Other
Scientific paper
Aug 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1269..357a&link_type=abstract
THE 10TH INTERNATIONAL SYMPOSIUM ON ORIGIN OF MATTER AND EVOLUTION OF GALAXIES: OMEG-2010. AIP Conference Proceedings, Volume 1
Other
Neutrino, Neutrino Oscillations, Nucleosynthesis, Stellar Evolution, Normalising, Neutrino, Muon, Pion, And Other Elementary Particles, Cosmic Rays, Neutrino Mass And Mixing, Stellar Structure, Interiors, Evolution, Nucleosynthesis, Ages, Black Holes, Spectroscopic Factors And Asymptotic Normalization Coefficients
Scientific paper
Current ideas on neutrino oscillation plus confirmation from neutrino experiments make possible the changing of neutrino flavor due to interactions with the electrons in medium. When neutrinos pass through a medium and interact with the electrons, an effective potential energy is produced due to coherent forward scattering that occurred in the medium. This potential engenders significant changes in the neutrino masses and their mixing in the medium. Thus electron neutrinos would oscillate into different mass eigenstate and this is dependent on the energy of the neutrinos. Some of the energy will be lost in the coherent scattering with the electrons by the charged current interaction. We have calculated the energy loss of the neutrinos by using a stopping power equation for a 20Msolar star.
Ahmad Nor Sofiah
Kassim Hasan Abu
Yusof Norhasliza
No associations
LandOfFree
Energy Loss of Neutrinos in 20Msolar Star does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Energy Loss of Neutrinos in 20Msolar Star, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Energy Loss of Neutrinos in 20Msolar Star will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1862646