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- The University of TokyoJP813 papers
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- The University of OsakaJP408 papers
- High Energy Accelerator Research OrganizationJP377 papers
- Tokyo Institute of TechnologyJP377 papers
- National Astronomical Observatory of JapanJP331 papers
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- Chinese Academy of SciencesCN316 papers
- University of Science and Technology of ChinaCN311 papers
- The University of MelbourneAU307 papers
- Institute for High Energy PhysicsES298 papers
122 papers · 1 filter
How Close Dark Matter Halos and MOND Are to Each Other: Three-Dimensional Tests Based on Gaia DR2
Yongda Zhu, Hai-Xia Ma, Xiao-Bo Dong +7
Aiming at discriminating different gravitational potential models of the Milky Way, we perform tests based on the kinematic data powered by the Gaia DR2 astrometry, over a large ra…
Electronic Properties of Pyrochlore-Type Ca2Ir2O7
Yuki Nakayama, Yoshihiko Okamoto, Daigorou Hirai +1
The electrical resistivity, magnetic susceptibility, and heat capacity of sintered samples of Ca2Ir2O7, in which pentavalent Ir atoms with 5d4 electron configuration form a pyrochl…
The Effect of Shock Wave Duration on Star Formation and the Initial Condition of Massive Cluster Formation
Daisei Abe, Tsuyoshi Inoue, Rei Enokiya +1
Stars are born in dense molecular filaments irrespective of their mass. Compression of the ISM by shocks cause filament formation in molecular clouds. Observations show that a mass…
Study on the reusability of fluorescent nuclear track detectors using optical bleaching
Abdul Muneem, Junya Yoshida, Hiroyuki Ekawa +14
Fluorescent nuclear track detectors (FNTDs) based on AlO:C,Mg crystals are luminescent detectors that can be used for dosimetry and detection of charged particles and n…
Formalizing Anisotropic Inflation in Modified Gravity
S. Nojiri, S. D. Odintsov, V. K. Oikonomou +1
Motivated by the fact that the pre-inflationary era may evolve in an exotic way, in this work we formalize anisotropic evolution in the context of modified gravity, focusing on pre…
A Data-constrained Magnetohydrodynamic Simulation of the X1.0 Solar Flare of 2021 October 28
Daiki Yamasaki, Satoshi Inoue, Yumi Bamba +2
The solar active region NOAA 12887 produced a strong X1.0 flare on 2021 October 28, which exhibits X-shaped flare ribbons and a circle-shaped erupting filament. To understand the e…