Velocity distribution of high-energy particles and the solar neutrino problem

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dc.creatorLiu, Jian-Miin
dc.date2001-08-18
dc.date.accessioned2026-07-07T01:59:41Z
dc.date.available2026-07-07T01:59:41Z
dc.descriptionHigh energy infers high velocity and high velocity is a concept of special relativity. The Maxwellian velocity distribution is corrected to be consistent with special relativity. The corrected distribution reduces to the Maxwellian distribution for small velocities, contains a relatively depleted high-energy tail and vanishes at the velocity of light. This corrected distribution will lower solar neutrino fluxes and change solar neutrino energy spectra but keep solar sound speeds.
dc.description5 pages, no figures
dc.identifierhttps://arxiv.org/abs/astro-ph/0108304
dc.identifierhttp://arxiv.org/abs/astro-ph/0108304
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/3212
dc.subjectAstrophysics
dc.titleVelocity distribution of high-energy particles and the solar neutrino problem
dc.typetext

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