姓名:梶野敏贵(外籍,教授,博导)

职称: 教授

邮箱: kajino@buaa.edu.cn

姓名NAME:Toshitaka Kajino

职称ACADEMIC TITLE:教授


 

Email:kajino@buaa.edu.cn

办公地点OFFICE:新主楼H1113

研究方向RESEARCH AREA:粒子物理与原子核物理,理论物理

 

个人简介SELF INTRODUCTION:

梶野敏贵教授2004年被选为美国物理学会成员。在2016被授予为我国外专千人学者,成为澳门新萄京6692 cc-最大平台手机版网址特聘教授,同时于2017年在澳门新萄京6692 cc-最大平台手机版网址成立了国际大爆炸宇宙学与元素起源国际交叉科学研究中心,任主任。他在原创性研究过程中发表了200多篇论文期刊并参加了250多个国际会议。1988年初从东京开始,每两年一届有一个核物理学和天文学在跨学科领域国际年会,名称是“物质起源和星系演化(omeg)”,他是这个会议的主导者。

担任过物理学与开放核与粒子物理杂志的各种国

内和国际评论委员会和编委会成员。研究领域包括天体的核反应的研究,大爆炸核合成过程,星星,超新星与中子星合并、星系化学动力学演化、中微子振荡和粒子宇宙学。

 

教育背景EDUCATION BACKGROUND:

梶野敏贵教授1984年从东京大学获学士和博士学后立即加入东京都大学获得教授助理职位

 

工作经历WORKING EXPERIENCE:

一直在东京都大学(1984 - 1993)和东京大学(1994 -现在)任教授,并于担任教授期间指导了32名研究生,从2017年3月开始在澳门新萄京6692 cc工作,目前招收了两名直博研究生.

 

课题组主页(或个人主页):

http://th.nao.ac.jp/MEMBER/kajino/e/index.html

 

奖励与荣誉AWARD AND HONOR:

2004 - present Fellow, American Physical Society (USA)

2016 – present One Thousand Talents Plan, Foreign Expert (China)

1986 Jun. - 1987Aug. Visiting Research Associate, National Superconducting Cyclotron

Laboratory,Michigan State University

1987 Sep. - 1992Aug. Consultant, Physics Division, Lawrence Livermore NationalLaboratory,

University ofCalifornia

1989 May -Jun. Visiting Professor, Harvard Smithsonian Center forAstrophysics,

1989 Jul., 1992Feb.-Apr. Visiting Professor, Research School of Physical Sciences,

Institute forAdvanced Studies, Australian National University

1992Jan. Visiting Professor, Research Centerfor Theoretical Astrophysics,

University ofSydney

1995 May –Jun. Visiting Professor, Laboratory for Nuclear andHigh-Energy Physics,

M & P.Curie University of Paris

1996 Oct., 1998Aug. Visiting Professor, Department of Physics, Ohio State University

1996 Jun.-Aug., 2001Jul.-Sep. Visiting Professor, Department of Physics and Center for


 

Astrophysics,University of Notre Dame

2013 Paper selected as Highlight of Journal of Physics G in 2013:

T. Suzuki, and T. Kajino, J. Phys.G40(2013), 083101, “Element

Synthesis in Supernova Environmentand Neutrino Oscillations”

2016年获北京外专千人

 

学术兼职ACADEMIC PART-TIME JOB:

- The University of Tokyo, GraduateSchool of Science, Professor

- National Astronomical Observatory of Japan, Division of Science, Professor

- The Graduate University for Advanced Studies, School of Physical

Science, Adjunct Professor

- Tohoku University, Graduate Program on Physics for the Universe,

Visiting Lecturer

- Japan Forum of Nuclear Astrophysics, Chairman

 

承担项目PROJECTS RESPONSIBLE FOR:

1. Creation of space-time,elementary particles and nuclei

2. Origin of dark matter,dark energy, and their roles in cosmic structure formation and cosmic microwavebackground anisotropies

3. Explosion mechanism andnucleosynthesis in supernovae, binary neutron star mergers, gamma-ray bursts

4. Galactic chemo-dynamicalevolution

5. Neutrino astrophysicsand oscillation physics

6. Origin of life andamino-acid homochirality

 

代表性学术成果REPRESENTATIVE ACADEMIC ACHIEVEMENTS:

T. Hayakawa, H. Ko, M.K. Cheoun, M. Kusakabe, T. Kajino, U. Mark, S. Chiba, K. Namakura, T. Alexey,K. Nomoto, M. Hashimoto, M. Ono, G. J. Mathews,

Phys. Rev. Lett.121(2018),Issue 10, id.102701,

Short-livedradioisotope98Tc synthesized by supernova neutrino process.

