Zobrazeno 1 - 10
of 431
pro vyhledávání: '"Midorikawa, S."'
Publikováno v:
Phys. Rev. D 100, 123022 (2019)
We examine the uncertainty of the calculation of the atmospheric neutrino flux and present a way to reduce it using accurately measured atmospheric muon flux. Considering the difference of the hadronic interaction model and the real one as a variatio
Externí odkaz:
http://arxiv.org/abs/1908.08765
In this paper, we extend the calculation of the atmospheric neutrino flux~\cite{hkkm2004,hkkms2006,hkkm2011} to the sites in polar and tropical regions. In our earliest full 3D-calculation~\cite{hkkm2004}, we used DPMJET-III~\cite{dpm} for the hadron
Externí odkaz:
http://arxiv.org/abs/1502.03916
We present the calculation of the atmospheric neutrino fluxes for the neutrino experiments proposed at INO, South Pole and Pyh\"asalmi. Neutrino fluxes have been obtained using ATMNC, a simulation code for cosmic ray in the atmosphere. Even using the
Externí odkaz:
http://arxiv.org/abs/1210.5154
Publikováno v:
Phys.Rev.D75:043006,2007
Using the ``modified DPMJET-III'' model explained in the previous paper, we calculate the atmospheric neutrino flux. The calculation scheme is almost the same as HKKM04 \cite{HKKM2004}, but the usage of the ``virtual detector'' is improved to reduce
Externí odkaz:
http://arxiv.org/abs/astro-ph/0611418
Publikováno v:
Phys.Rev.D75:043005,2007
We have studied the hadronic interaction for the calculation of the atmospheric neutrino flux by summarizing the accurately measured atmospheric muon flux data and comparing with simulations. We find the atmospheric muon and neutrino fluxes respond t
Externí odkaz:
http://arxiv.org/abs/astro-ph/0611201
Publikováno v:
Phys.Rev. D70 (2004) 043008
We have revised the calculation of the flux of atmospheric neutrinos based on a 3-dimensional scheme with the realistic IGRF geomagnetic model. The primary flux model has been revised, based on the AMS and BESS observations, and the interaction model
Externí odkaz:
http://arxiv.org/abs/astro-ph/0404457
Precise knowledge of the hadronic interaction between primary cosmic rays and atmospheric nuclei is very important and fundamental to study atmospheric neutrinos and their oscillations. We studied hadronic interaction models using the data of primary
Externí odkaz:
http://arxiv.org/abs/astro-ph/0312632
Autor:
Kasahara, K., Mochizuki, E., Torii, S., Tamura, T., Tateyama, N., Yoshida, K., Yamagami, T., Saito, Y., Nishimura, J., Murakami, H., Kobayashi, T., Komori, Y., Honda, M., Ohuchi, T., Midorikawa, S., Yuda, T.
Publikováno v:
Phys.Rev. D66 (2002) 052004
We observed atmospheric gamma-rays around 10 GeV at balloon altitudes (15~25 km) and at a mountain (2770 m a.s.l). The observed results were compared with Monte Carlo calculations to find that an interaction model (Lund Fritiof1.6) used in an old neu
Externí odkaz:
http://arxiv.org/abs/hep-ex/0206055
Publikováno v:
Phys.Rev. D64 (2001) 053011
A 3-dimensional calculation of atmospheric neutrinos flux is presented, and the results are compared with those of a 1-dimensional one. In this study, interaction and propagation of particles is treated in a 3-dimensional way including the curvature
Externí odkaz:
http://arxiv.org/abs/hep-ph/0103328
Publikováno v:
Phys.Rev.D54:5578-5584,1996
We compare several different calculations of the atmospheric neutrino flux in the energy range relevant for contained neutrino interactions, and we identify the major sources of difference among the calculations. We find nothing that would affect the
Externí odkaz:
http://arxiv.org/abs/hep-ph/9608253