Neutrino masses in astroparticle physics - MPP Theory Group

708 G.G. Raffelt / New Astronomy Reviews 46 (2002) 699–708Loredo, T.J., Lamb, D.Q., 1989. Neutrino from SN 1987A: Strumia, A.. Interpreting the LSND anomaly: Sterile neutrinos orImplications for cooling of the nascent neutron star and the CPT-violation or . . . ?, hep-ph/0201134 [Phys. Lett. B 539,mass of the electron anti-neutrino. Ann. N.Y. Acad. Sci. 571, 91].601. Tayloe, R. MiniBooNE: Status and Plans, Talk at Neutrino 2002,Loredo, T.J., Lamb, D.Q., 2002. Bayesian analysis of neutrinos for transparencies see http://neutrino2002.ph.tum.de/observed from supernova SN 1987A. PhRvD 65, 063002, Totani, T., 1998. Electron neutrino mass measurement by super-[astro-ph/0107260].nova neutrino bursts and implications on hot dark matter.Lunardini, C., Smirnov, A.Y., 2001. High-energy neutrino conver- PhRvL 80, 2039, [astro-ph/9801104].sion and the lepton asymmetry in the universe. PhRvD 64, Tremaine, S., Gunn, J.E., 1979. Dynamical role of light neutral073006, [hep-ph/0012056]. leptons in cosmology. PhRvL 42, 407.Nishikawa, K., 2002. K2K Results, Talk at Neutrino 2002, for Weiler, T.J., 1999. Cosmic ray neutrino annihilation on relictransparencies see http://neutrino2002.ph.tum.de/neutrinos revisited: A mechanism for generating air showersOsipowicz, A. et al. (KATRIN Collaboration). KATRIN: A next above the Greisen–Zatsepin–Kuzmin cut-off. APh 11, 303,generation tritium beta decay experiment with sub-eV sensitivi- [hep-ph/9710431].ty for the electron neutrino mass, hep-ex/0109033.Weinheimer, C. et al., 1999. High precision measurement of thePastor, S., Raffelt, G.G., Semikoz, D.V., 2002. Physics of tritium beta spectrum near its endpoint and upper limit on thesynchronized neutrino oscillations caused by self-interactions. neutrino mass. Phys. Lett. B 460, 219.PhRvD 65, 053011, [hep-ph/0109035].Weinheimer, C., 2002. Direct neutrino mass experiments: PresentSamuel, S., 1993. Neutrino oscillations in dense neutrino gases. and future, Talk at Neutrino 2002, for transparencies seePhRvD 48, 1462.http://neutrino2002.ph.tum.de/Sciama, D.W., 1998. Updated parameters for the decaying neutrino White, S.D.M., Frenk, C.S., Davis, M., 1983. Clustering in atheory and EURD observations of the diffuse UV background. neutrino-dominated universe. Astrophys. J. Lett. 274, L1.A&A 335, 12, [astro-ph/9709243].Wong, Y.Y., 2002. Analytical treatment of neutrino asymmetryShirai, J., 2002. Start of Kamland, Talk at Neutrino 2002, for equilibration from flavour oscillations in the early universe,transparencies see http://neutrino2002.ph.tum.de/ hep-ph/0203180 [PhRvD66, 025015].Sigl, G., 2001. Ultrahigh-energy cosmic rays: A probe of physicsand astrophysics at extreme energies. Science 291, 73, [astroph/0104291].