M. A. Famiano, R. N.Boyd, T. Kajino, T. Onaka, and Y. Mo,

Sci. Rep.8(2018),8833,

Amino Acid ChiralSelection Via Weak Interactions in Stellar Environments: Implications for theOrigin of Life.

M. A.Famiano, R. N. Boyd, T. Kajino, T. Onaka,

Astrobiology18(2018), 190-206,

Selection of Amino AcidChirality via Weak Interactions with14Nin CrossedElectric andMagnetic Fields.

R. N. Boyd, M. A.Famiano, T. Kajino, T. Onaka, and Y. Mo,

Astrophys. J.856(2018),article id. 26, 5 pp,

Sites that can produceleft-handed amino acids in the supernova neutrino aminoacidprocessing model.

T. Maruyama, A. B.Balantekin, M.-K. Cheoun, T. Kajino, and G. J. Mathews,

Phys. Lett.B779(2018),160-165,

Axion Production fromLandau Quantization in the Strong Magnetic Field of Magnetars.

T. Suzuki, T. Yoshida,S. Shibagaki, T. Kajino, and T. Otsuka,

Astrophys.J.859(2018), Issue 2, article id. 133, 9 pp,

Beta-decay Ratesfor Exotic Nuclei and r-process Nucleosynthesis up to Thorium and Uranium.

J. W. Shin, M. K.Cheoun, T. Kajino, and T. Hayakawa,

JCAP09(2018), 024,

Spectralshape analysis for electron antineutrino oscillation study by using8Ligenerator with252Cf source.

K. Mori,M. A.Famiano,T. Kajino,T. Suzuki, P. M. Garnavich, G. J. Mathews, R. Diehl, S.-C. Leung, andK. Nomoto,

Astrophys. J.863(2018),Issue 2, article id. 176, 10 pp,

NucleosynthesisConstraints on the Explosion Mechanism for Type Ia Supernovae.

M. R. Gangopadhyay, G.J. Mathews, K. Ichiki, and T. Kajino,

Eur. Phys. J.C78(2018), Issue 9, article id. 733, 10 pp,

Explaining low lanomalies in the CMB power spectrum with resonant superstring excitationsduring inflation.

G.Abdellaoui et al. with T. Kajino (JEM EUSO Collaboration),

Astropart.Phys.102(2018), 98-111,

EUSO-TA -First results from a ground-based EUSO telescope.

G.Abdellaoui et al. with T. Kajino (JEM EUSO Collaboration),

J. Instr.13,(2018), Issue 05, pp. P05023,

Firstobservations of speed of light tracks by a fluorescence detector looking downon the atmosphere.

T. Kajino,and G. J. Mathews,

Rep.Prog.Phys.80(2017), 084901 (16pp),

Impact ofnew data for neutron-rich heavy nuclei on theoretical models for r-processnucleosynthesis.

S. Q. Hou, J. J. He, A.Parikh, D. Kahl, C. A. Bertulani, T. Kajino, G. J. Mathews & G. Zhao,

Astrophys. J.834(2017), 165,

Non-extensiveStatistics to the Cosmological Lithium Problem.

Y.Hirai, Y.Ishimaru, T. R. Saitoh, M. S. Fujii, J. Hidaka, and T. Kajino,

MNRAS466(2017),2472-2487,

The Relation between Enrichmentof R-process Elements and Dynamical Evolution of Dwarf Galaxies.

J. W. Shin,M. K. Cheoun, T. Kajino, and T. Hayakawa,

JCAP04(2017), 044,

Short-baseline electronantineutrino disappearance study by using neutrino sources From C13+Be9 reaction.

