Version: 6.3

Neutrino fluxes from CNO cycle in the Sun in the non stationary case with mixing

Author

A. Kopylov and V. Petukhov

Affiliations

Institute of Nuclear Research of Russian Academy of Sciences, Prospect of 60th Anniversary of October Revolution 7A, 117312 Moscow, Russia

E-mail

beril@al20.inr.troitsk.ru

Journal

Journal of Cosmology and Astroparticle Physics Create an alert RSS this journal

month

Volume 2009, August 2009

Citation

A. Kopylov and V. Petukhov JCAP08(2009)006

doi: 10.1088/1475-7516/2009/08/006


 
Tag this article Full text PDF (504 KB)
Abstract
The calculated deviations of the mean molecular weight and the abundances of hydrogen, helium etc. from the standard values are presented for the non stationary case with mixing of the solar model when the neutrino flux F13 from the decay of 13N is higher than a standard model predicts. The inferences for the future experiments are made, particularly for a lithium radiochemical detector.
Keywords

neutrino experiments

solar and atmospheric neutrinos

PACS

26.65.+t Solar neutrinos

96.50.Vg Energetic particles

96.60.Ly Oscillations and waves; helioseismology

96.60.Vg Particle emission, solar wind

27.20.+n 6(less-than-or-equal-to)A(less-than-or-equal-to)19

96.50.sb Composition, energy spectra and interactions

Subjects

Nuclear physics

Astrophysics and astroparticles

Dates

Issue 08 (August 2009)

Received 16 February 2009 , accepted for publication 15 July 2009

Published 6 August 2009



View by subject


Export




Please login to access our web services, or create an account if you don't yet have one.

You must have cookies enabled in your web browser to be able to login.

Username
Password

Forgotten your password? Get a new one here.