Results 41 to 50 of about 243,227 (257)

Neutrino mixing and neutrino telescopes [PDF]

Journal of Cosmology and Astroparticle Physics, 2007
Measuring flux ratios of ultra-high energy neutrinos is an alternative method to determine the neutrino mixing angles and the CP phase delta. We conduct a systematic analysis of the neutrino mixing probabilities and of various flux ratios measurable at neutrino telescopes.
openaire   +2 more sources

Stodolsky's Theorem and Neutrino Oscillation Phases -- for pedestrians [PDF]

, 2002
Neutrino oscillations are experimentally observable only as a result of interference between neutrino states with different masses and THE SAME ENERGY.
Lipkin, Harry J.
core   +6 more sources

Thermal neutrinos from pre-supernova [PDF]

, 2006
We would like to discuss prospects for neutrino observations of the core-collapse supernova progenitor during neutrino-cooled stage. We will present new theoretical results on thermal neutrino and antineutrino spectra produced deep inside the pre ...
A. Odrzywolek, Beacom, M. Kutschera, M. Misiaszek, Odrzywolek, Weaver, Woosley   +6 more
core   +3 more sources

Feasibility Study on the Discrimination of Fluor Concentration in the Liquid Scintillator Using PMT Waveform and Short-Pass Filter

Sensors, 2023
Neutrinos are difficult to detect because they weakly interact with matter, making their properties least known. The response of the neutrino detector depends on the optical properties of the liquid scintillator (LS).
Na-Ri Kim, Kyung-Kwang Joo, Hyun-Gi Lee
doaj   +1 more source

Neutrino Opacities in Neutron Stars with Kaon Condensates [PDF]

, 2003
The neutrino mean free paths in hot neutron-star matter are obtained in the presence of kaon condensates. The kaon-induced neutrino absorption process, which is allowed only in the presence of kaon condensates, is considered for both nondegenerate and ...
A. E. Nelson, B. L. Friman, C.-H. Lee, C.-R. Ji, D. B. Kaplan, D. B. Kaplan, D. N. Voskresensky, E. E. Kolomeitsev, G. E. Brown, G. E. Brown, H. Fujii, H. Fujii, H. Fujii, H. Heiselberg, J. A. Pons, J. A. Pons, J. A. Pons, J. M. Lattimer, J. Navarro, M. Christiansen, M. Prakash, M. Prakash, M. Prakash, M. Prakash, M. Takahara, M. Yasuhira, M. Yasuhira, M. Yasuhira, Masatomi Yasuhira, N. Iwamoto, N. K. Glendenning, N. K. Glendenning, Naoki Iwamoto, O. G. Benvenuto, P. Haensel, R. F. Sawyer, R. Niembro, S. Reddy, S. Reddy, S. Reddy, S. Yamada, T. Maruyama, T. Muto, T. Muto, T. Muto, T. Muto, T. Muto, T. Norsen, T. Norsen, T. Takatsuka, T. Takatsuka, T. Tatsumi, T. Tatsumi, T. Tatsumi, T. Tatsumi, T. Tatsumi, T. Tatsumi, T. W. Baumgarte, T. W. Baumgarte, Takumi Muto, Toshitaka Tatsumi, V. Thorsson, W. Keil   +62 more
core   +2 more sources

Progress in neutrino oscillation searches and their implications

, 2003
Neutrino Oscillation, in which a given flavour of neutrino transforms into another is a powerful tool for probing small neutrino masses. The intrinsic neutrino properties involved are neutrino mass squared difference $\Delta m^2$ and the mixing angle in ...
A Bandyopadhyay, A Bandyopadhyay, B T Cleveland, C Athanassopoulos, Ch Berger, Ch. Berger, D Buskulic, D Casper, E A Hawker, E Fiorini, F Terranova, G L Fogli, H Ejiri, H V Klapdor-Kleingrothaus, J N Abdurashitov, J N Bahcall, L Borodovsky, L Wolfenstein, M Agiletta, M Altmann, M Goodman, M Honda, M Maltoni, Q R Ahmad, R Becker-Szendy, S Choubey, S Choubey, S H Ahn, S M Bilenky, S M Bilenky, S P Mikheyev, S T Petcov, S T Petcov, Srubabati Goswami, T K Gaisser, V D Barger, V Paolone, W Hampel, Y Farzan, Y Fukuda, Y Fukuda, Y Fukuda   +41 more
core   +1 more source

Solar Neutrinos Before and After Neutrino 2004 [PDF]

, 2004
We compare, using a three neutrino analysis, the allowed neutrino oscillation parameters and solar neutrino fluxes determined by the experimental data available Before and After Neutrino 2004. New data available after Neutrino2004 include refined KamLAND
Bahcall, John N., Gonzalez-Garcia, M. C., Pena-Garay, Carlos   +2 more
core   +4 more sources

Neutrino and anti-neutrino transport in accretion disks

, 2012
We numerically solve the one dimensional Boltzmann equation of the neutrino and anti-neutrino transport in accretion disks and obtain the fully energy dependent and direction dependent neutrino and anti-neutrino emitting spectra, under condition that the
M. Ruffert, Ye-Fei Yuan, Zhen Pan
core   +1 more source

Neutrinoful universe [PDF]

Journal of High Energy Physics, 2014
The Standard Model of particle physics fails to explain the important pieces in the standard cosmology, such as inflation, baryogenesis, and dark matter of the Universe. We consider the possibility that the sector to generate small neutrino masses is responsible for all of them; the inflation is driven by the Higgs field to break $B-L$ gauge symmetry ...
Higaki, Tetsutaro, Kitano, Ryuichiro, Sato, Ryosuke   +2 more
openaire   +2 more sources

$\nu - K^0$ Analogy, Dirac-Majorana Neutrino Duality and the Neutrino Oscillations

, 2001
The intent of this paper is to convey a new primary physical idea of a Dirac-Majorana neutrino duality in relation to the topical problem of neutrino oscillations.
Bahcall J. N., Caldwell D. O., E. M. LIPMANOV, Eskut E., Fukuda Y., Groom D. E., Pontecorvo B., Proc E.g.   +7 more
core   +2 more sources