Neutrinos in Particle Physics and Astrophysics
Conference paper
First Online:
Abstract
Neutrinos, first introduced for theoretical reasons, were discovered long ago, but their main properties have been established rather recently, especially by analyzing the so-called atmospheric and solar neutrinos. Now we know that there are three kinds of neutrinos that, in their propagation, get mixed among themselves through the mechanism of oscillations. In this paper we discuss this phenomenon and the main features of neutrinos; we mention also the neutrinos emitted by supernovae and the relic neutrinos. Neutrino telescopes represent a useful tool for investigating new phenomena both in particle physics and in astrophysics.
Keywords
Neutrino Mass Neutrino Oscillation Solar Neutrino Atmospheric Neutrino Electron Neutrino
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.
Preview
Unable to display preview. Download preview PDF.
References
- 1.Fermi, E. (1934) Tentativo di una teoria dei raggi β, Nuovo Cim. XI, 1–19.CrossRefGoogle Scholar
- 2.Cowan, C., Reines, F., Harrison, F.B., Kruse, H.W. and McGuire, A.D. (1956) Detection of the free neutrino: a confirmation, Science 124, 103–104.CrossRefGoogle Scholar
- 3.Dunby, G. et al. (1962) Observation of high-energy neutrino reactions and the existence of two kinds of neutrinos, Phys. Rev. Lett. 9, 36–44.CrossRefGoogle Scholar
- 4.Pearl, M.L. et al. (1975) Evidence for anomalous lepton production in e+ - e- annihilation, Phys. Rev. Lett. 35, 1489–1492.CrossRefGoogle Scholar
- 5.Kodama, K. et al. (2008) Final tau-neutrino results from the DONuT experiment, Phys.Rev. D78, 052002 (1–37).Google Scholar
- 6.Davis, R. (1964) Solar neutrinos. II.Experimental, Phys. Rev. Lett. 12, 303–305.CrossRefGoogle Scholar
- 7.Hirata, K.S. et al. (1988) Experimental study of the atmospheric neutrino flux, Phys. Lett. B205, 416–420.Google Scholar
- 8.B. Pontecorvo (1957) Inverse beta processes and non conservation of lepton charge, Zh. Eksp. Teor. Fiz.34, 247, Sov. Phys. JETP 7, 172–173.Google Scholar
- 9.Maki, Z. M., Nakagawa, M. and Sakata, S. (1962) Remarks on the unified model of elementary particles, Prog. Theor. Phys. 28, 870–880.CrossRefGoogle Scholar
- 10.Kajita, T. (1999) Atmospheric neutrino results from Super-Kamiokande and Kamiokande – Evidence for νμ oscillations, Neutrino Physics and Astrophysics, Proceedings of the XVIII International Conference on Neutrino Physics and Astrophysics, ed. By Y. Suzuki and Y. Totsuka, Elsevier, Amsterdam, 123–132.Google Scholar
- 11.. Ann, M.H. (2006) Measurement of neutrino oscillations by the K2K experiment, Phys.Rev. D74, 072003 (1–39).Google Scholar
- 12.. sStrumia, A. and Vissani, F. (2008) Neutrino masses and mixing and…, arXiv.org/abs/hep-ph/069 6054 (1–219).Google Scholar
- 13.. J.N. Bahcall, J.N, Basu,S and Pinsonneault, M.H. (2001) Solar models: Current epoch and time dependences, neutrinos, and helioseismological properties. Astrophys. J. 555, 990–1012.Google Scholar
- 14.. McDonald, A.B. (2000) First Neutrino Observations from the Sudbury Neutrino Observatory, Neutrino 2000, Proceedings of the XIXth International Conference on Neutrino Physics and Astrophysics, Sudbury, ed. by J. Law, R.W. Ollerhead and J.J. Simpson, North Holland, 21–28.Google Scholar
- 15.Eguchi, K. et al. (2003) First results from KamLAND: Evidence for reactor antineutrino disappearance, Phys. Rev. Lett. 90, 021802 (1–6).Google Scholar
- 16.Fogli, G.L., Lisi, E., Marrone, A., Palazzo, A. and Rotunno, A.M. (2008) Neutrino masses and mixing, Nucl. Phys. Proc. Suppl. 188, 27–30.CrossRefGoogle Scholar
- 17.Otten, E.W. and Weinheimer, C. (2008) Neutrino mass from tritium beta decay, Rept. Prog. Phys. 71 086201.CrossRefGoogle Scholar
- 18.Bonn, J. (2008) The Karlsruhe tritium neutrino mass experiment KATRIN AIP, Conf. Proc. 972, 404–411.CrossRefGoogle Scholar
- 19.Costa, G. (1997) Unification of the fundamental interactions: problems and perspectives, Spectroscopy and Dynamics of Collective Excitations in Solids, ed. by B. Di Bartolo, Plenum Press, New York, 581–597.Google Scholar
- 20.Goldhaber, M., Grodzins, L. and Sunyar, A.W. (1958) Helicity of neutrinos, Phys. Rev. 109, 1015–1017.CrossRefGoogle Scholar
- 21.. Feruglio, F., Hagedorn, C., Yin Lin and Merlo, L. (2008) Theory of the neutrino mass, Fourth International Workshop on Neutrino Oscillations in Venice, ed. by M. Baldo-Ceolin, Papergraf, Padova, 29–43.Google Scholar
- 22.Fogli, G.L., Lisi, E., Mirizzi, A. and Montanino, D. (2007) Supernova neutrino observation twenty years after SN1987A: status and perspectives, Nuovo Cim. 122B, 573–578.Google Scholar
- 23.. DeYoung, T. (IceCube collaboration) (2009) Recent results from IceCube and AMANDA, arXi/astro-phv:0910.3644.Google Scholar
- 24.Wright, E.L. (2003) COBE observation of the cosmic infrared background, New. Astron. Rev. 48, 465–468.Google Scholar
- 25.Smoot, G.F. (2007) Nobel Lecture: Cosmic microwave background radiation anisotropies: their discoveries and utilization, Rev. Mod. Phys. 79, 1349–1379.CrossRefGoogle Scholar
- 26.Gelmini, G.B. (2005) Prospect for relic neutrino searches, Nobel Symposium 2004: Neutrino Physics, Phys. Scripta T121, 131–136.CrossRefGoogle Scholar
Copyright information
© Springer Science+Business Media B.V. 2011