D. G.Yamazaki, M. Kusakabe, T. Kajino, G. J. Mathews, and M.-K. Cheoun,

Int. J. Mod.Phys.E26(2017), 1741006 (12 pages),

The new hybrid BBNmodel with the photon cooling, X particle, and the primordialmagneticfield.

Grant J.Mathews, Motohiko Kusakabe, and Toshitaka Kajino,

Mod. Phys. Lett.E26(2017),1741001 (21 pages),

Introduction toBig-Bang Nucleosynthesis and Modern Cosmology.

MotohikoKusakabe, Grant J. Mathews, Toshitaka Kajino, and Myung-Ki Cheoun,

Int. J. Mod. Phys.E26(2017),1741004 (27 pages),

Review on effects oflong-lived negatively charged massive particles on big-bang nucleosynthesis.

J. W. Shin,M. K. Cheoun, T. Kajino, and T. Hayakawa,

J. Phys.Lett.G44(2017),09LT01; Corrigendum,G45(2018),029501,

A new schemefor short baseline electron antineutrino disappearance study.

H. Sasaki,T. Kajino, T. Takiwaki, T. Hayakawa, A. B. Balantekin, and Y. Pehlivan,

Phys. Rev.D96(2017), 043013,

Possible effects ofcollective neutrino oscillations in the three flavor multi-angle simulations onsupernova νp-process.

T. Hayakawa, T.Nakamura, H. Kotaki, M. Kando, and T. Kajino,

Quantum Beam Scienc1(2017),3 (12pp),

Explosivenucleosynthesis study using laser driveng-ray pulses.

G.Abdellaoui et al. with T. Kajino (JEM EUSO Collaboration),

NuclearInst. And Methods in Physics Research,A866(2017), 150-163,

Cosmic rayoriented performance studies for the JEM-EUSO first level trigger.

G. Abdellaoui et al.with T. Kajino (JEM EUSO Collaboration),

Planetaryand Space Science,143(2017), 245-255,

Meteorstudies in the framework of the JEM-EUSO program.

 

T. Hayakawa, Y. Toh, M.Huang, T. Shizuma, A. Kimura, S. Nakamura, H. Harada, N. Iwamoto, S. Chiba andT. Kajino,

Phys. Rev.C94(2016), 055803,

Measurementof isomer productiuon ratio for the112Cd(n,g)113Cd reactionusing neutron beams at J-PARC.

S.Shibagaki, T. Kajino, G. J. Mathews, S. Chiba, S. Nishimura, and G. Lorusso,

Astrophys.J.816(2016), 79,

Relativecontributions of the weak, main and fission-recycling r-process.

T. Maruyama,M.-K. Cheoun, T. Kajino, and G. J. Mathews,

Phys. Lett.B757(2016),125-129,

Pion Production viaProton Synchrotron Radiation in Strong Magnetic Fields in Relativistic FieldTheory: Scaling Relations and Angular Distributions.

M. A.Famiano, A. B. Balantekin, and T. Kajino,

Phys. Rev.C93(2016),045804,

Low-lying resonancesand relativistic screening in Big Bang Nucleosynthesis.

C.Bertulani, and T. Kajino,

Prog. Part.Nucl.Phys.89(2016),56-100,

Frontiers inNuclear Astrophysics.

J. Hidaka,T. Kajino, and G. J. Mathews,

Astrophys.J.827(2016), 85 (6pp),

Red-supergiantand Supernova Rate Problems: Implication for the Relic Supernova NeutrinoSpectrum.

 

G. J.Mathews, B.Rose, P. Garnavich, D. Yamazaki, and T. Kajino,

Astrophys. J.827(2016),60 (11pp),

Detectability of cosmicdark flow in the type Ia supernova redshift-distance relation.

M. A.Famiano, T. Kajino, W. Aoki, and T. Suda,

Astrophys. J.830(2016),61 (13pp),

Dependence of the Sr/Baand Sr/Eu Ratios on the Nuclear Equation of states in the metal-poor halostars.

M. L.Warren, G. J. Mathews, M. Meixner, J. Hidaka, and T. Kajino,

Int. J.Mod. Phys.A31(2016), 1650137,

Impact ofsterile neutrino dark matter on core-collapse supernovae.

