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Sensitivity of JEM-EUSO to GRB Neutrinos · Around

2009

Sensitivity of JEM-EUSO to GRB Neutrinos

Asano, Katsuaki, Shinozaki, Kenji, Teshima, Masahiro

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JEM-EUSO is a mission to study ultra-high-energy cosmic rays (UHECRs) by measuring the fluorescence light from giant air showers at the altitude of the International Space Station.

In the tilted mode, JEM-EUSO will become very sensitive to the \v{C}erenkov light from the earth skimming tau neutrinos at the energy range of $10^{16-18}$eV.
In this paper we will discuss high-energy tau neutrinos from nearby gamma-ray bursts (GRBs).
From simulations of cascade in GRB photon fields including various hadronic/leptonic processes, we estimate the neutrino flux from GRBs.

Built on

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Similar

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Then

Guetta, D., & Piran, T. S. 2007, JCAP, 07, 003
2007
Later among the works it cites.
Ebisuzaki, T. et al., Nucl. Phys. B (Proc. Suppl.), 175, 237 (2008)
2008
Later among the works it cites.
Murase, K., 2008, J. Phys.: Conf. Series
2008
Later among the works it cites.
Kaneko, Y. et al. 2008, Astro. Phys. J., 677, 1168
2008
Later among the works it cites.
Asano, K., Inoue, S., & Mészáros, P. 2009, Astro. Phys. J. 699, 953
2009
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