Ultrahigh-energy neutrino interactions

Astroparticle Physics

Volumn 5, Issue 2, 1996, Pages 81-110

  Gandhi, Raj ^a   Quigg, Chris ^b,c   Reno, Mary Hall ^d   Sarcevic, Ina ^e  

^a HARISH CHANDRA RESEARCH INSTITUTE   (India)

^b FERMI NATIONAL ACCELERATOR LABORATORY   (United States)

^c Department of Obstetrics Gynecology   (United States)

^d UNIVERSITY OF IOWA   (United States)

^e University of Arizona   (United States)

Author keywords

Neutrino astronomy; Neutrino electron scattering; Neutrino nucleon scattering

Indexed keywords

EID: 0030215597     PISSN: 09276505     EISSN: None     Source Type: Journal    
DOI: 10.1016/0927-6505(96)00008-4     Document Type: Article

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44. The Deep Underwater Muon and Neutrino Detector is described by V.Z. Peterson, in: Currents in Astrophysics and Cosmology: Papers in Honor of Maurice M. Shapiro, G.G. Fazio and R. Silberberg, eds. (Cambridge University Press, Cambridge, 1994) p. 169; P.K.F. Grieder, in: NESTOR, Third NESTOR International Workshop, 19-21 October 1993, L.K. Resvanis, ed. (Athens University Press, Athens, 1994) p. 168; For a personal history of the DUMAND Project, see A. Roberts, Rev. Mod. Phys. 64 (1992) 259.
45. The Deep Underwater Muon and Neutrino Detector is described by V.Z. Peterson, in: Currents in Astrophysics and Cosmology: Papers in Honor of Maurice M. Shapiro, G.G. Fazio and R. Silberberg, eds. (Cambridge University Press, Cambridge, 1994) p. 169; P.K.F. Grieder, in: NESTOR, Third NESTOR International Workshop, 19-21 October 1993, L.K. Resvanis, ed. (Athens University Press, Athens, 1994) p. 168; For a personal history of the DUMAND Project, see A. Roberts, Rev. Mod. Phys. 64 (1992) 259.
46. The Deep Underwater Muon and Neutrino Detector is described by V.Z. Peterson, in: Currents in Astrophysics and Cosmology: Papers in Honor of Maurice M. Shapiro, G.G. Fazio and R. Silberberg, eds. (Cambridge University Press, Cambridge, 1994) p. 169; P.K.F. Grieder, in: NESTOR, Third NESTOR International Workshop, 19-21 October 1993, L.K. Resvanis, ed. (Athens University Press, Athens, 1994) p. 168; For a personal history of the DUMAND Project, see A. Roberts, Rev. Mod. Phys. 64 (1992) 259.
47. See also R.J. Wilkes, DUMAND and AMANDA: High-Energy Neutrino Astrophysics, University of Washington preprint UWSEA-PUB-94-07 (electronic archive: astro-ph/9412019), to be published in the proceedings of 22nd Annual SLAC Summer Institute on Particle Physics: Particle Physics, Astrophysics and Cosmology, Stanford, CA, 8-19 August 1994.
48. The Baikal Neutrino Telescope is described by R. Wischnewski, in: NESTOR, Third NESTOR International Workshop, 19-21 October 1993, L.K. Resvanis. ed. (Athens University Press, Athens, 1994) p. 213; R. Wischnewski, in: Neutrino Telescopes, Proceedings of the Fifth International Workshop, Venice, 2-4 March 1993, M. Baldo Ceolin, ed. (University of Padua, Padua, 1993) p. 299; Ch. Spiering, in: TAUP 91, Proceedings of the 2nd International Workshop on Theoretical and Phenomenological Aspects of Underground Physics, Toledo, Spain, 9-13 September 1991, A. Morales, J. Morales and J.A. Villar, eds., Nucl. Phys. B (Proc. Supp.) 28A (1992) 491; see also J. Krabi et al., Sensitivity of the Baikal Neutrino Telescope NT-200 to Point Sources of Very High Energy Neutrinos, Institute for High Energy Physics, Zeuthen preprint PHE 91-13 (unpublished).
49. The Baikal Neutrino Telescope is described by R. Wischnewski, in: NESTOR, Third NESTOR International Workshop, 19-21 October 1993, L.K. Resvanis. ed. (Athens University Press, Athens, 1994) p. 213; R. Wischnewski, in: Neutrino Telescopes, Proceedings of the Fifth International Workshop, Venice, 2-4 March 1993, M. Baldo Ceolin, ed. (University of Padua, Padua, 1993) p. 299; Ch. Spiering, in: TAUP 91, Proceedings of the 2nd International Workshop on Theoretical and Phenomenological Aspects of Underground Physics, Toledo, Spain, 9-13 September 1991, A. Morales, J. Morales and J.A. Villar, eds., Nucl. Phys. B (Proc. Supp.) 28A (1992) 491; see also J. Krabi et al., Sensitivity of the Baikal Neutrino Telescope NT-200 to Point Sources of Very High Energy Neutrinos, Institute for High Energy Physics, Zeuthen preprint PHE 91-13 (unpublished).
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131. Other simulations of the atmospheric neutrino fluxes are in good agreement with the Volkova calculation in the range of interest to us: T.K. Gaisser, T. Stanev and G. Barr, Phys. Rev. D 38 (1988) 85; G. Barr, T.K. Gaisser and T. Stanev, Phys. Rev. D 39 (1989) 3532; V. Agrawal, T.K. Gaisser, P. Lipari and T. Stanev, Bartol preprint BA-95-49 (electronic archive: hep-ph/9509423); A. Butkevich, L.G. Dedenko and I.M. Zheleznyh, Yad. Fiz. 50 (1989) 142 [English transl.: Sov. J. Nucl. Phys. 50 (1989) 90]; K. Mitsui, Y. Minorikawa and H. Komori, Nuovo Cim. 9C (1986) 995; P. Lipari, astropp119593. For a comparison with data, see Fig. 10 of Ref. [12].
132. Other simulations of the atmospheric neutrino fluxes are in good agreement with the Volkova calculation in the range of interest to us: T.K. Gaisser, T. Stanev and G. Barr, Phys. Rev. D 38 (1988) 85; G. Barr, T.K. Gaisser and T. Stanev, Phys. Rev. D 39 (1989) 3532; V. Agrawal, T.K. Gaisser, P. Lipari and T. Stanev, Bartol preprint BA-95-49 (electronic archive: hep-ph/9509423); A. Butkevich, L.G. Dedenko and I.M. Zheleznyh, Yad. Fiz. 50 (1989) 142 [English transl.: Sov. J. Nucl. Phys. 50 (1989) 90]; K. Mitsui, Y. Minorikawa and H. Komori, Nuovo Cim. 9C (1986) 995; P. Lipari, astropp119593. For a comparison with data, see Fig. 10 of Ref. [12].
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