Results 41 to 50 of about 41,366 (209)

Current Status of the Resonant Spin-Flavor Precession Solution to the Solar Neutrino Problem [PDF]

open access: yes, 1999
We discuss the current status of the resonant spin-flavor precession (RSFP) solution to the solar neutrino problem. We perform a fit to all the latest solar neutrino data for various assumed magnetic field profiles in the sun.
Adelberger   +55 more
core   +2 more sources

Solar Neutrinos Before and After Neutrino 2004 [PDF]

open access: yes, 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.   +2 more
core   +4 more sources

Solar mass-varying neutrino oscillations [PDF]

open access: yes, 2005
We propose that the solar neutrino deficit may be due to oscillations of mass-varying neutrinos (MaVaNs). This scenario elucidates solar neutrino data beautifully while remaining comfortably compatible with atmospheric neutrino and K2K data and with ...
Danny Marfatia   +4 more
core   +2 more sources

On Stellar Evolution in a Neutrino Hertzsprung–Russell Diagram

open access: yesThe Astrophysical Journal, 2020
We explore the evolution of a select grid of solar metallicity stellar models from their pre-main-sequence phase to near their final fates in a neutrino Hertzsprung–Russell diagram, where the neutrino luminosity replaces the traditional photon luminosity.
Ebraheem Farag   +4 more
doaj   +1 more source

The Charged Neutrino: A New Approach to the Solar Neutrino Problem

open access: yes, 1994
We have considered the effect of the reduction of the solar neutrino flux on earth due to the deflection of the charged neutrino by the magnetic field of the solar convective zone.
Ignatiev, A. Yu., Joshi, G. C.
core   +2 more sources

Linking solar and long baseline terrestrial neutrino experiments [PDF]

open access: yes, 1999
We show that in the framework of three light neutrino species with hierarchical masses and assuming no fine tuning between the entries of the neutrino mass matrix, one can use the solar neutrino data to obtain information on the element $U_{e3}$ of the ...
A. De Rújula   +16 more
core   +2 more sources

Solar Models and Solar Neutrinos [PDF]

open access: yesNeutrino Physics, 2005
Invited talk at the XXIII Physics in Collisions Conference (PIC03), Zeuthen, Germany, June 2003, 18 pages, LaTeX, 6 eps and ps figures.
openaire   +3 more sources

A New Method for Probabilistic Spatiotemporal Forecasts of Solar Soft X‐Ray “S‐Class” (>X10) Superflares

open access: yesJournal of Geophysical Research: Space Physics, Volume 131, Issue 2, February 2026.
Abstract Solar superflares of S‐class (>X10 in soft X‐rays) pose extreme space weather hazards, yet their prediction remains a fundamental challenge owing to their rapid and transient natures and the limitations of conventional event‐based forecasts. We introduce for the first time, a probabilistic spatiotemporal framework designed to identify extended
V. M. Velasco Herrera   +12 more
wiley   +1 more source

Solar Neutrino Observables Sensitive to Matter Effects

open access: yesAdvances in High Energy Physics, 2012
We discuss constraints on the coefficient AMSW which is introduced to simulate the effect of weaker or stronger matter potential for electron neutrinos with the current and future solar neutrino data.
H. Minakata, C. Peña-Garay
doaj   +1 more source

The possibility to observe the non-standard interaction by the Hyperkamiokande atmospheric neutrino experiment

open access: yesNuclear Physics B, 2017
It was suggested that a tension between the mass-squared differences obtained from the solar neutrino and KamLAND experiments can be solved by introducing the non-standard flavor-dependent interaction in neutrino propagation. In this paper we discuss the
Shinya Fukasawa, Osamu Yasuda
doaj   +1 more source

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