Abstract
The energy spectrum of neutrons produced by cosmic ray muons in the underground detector LVD (3650 m.w.e.) is obtained for the energy range of 30–450 MeV. The spectrum is derived using the energy release spectrum of neutron interaction products in 1.5 m3 scintillation counters.
Similar content being viewed by others
References
Malgin, A.S., Ryazhskaya, O.G., Ryasny, V.G., and Khal’chukov, F.F., Pis’ma Zh. Eksp. Teor. Fiz., 1982, vol. 36, p. 308 [JETP Lett. (Engl. Transl.), vol. 36, p. 378].
Barton, J.C., Proc. 19th ICRC, La Jolla, 1985, vol. 8, p. 98.
Armbruster, B. et al., Phys. Rev. D, 2002, vol. 65, no. 112, p. 1.
Ahlietta, M. et al., Proc. 26th ICRC, Salt Lake Sity, 1999, vol. 2, p. 44.
Aglietta, M. et al. (LVD Collaboration), Proc. 29th ICRC, Pune, 2005, vol. 6, p. 337.
Agafonova, N.Yu. et al. (LVD Collaboration), Izv. Ross. Akad. Nauk, Ser. Fiz., 2005, vol. 69, no. 3, p. 400.
Dementyev, A., Gurentsov, V., Ryazhskaya, O., and Sobolevsky, N., Nucl. Phys. B (Proc. Suppl.), 1999, vol. 70, p. 486.
Author information
Authors and Affiliations
Corresponding author
Additional information
Original Russian Text © N.Yu. Agafonova, V.V. Boyarkin, V.L. Dadykin, E.A. Dobrynina, R.I. Enikeev, V.V. Kuznetsov, A.S. Malgin, O.G. Ryazhskaya, V.G. Ryasny, V.F. Yakushev (LVD collaboration), N.M. Sobolevsky, 2009, published in Izvestiya Rossiiskoi Akademii Nauk. Seriya Fizicheskaya, 2009, Vol. 73, No. 5, pp. 666–667.
(LVD collaboration)
About this article
Cite this article
Agafonova, N.Y., Boyarkin, V.V., Dadykin, V.L. et al. The energy spectrum of neutrons produced by cosmic ray muons in LVD. Bull. Russ. Acad. Sci. Phys. 73, 628–629 (2009). https://doi.org/10.3103/S1062873809050281
Published:
Issue Date:
DOI: https://doi.org/10.3103/S1062873809050281