Basic Information

写真a

Yasushi NARA


Title

Professor

Nationality

JAPAN

Research Fields, Keywords

Theoretical Nuclear Physics

E-Mail Address

E-mail address

Homepage URL

https://inspirehep.net/literature?sort=mostrecent&size=25&page=1&q=f%20a%20y%20nara&ui-citation-summary=true

Research Field

My main interest is to explore and understand the ultimate properties of matter at extreme conditions such as the matter just after the Big-Bang. High energy nuclear collisions can create such hot and dense matter which was existed just after the Big-Bang. This state of matter is called Quark-Gluon Plasma (QGP). QGP is a new form of matter; protons and neutrons are melted to quarks and gluons. In particular, I am interested in understanding a spacetime evolution of matter created in the nuclear collisions.
To the head of this page.▲

Professional Career On-Campus 【 display / non-display 】

  • Akita International University Faculty of International Liberal Arts Global Connectivity Program, Professor, 2021/04 -

  • Akita International University Faculty of International Liberal Arts Basic Education Mathematics,Natural Science, Professor, 2013/04 - 2021/03

To the head of this page.▲

Academic Society Affiliations 【 display / non-display 】

  • The Physical Society of Japan (JPS), 1993/04 - , JAPAN

To the head of this page.▲

Field of Expertise 【 display / non-display 】

  • Particle/Nuclear/Cosmic ray/Astro physics

To the head of this page.▲
 

Academic Papers 【 display / non-display 】

  • Comparing pion production in transport simulations of heavy- ion collisions at 270AMeV under controlled conditions, Physical Review C, vol.109 (4) (p.044609-1 - 044609-34-8) , 2024/04, Jun Xu, et. al

    DOI:doi:10.1103/PhysRevC.109.044609, Research paper (scientific journal), Multiple Authorship, English

  • Bulk properties of the system formed in U+U collisions at sNN=2.12 GeV using the jet AA microscopic transport model, Physical Review C, vol.109 (5) (p.054902-1 - 054902-8) , 2024/03, A. K. Sahoo, X. He, Y. Nara and S. Singha

    DOI:doi:10.1103/PhysRevC.109.054902, Research paper (scientific journal), Multiple Authorship, English

  • Enhanced Dilepton production near the color superconducting phase and the QCD critical point, European Physical Journal C, vol.60 (4) (p.82-1 - 82-8) , 2024/02, Toru Nishimura, Yasushi Nara, Jan Steinheimer

    DOI:doi:10.1140/epja/s10050-024-01273-y, Research paper (scientific journal), Multiple Authorship, English

  • Repulsive potentials in dense neutron star matter and binding energy of Lambda in hypernuclei, Physical Review C, vol.108 (6) (p.065803-1 - 065803-15) , 2023/12, A. Jinno, K. Murase, Y. Nara and A. Ohnishi

    DOI:10.1103/PhysRevC.108.065803, Research paper (scientific journal), Multiple Authorship, English

  • Poincaré covariant cascade method for high-energy nuclear collisions, Physical Review C, vol.108 (2) (p.024910-1 - 024910-13) , 2023/08, Y. Nara, A. Jinno, T. Maruyama, K. Murase and A. Ohnishi

    DOI:10.1103/PhysRevC.108.024910, Research paper (scientific journal), Multiple Authorship, English

display all >>

To the head of this page.▲

Books 【 display / non-display 】

  • Properties of QCD Matter at High Baryon Density, Springer Singapore, 2022/12, H. Elfner, J. Y. Jia, Z. W. Lin, Y. Nara, L. G. Pang, C. Shen, S. S. Shi, M. Stephanov, L. Yan, Y. Yin, and P. F. Zhuang

    Scholarly Book, Allotment Writing, English

To the head of this page.▲

Grant-in-Aid for Scientific Research 【 display / non-display 】

  • Grant-in-Aid for Scientific Research (C)，2021/04 - 2024/03，Study of high density QCD matter by the quantum molecular fluid dynamics simulation

  • Grant-in-Aid for Scientific Research (B)，2017/04 - 2020/03

  • Grant-in-Aid for Scientific Research (C)，2017/04 - 2020/03，Development of a event-generator for high energy nuclear colliisons based on a microscopic transport theory

  • Grant-in-Aid for Scientific Research (C)，2015/04 - 2018/03

  • Grant-in-Aid for Scientific Research (C)，2015/04 - 2017/03

display all >>

To the head of this page.▲

Presentations 【 display / non-display 】

  • Meeting of the Physics Society of Japan, 2025 spring meeting, Domestic Conference, 2025/03, A new formulation for the relativistic quantum molecular dynamics II, Oral Presentation (general)

  • STAR Collaboration Meeting: eTOF and BES-II workshop, International Conference, 2024/12, A new RQMD formulation: Potentials/EoS in the microscopic transport model JAM, Oral Presentation (general)

  • Meeting of the Physics Society of Japan, 2024 meeting, Domestic Conference, 2024/09, Dynamics of nuclear collisions from microscopic transport models, Oral Presentation (general)

  • Meeting of the Physics Society of Japan, 2024 meeting, Domestic Conference, 2024/09, A new formulation for the relativistic quantum molecular dynamics, Oral Presentation (general)

  • Meeting of the Physics Society of Japan, 2024 spring meeting, Domestic Conference, 2024/03, Analysis of directed flow by relativistic quantum molecular dynamics (RQMD) with chiral symmetry restoration (CSR), Oral Presentation (general)

display all >>

To the head of this page.▲
 
 
 

Community Activities Outside University 【 display / non-display 】

  • AIU Open Lecture，2022/01

    Matter changes its sate from solid, liquid, to gas according to the temperature and density. Around thousands of temperature, plasma state appears, which consists of ions. For example, the Sun is a plasma. What will happen when temperature or density is even higher?
    According to the Big-Bang cosmology, our universe began 13.8 billion years ago from Big-Bang. The highest temperature was achieved in the early universe. On the other hand, there are compact stars such as black holes and neutron stars. It is expected that the core of neutron star is the highest density in the current universe. We can explore high temperature and density state of matter by experiment in the laboratory by using high energy heavy-ion collisions. In this lecture, I introduce what we know about such extreme state of matter from high-energy heavy-ion collision.

To the head of this page.▲