Abstract
Ultra high energy cosmic neutrinos may not propagate unattenuated in space over cosmological distances because they can interact with the relic cosmological neutrino background. This process initiates neutrino cascades which provide a possible signature of the background neutrinos and could give rise to the observed cosmic ray flux beyond the GZK cutoff. discuss high energy neutrino propagation in space with special focus on generation and development of neutrino cascades. Analytical estimates as well as numerical investigations are presented to show how this byproduct of high energy neutrino propagation can cause various interesting phenomena in the Universe.
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
Preview
Unable to display preview. Download preview PDF.
Similar content being viewed by others
References
M. Takeda, et al.: Astrophys. J. 522, 225 (1999)
T. J. Weiler: Phys. Rev. Lett. 49, 234 (1982) E. Roulet: Phys. Rev. D 47, 5247 (1993)
S. Yoshida: Astropart. Phys. 2, 187 (1994)
S. Weinberg: Gravitation and Cosmology (Wiley, New York, 1972)
R. W. Strickland, D. N. Schramm: Astrophys. J. 481, 571 (1997)
Y. Fukuda, et al.: Phys. Rev. Lett. 81, 1562 (1998)
S. A. Bludman: Phys. Rev. D 45, 4720 (1992)
A. Sandage, C. Cacciari: Astrophys. J. 350, 645 (1990)
P. Bhattacharjee, C. T. Hill, and D. N. Schramm: Phys. Rev. Lett. 69 (1992) 567.
P. Bhattacharjee and G. Sigl: Phys. Rep. 327, 109 (2000).
S. Yoshida, H. Dai, C. H. Jui, P. Sommers: Astrophys. J. 479, 547 (1997)
G. Sigl, S. Lee, P. Bhattacharjee, S. Yoshida: Phys. Rev. D 59, 043504 (1998)
D. Fargion, B. Mele, A. Salis: Astrophys. J. 517, 725 (1999) T. J. Weiler: Astropart. Phys. 3, 303 (1999)
S. Yoshida, G. Sigl, S. Lee: Phys. Rev. Lett. 81, 5505 (1998)
C. T. Hill: Nucl. Phys. 224B (1983) 469.
P. W. Gorham, K. M. Liewer, C. J. Naudet: astro-ph/9906504, Proc. 26th International Cosmic Ray Conference, (Utah, 1999) P. W. Gorham, et al.: astro-ph/0102435, Proc. First International Workshop on Radio Detection of High-Energy Particles, Amer. Inst. of Phys., 2001, and at http://www.physics.ucla.edu/~moonemp/radhep/workshop.html
M. A. Lawrence, R. J. O. Reid, A. A. Watson: J. Phys. G Nucl. Part. Phys 17, 733 (1991)
D. J. Bird, et al.: Phys. Rev. Lett. 71, 3401 (1993)
M. Takeda, et al.: Phys. Rev. Lett. 81, 1163 (1998)
P. Sreekumar, et al.: Astrophys. J. 494, 523 (1998)
R. M. Baltrusaitis, et al.: Phys. Rev. D 31, 2192 (1985)
For general information see http://amanda.berkeley.edu/ see also F. Halzen: New Astron. Rev 42, 289 (1999) for newest status see, e.g., G. C. Hill, et al. (Amanda Collaboration): astroph/0106064
T. Totani: Mon. Not. R. Astron. Soc. 307, L41 (1999)
E. Waxman, J. N. Bahcall: Phys. Rev. D 59, 023002 (1999)
Author information
Authors and Affiliations
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 2001 Springer-Verlag Berlin Heidelberg
About this chapter
Cite this chapter
Yoshida, S. (2001). Neutrino Cascades: The Byproducts of Propagation of Ultra-High-Energy Neutrinos. In: Lemoine, M., Sigl, G. (eds) Physics and Astrophysics of Ultra-High-Energy Cosmic Rays. Lecture Notes in Physics, vol 576. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-45615-5_10
Download citation
DOI: https://doi.org/10.1007/3-540-45615-5_10
Published:
Publisher Name: Springer, Berlin, Heidelberg
Print ISBN: 978-3-540-42899-2
Online ISBN: 978-3-540-45615-5
eBook Packages: Springer Book Archive