Author

Kajino, Toshitaka

INSPIRE profile1003907 ORCID0000-0002-8619-359X

59 papers·1,858 citations in this corpus

	Paper	Category
Dec 29, 2010#10*1012.5701	Reanalysis of the (J = 5) state at 592 keV in 180Ta and its role in the neutrino-process nucleosynthesis of 180Ta in supernovae T. Hayakawa🇯🇵 · P. Mohr🇩🇪 · T. Kajino🇯🇵 · S. Chiba🇯🇵 · G. J. Mathews🇺🇸	↳ astro-ph.HE	PRC	19
Sep 17, 2010#8*1009.3082	Neutrino reactions via neutral and charged current by Quasi-particle Random Phase Approximation(QRPA) Myung-Ki Cheoun🇰🇷 · Eunja Ha🇰🇷 · K. S. Kim🇰🇷 · Toshitaka Kajino🇯🇵	↳ astro-ph.HE	J.Phys.G	39
Aug 28, 2006#2*nucl-th/0608056	Neutrino Nucleus Reactions based on New Shell Model Hamiltonians Toshio Suzuki🇯🇵 · Satoshi Chiba🇯🇵 · Takashi Yoshida🇯🇵 · Toshitaka Kajino🇯🇵 · Takaharu Otsuka🇯🇵	nucl-th	PRC	101
Sep 17, 2004#2*astro-ph/0409395	Evidence for nucleosynthesis in supernova $γ$ -process: Universal scaling on p-nuclei T.Hayakawa🇯🇵 · N.Iwamoto🇯🇵 · T.Shizuma🇯🇵 · T.Kajino🇯🇵 · H.Umeda🇯🇵 · K. Nomoto🇯🇵	↳ astro-ph	PRL	49
Oct 22, 2002#2*nucl-th/0210059	Astrophysical reaction rate for $α (α n, γ)$ $^{9}$ Be by photodisintegration K. Sumiyoshi (1)🇯🇵 · H. Utsunomiya (2)🇯🇵 · S. Goko (2)🇯🇵 · T. Kajino (3) ((1) Numazu Coll. Tech. (2) Konan Univ. (3) NAO)🇯🇵	nucl-th	NPA	41
Jun 20, 2002#13*astro-ph/0206322	R-Process Nucleosynthesis In Neutrino-Driven Winds From A Typical Neutron Star With M = 1.4 Msun M. Terasawa🇯🇵 · K. Sumiyoshi🇯🇵 · S. Yamada🇯🇵 · H. Suzuki🇯🇵 · T. Kajino🇯🇵	↳ astro-ph	ApJL	31
Jul 20, 2001#4*astro-ph/0107368	New Nuclear Reaction Flow during r-Process Nucleosynthesis in Supernovae: Critical Role of Light Neutron-Rich Nuclei M. Terasawa🇯🇵 · K. Sumiyoshi🇯🇵 · T. Kajino🇯🇵 · G. J. Mathews🇺🇸 · I. Tanihata🇯🇵	↳ astro-ph	ApJ	135
May 24, 2000#3*astro-ph/0005446	Neutrino Degeneracy and Decoupling: New Limits from Primordial Nucleosynthesis and the Cosmic Microwave Background M. Orito🇯🇵 · T. Kajino🇯🇵 · G. J. Mathews🇯🇵 · R. N. Boyd🇺🇸	↳ astro-ph	—	43
Sep 20, 1996#1*nucl-th/9609041	Reaction Rates of neutron capture by Li- and Be-isotopes H. Herndl🇦🇹 · R. Hofinger🇦🇹 · P. Mohr🇦🇹 · H. Oberhummer🇦🇹 · T. Kajino🇯🇵 · N. Terasawa🇯🇵	nucl-th	—	1

Reanalysis of the (J = 5) state at 592 keV in 180Ta and its role in the neutrino-process nucleosynthesis of 180Ta in supernovae
T. Hayakawa🇯🇵 · P. Mohr🇩🇪 · T. Kajino🇯🇵 · S. Chiba🇯🇵 · G. J. Mathews🇺🇸
Dec 29, 2010#10*↳ astro-ph.HEPRC19 citations
Neutrino reactions via neutral and charged current by Quasi-particle Random Phase Approximation(QRPA)
Myung-Ki Cheoun🇰🇷 · Eunja Ha🇰🇷 · K. S. Kim🇰🇷 · Toshitaka Kajino🇯🇵
Sep 17, 2010#8*↳ astro-ph.HEJ.Phys.G39 citations
Neutrino Nucleus Reactions based on New Shell Model Hamiltonians
Toshio Suzuki🇯🇵 · Satoshi Chiba🇯🇵 · Takashi Yoshida🇯🇵 · Toshitaka Kajino🇯🇵 · Takaharu Otsuka🇯🇵
Aug 28, 2006#2*nucl-thPRC101 citations
Evidence for nucleosynthesis in supernova $γ$ -process: Universal scaling on p-nuclei
T.Hayakawa🇯🇵 · N.Iwamoto🇯🇵 · T.Shizuma🇯🇵 · T.Kajino🇯🇵 · H.Umeda🇯🇵 · K. Nomoto🇯🇵
Sep 17, 2004#2*↳ astro-phPRL49 citations
Astrophysical reaction rate for $α (α n, γ)$ $^{9}$ Be by photodisintegration
K. Sumiyoshi (1)🇯🇵 · H. Utsunomiya (2)🇯🇵 · S. Goko (2)🇯🇵 · T. Kajino (3) ((1) Numazu Coll. Tech. (2) Konan Univ. (3) NAO)🇯🇵
Oct 22, 2002#2*nucl-thNPA41 citations
R-Process Nucleosynthesis In Neutrino-Driven Winds From A Typical Neutron Star With M = 1.4 Msun
M. Terasawa🇯🇵 · K. Sumiyoshi🇯🇵 · S. Yamada🇯🇵 · H. Suzuki🇯🇵 · T. Kajino🇯🇵
Jun 20, 2002#13*↳ astro-phApJL31 citations
New Nuclear Reaction Flow during r-Process Nucleosynthesis in Supernovae: Critical Role of Light Neutron-Rich Nuclei
M. Terasawa🇯🇵 · K. Sumiyoshi🇯🇵 · T. Kajino🇯🇵 · G. J. Mathews🇺🇸 · I. Tanihata🇯🇵
Jul 20, 2001#4*↳ astro-phApJ135 citations
Neutrino Degeneracy and Decoupling: New Limits from Primordial Nucleosynthesis and the Cosmic Microwave Background
M. Orito🇯🇵 · T. Kajino🇯🇵 · G. J. Mathews🇯🇵 · R. N. Boyd🇺🇸
May 24, 2000#3*↳ astro-ph43 citations
Reaction Rates of neutron capture by Li- and Be-isotopes
H. Herndl🇦🇹 · R. Hofinger🇦🇹 · P. Mohr🇦🇹 · H. Oberhummer🇦🇹 · T. Kajino🇯🇵 · N. Terasawa🇯🇵
Sep 20, 1996#1*nucl-th1 citation

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