2). 164–164. 11 indexed citations
5.
Ono, M., Shigehiro Nagataki, Hirotaka Ito, et al.. (2013). MATTER MIXING IN ASPHERICAL CORE-COLLAPSE SUPERNOVAE: A SEARCH FOR POSSIBLE CONDITIONS FOR CONVEYING56Ni INTO HIGH VELOCITY REGIONS. The Astrophysical Journal. 773(2). 161–161. 24 indexed citations
6.
Ono, M., et al.. (2012). Effects of a New Triple-α Reaction on the s-Process in Massive Stars. Progress of Theoretical Physics. 127(1). 171–178. 3 indexed citations
7.
Kotake, Kei, et al.. (2011). EXPLOSIVE NUCLEOSYNTHESIS IN THE NEUTRINO-DRIVEN ASPHERICAL SUPERNOVA EXPLOSION OF A NON-ROTATING 15M☉STAR WITH SOLAR METALLICITY. The Astrophysical Journal. 738(1). 61–61. 13 indexed citations
8.
Hashimoto, M., et al.. (2008). Cosmic microwave background constraints on a decaying cosmological term related to the thermal evolution. Physical review. D. Particles, fields, gravitation, and cosmology. 77(12). 1 indexed citations
9.
Yasutake, Nobutoshi, Kei Kotake, M. Hashimoto, & Shoichi Yamada. (2007). Effects of QCD phase transition on gravitational radiation from two-dimensional collapse and bounce of massive stars. Physical review. D. Particles, fields, gravitation, and cosmology. 75(8). 15 indexed citations
10.
Hashimoto, M., et al.. (2004). Nucleosynthesis inside an Accretion Disk in a Type II Collapsar. Publications of the Astronomical Society of Japan. 56(2). 407–414. 5 indexed citations
11.
Hashimoto, M., et al.. (2003). P-process nucleosynthesis inside supernova-driven supercritical accretion disks. Nuclear Physics A. 718. 611–613. 2 indexed citations
12.
Arai, K., et al.. (2003). Nucleosynthesis inside accretion disks around intermediate—mass black holes. Nuclear Physics A. 718. 572–574. 1 indexed citations
13.
Yoshida, Takashi, M. Hashimoto, & H. Yamaoka. (2001). Neutrino nucleosynthesis of Li and B through type II supernova explosions for population III stars. Nuclear Physics A. 688(1-2). 436–438. 1 indexed citations
14.
Nomoto, K. & M. Hashimoto. (1997). 1 NUCLEOSYNTHESIS IN TYPE II SUPERNOVAE. 162 indexed citations
15.
Wanajo, Shinya, K. Nomoto, M. Hashimoto, Toshitaka Kajino, & S. Kubono. (1997). Explosive nucleosynthesis in ONeMg novae. Nuclear Physics A. 616(1-2). 91–96. 4 indexed citations
16.
Wanajo, Shinya, K. Nomoto, M. Hashimoto, & J. W. Truran. (1997). A quasi-analytic study of nucleosynthesis in ONeMg novae. Nuclear Physics A. 621(1-2). 499–502. 2 indexed citations
17.
Arai, K. & M. Hashimoto. (1995). Accretion disk models with hydrogen burning around a black hole.. 302. 99. 1 indexed citations
18.
Tsujimoto, Takuji, K. Nomoto, M. Hashimoto, Shintarou Yanagida, & F.‐K. Thielemann. (1993). Relative frequencies of type Ia and type II supernovae in the Galaxy LMC, and SMC. 581–586. 1 indexed citations
19.
Hashimoto, M., Yoshiharu Eriguchi, K. Arai, & E. Müeller. (1993). Self-gravitating and rotating hot toroids. 268(1). 131–136. 3 indexed citations
20.
Prantzos, Nikos, M. Hashimoto, & K. Nomoto. (1990). The s-process in massive stars : yields as a function of stellar mass and metallicity. 234. 211–229. 22 indexed citations

Rankless uses publication and citation data sourced from OpenAlex, an open and comprehensive bibliographic database. While OpenAlex provides broad and valuable coverage of the global research landscape, it—like all bibliographic datasets—has inherent limitations. These include incomplete records, variations in author disambiguation, differences in journal indexing, and delays in data updates. As a result, some metrics and network relationships displayed in Rankless may not fully capture the entirety of a scholar's output or impact.

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