J. W. Shin,M. K. Cheoun, T- S. Park, and T. Kajino,

Phys. Rev.C94(2016), 045804,

New neutrinosource for the study of solar neutrino physics in the vacuum-matter transitionregion.

K. Mori,M. A.Famiano,T. Kajino,T. Suzuki,J. Hidaka, M. Honma, K. Iwamoto, K. Nomoto, andT. Otsuka,

Astrophys. J.833(2016), 179,

Impact of New GTStrengths on Explosive SN Ia Nucleosynthesis.

G. Lorusso,et al. with T. Kajino,

Phys. Rev. Lett.114(2015),192501,

β -Decay Half-Lives of110 Neutron-Rich Nuclei across the N =82 Shell Gap: Implications for theMechanism and Universality of the Astrophysical r Process.

Dai. G. Yamazaki,Toshitaka Kajino, Grant J. Mathews, and Kiyotomo Ichiki,

Phys. Rep.517(2012),141-167,

The Search for aPrimordial Magnetic Field.

Takashi Yoshida,Toshitaka Kajino, Hidekazu Yokomakura, Kei-ichi Kimura, Akira Takamura, andDieter Hartmann,

Phys. Rev.Lett.96(2006), 091101,

SupernovaNeutrinos Nucleosynthesis of Light Elements with Neutrino Oscillations.

A. Frebel, et al. withT. Kajino,

Nature434(2005), 871-873,

Nucleosyntheticsignature of the first stars.

 

TakashiYoshida, Toshitaka Kajino, and Dieter Hartmann,

Phys. Rev.Lett.94(2005), 231101,

Constrainingthe Spectrum of Supernova Neutrinos fromn-Process Induced LightElement Synthesis.

T. Hayakawa,N. Iwamoto, T. Shizuma, T. Kajino, H. Umeda, and K. Nomoto,

Phys. Rev. Lett.93(2004), 161102,

Evidence fornucleosynthesis in supernovag-process: Universal scaling on p-nuclei.

K. Ichiki,M. Yahiro, T. Kajino, M. Orito, and G. J. Mathews,

Phys. Rev.D66(2002), 043521,

Observationalconstraints on dark radiation in brane cosmology.

H. Kawakita,et al. with T. Kajino,

Science294(2001), 1089-1091,

The SpinTemperature of NH3in Comet C/1999S4 (LINEAR).

M. Terasawa, K.Sumiyoshi, T. Kajino, I. Tanihata, and G. J. Mathews,

Astrophys. J.562(2001), 470-479,

New Nuclear ReactionFlow towards R-Process Nucleosynthesis in Supernovae: A Critical Role of theLight Neutron-Rich Nuclei.

S. Wanajo,T. Kajino, and G. J. Mathews, and K. Otsuki,

Astrophys.J.554(2001), 578-586,

Ther-process in netrino-driven winds from nascent compact neutron stars ofcore-collapse supernovae.

K. Otsuki, H. Tagoshi,T. Kajino and S. Wanajo,

Astrophys. J.533(2000), 424-439,

The generalrelativistic effects on neutrino-driven winds from young, hot neutron stars andthe r-process nucleosynthesis.

F. C.Barker, and T. Kajino,

AustralianJ. Phys.44(1991), 369-396,

Channelcontributions to low energy12C(4He,g)16O crosssection in massive stars.

T. Kajino,

Phys. Rev. Lett.66(1991),125-128,

Can quark-gluon plasma formation inrelativistic heavy-ion collisions constraininhomogeneous cosmologies?

T. Kajino,and R. N. Boyd,

Astrophys.J.359(1990), 267-276,

Productionof light elements in primordial nucleosynthesis.

T. Kajino,

Nucl. Phys.A460(1986), 559-580,

Thenuclearstructure and reactions of3He(4He,g)7Be and3H(4He,g)7Liatastrophysical energies.

 

T. Kajino, and A.Arima,

Phys. Rev. Lett.52(1984), 739-742,

Resonating groupcalculations of radiative capture reactions3He(4He,g)7Be and3H(4He,g)7Li atastrophysical low energies and missing solar neutrino problem.

 

 

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