187 citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- T. Yamada4 profiles40 · h 22
- Y. Funaki2 profiles35 · h 27
- P. Schuck4 profiles26 · h 36
- A. Tohsaki2 profiles25 · h 30
- H. Horiuchi2 profiles21 · h 40
- Bo Zhou2 profiles13 · h 14
- Z. Ren2 profiles12 · h 39
- G. Röpke3 profiles11 · h 41
- Chang Xu2 profiles10 · h 51
- Hisashi Horiuchi10 · h 14
- M. Lyu10 · h 9
- K. Ikeda9 · h 34
- The University of OsakaJP50 papers
- RIKEN Nishina CenterJP37 papers
- RIKENJP31 papers
- Centre National de la Recherche ScientifiqueFR28 papers
- Université Paris-SudFR25 papers
- Kyoto UniversityJP23 papers
- University of RostockDE23 papers
- University of MiyazakiJP20 papers
- International Institute for Advanced StudiesJP19 papers
- Laboratoire de Physique et Modélisation des Milieux CondensésFR19 papers
- The University of TokyoJP19 papers
- Institute of Space and Astronautical ScienceJP18 papers
8 papers · 1 filter
Nuclei in Core-Collapse Supernovae Engine
Shun Furusawa, Hiroki Nagakura
Herein, we review the nuclear equations of state (EOSs) %for core-collapse supernova simulations and the constituent nuclei of core-collapse supernovae (CCSNe) and their roles in C…
Leptonic and semi-leptonic neutrino interactions with muons in the proto-neutron star cooling
Ken'ichi Sugiura, Shun Furusawa, Kohsuke Sumiyoshi +1
It is known that muons are scarce just after the birth of a proto-neutron star via a supernova explosion but get more abundant as the proto-neutron star cools via neutrino emission…
Single Event Tolerance of X-ray SOI Pixel Sensors
Kouichi Hagino, Mitsuki Hayashida, Takayoshi Kohmura +19
We evaluate the single event tolerance of the X-ray silicon-on-insulator (SOI) pixel sensor named XRPIX, developed for the future X-ray astronomical satellite FORCE. In this work,…
Cluster structures of the states of with the 3 four-body orthogonality condition model
Qian Wu, Yasuro Funaki, Xurong Chen
We study structures of the states of C within the framework of four-body orthogonality condition model with the Gaussian expansion method. We obtain five $…
Effects of nuclear matter and composition in core-collapse supernovae and long-term proto-neutron star cooling
Kohsuke Sumiyoshi, Shun Furusawa, Hiroki Nagakura +4
We study the influence of hot and dense matter in core-collapse supernovae by adopting up-to-date nuclear equation of state (EOS) based on the microscopic nuclear many-body framewo…
Equation of state in neutron stars and supernovae
Kohsuke Sumiyoshi, Toru Kojo, Shun Furusawa
Neutron stars and supernovae provide cosmic laboratories of highly compressed matter at supra nuclear saturation density which is beyond the reach of terrestrial experiments. The p…
Protoneutron Star Convection Simulated with a New General Relativistic Boltzmann Neutrino Radiation-Hydrodynamics Code
Ryuichiro Akaho, Akira Harada, Hiroki Nagakura +6
We investigate the protoneutron star (PNS) convection using our newly developed general relativistic Boltzmann neutrino radiation-hydrodynamics code. This is a pilot study for more…
X-ray Radiation Damage Effects on Double-SOI Pixel Detectors for the Future Astronomical Satellite "FORCE"
Masatoshi Kitajima, Kouichi Hagino, Takayoshi Kohmura +20
We have been developing the monolithic active pixel detector "XRPIX" onboard the future X-ray astronomical satellite "FORCE". XRPIX is composed of CMOS pixel circuits, SiO2 insulat…