output
20022025
most citedObservation of a resonance-like structure in the pi^+- psi' mass distribution in exclusive B-->K pi^+- psi' decays

550 citations

Showing 2017Show all

26 papers · 1 filter

hep-ex2017190 cited

Measurement of the multi-TeV neutrino cross section with IceCube using Earth absorption

IceCube Collaboration, M. G. Aartsen, M. Ackermann +314

Neutrinos interact only very weakly, so they are extremely penetrating. However, the theoretical neutrino-nucleon interaction cross section rises with energy such that, at energies…

astro-ph.SR201728 cited

Convective velocity suppression via the enhancement of subadiabatic layer: Role of the effective Prandtl number

Y. Bekki, H. Hotta, T. Yokoyama

It has recently been recognized that the convective velocities achieved in the current solar convection simulations might be over-estimated. The newly-revealed effects of the preva…

cs.CV2017164 cited

Computational ghost imaging using deep learning

Tomoyoshi Shimobaba, Yutaka Endo, Takashi Nishitsuji +8

Computational ghost imaging (CGI) is a single-pixel imaging technique that exploits the correlation between known random patterns and the measured intensity of light transmitted (o…

astro-ph.SR201754 cited

Improvement of solar cycle prediction: Plateau of solar axial dipole moment

H. Iijima, H. Hotta, S. Imada +2

Aims. We report the small temporal variation of the axial dipole moment near the solar minimum and its application to the solar cycle prediction by the surface flux transport (SFT)…

astro-ph.GA201726 cited

Fragmentation of Filamentary Cloud Permeated by Perpendicular Magnetic Field

Tomoyuki Hanawa, Takahiro Kudoh, Kohji Tomisaka

We examine the linear stability of an isothermal filamentary cloud permeated by a perpendicular magnetic field. Our model cloud is assumed to be supported by gas pressure against t…

astro-ph.HE201787 cited

Electron Surfing and Drift Accelerations in a Weibel-dominated High-Mach-number Shock

Yosuke Matsumoto, Takanobu Amano, Tsunehiko N. Kato +1

How electrons get accelerated to relativistic energies in a high-Mach-number quasi-perpendicular shock is presented by means of ab initio particle-in-cell simulations in three dime…