Abstract
The vertical muon energy spectra at sea level have been estimated from directly measured primary cosmic-ray nucleon spectrum. The hadronic energy moments have been calculated from the CERN LEBC EHS data on the Lorentz invariant cross-section results on pp → π±X and pp → K±X inclusive reactions and are duly corrected for A–A collisions. Finally, the sea level muon energy spectra have been calculated from the decay of conventional mesons, using standard formulation. The estimated muon spectra are found to be in good agreement with the directly measured muon spectra obtained from the different experiments.
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References
M. Honda et al.: Phys.Re v. D 52 (1995) 4985.
T.K. Gaisser and T. Stanev: in Proc. 24th Int. Cosmic Ray Conf., Rome, 1995, Vol. 1, p.694.
Y. Fukuda et al.: Phys. Rev.Lett. 81 (1998) 1562.
S.A. Stephens: in Proc. 16th Int. Cosmic Ray Conf., Kyoto, 1979, Vol.10, p.90.
BESS-98 Flight, T. Sanuki et al.: Astrophys. J. 545 (2000) 1135.
W. Menn et al.: Astrophys. J. 533 (2000) 281.
J. Alcaraz et al.: Phys.Let t.B 472 (2000) 215.
M. Boezio et al.: Astrophys. J. 518 (1999) 457.
R. Bellotti et al.: Phys. Rev.D 60 (1999) 052002.
E.S. Seo et al.: Astrophys. J. 378 (1991) 763.
K. Asakimori et al.: Astrophys.J. 502 (1998) 278.
CRN, D. Muller et al.: Astrophys. J. 374 (1991) 356.
SOKOL, I.P. Ivanenko et al.: in Proc. 23rd Int. Cosmic Ray Conf., Calgary, 1993, Vol.2, p.17.
A. Dar: Cosmic Ray muons at ground level and deep underground, Technion Physics Report No.84-41, 1984.
Aguliar Benitez et al.: Z. Phys. C 50 (1991) 405.
G.B. Yodh, R.W. Ellsworth, T. Stanev, and T.K. Gaisser: Nucl. Phys. B 183 (1981) 12.
D.P. Bhattacharyya: Can.J.Phys. 61 (1983) 434.
Y. Minorikawa and K. Mitsui: Lett. Nuovo Cimento 44 (1985) 651.
M. Mitra, P. Pal, and D.P. Bhattacharyya: Nuovo Cimento 20 (1997) 527.
S.N. Boziev, A.E. Chudakov, and A.V. Voevodsky: in Proc. 21st Int. Cosmic Ray Conf., Adelaide, 1990, Universty of Adelaide, Vol.9, p.38.
CAPRICE-94, J. Kremmer et al.: in Proc. 26th Int. Cosmic Ray Conf., Salt Lake City (Utah), 1999, Vol.2, 76.
O.C. Allkofer, K. Carstensen, W.D. Dau, H. Jokisch, and H.J. Meyer: Proc. I.C.R. Symp., Tokyo, 1976, p.26.
O.C. Allkofer, K. Carstensen, and W.D. Dau: Phys.Le tt.B 36 (1971) 425.
P.J. Hayman and A.W. Wolfendale: Proc.P hys.So c.Lo ndon 80 (1962) 710.
M.P. De Pascale et al.: J.Geop hys.Res. 98 (1993) 3501.
L.V. Volkova, G.T. Zatsepin, and L.A. Kuz'michev: Sov. J. Nucl. Phys. 29 (1979) 645.
A. Dar: Phys. Rev.Lett. 51 (1983) 227.
A.V. Butkevich, L.G. Dedenko, and I.M. Zheleznykh: Sov. J. Nucl. Phys. 50 (1989) 90.
P. Lipari: Astroparticle Phys. 1 (1993) 195.
V. Agrawal, T.K. Gaisser, P. Lipari, and T. Stanev: Phys.R ev. D 53 (1996) 1314.
E.V. Bugaev et al.: Phys. Rev. D. 58 (1998) 054001.
D.P. Bhattacharya: Phys.Rev. D 13 (1976) 1851.
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Haldar, T.K., Mitra, M. & Bhattacharyya, D. Estimation of Sea Level Muon Energy Spectrum at High Latitude from the Latest Primary Nucleon Spectra Near the Top of the Atmosphere. Czechoslovak Journal of Physics 53, 613–623 (2003). https://doi.org/10.1023/A:1024822518795
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DOI: https://doi.org/10.1023/A:1024822518795