Version: 6.3

Prospects for studying the solar CNO cycle by means of a lithium neutrino detector

Author

A Kopylov and V Petukhov

Affiliations

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

E-mail

beril@al20.inr.troitsk.ru

Journal

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

Issue

Volume 2008, October 2008

Citation

A Kopylov and V Petukhov JCAP10(2008)007

doi: 10.1088/1475-7516/2008/10/007


 
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Abstract

Lithium detectors have a high sensitivity to CNO neutrinos from the Sun. The present experimental data and prospects for future experiments on the detection of CNO neutrinos are discussed. A nonstationary case is considered when the flux of 13N neutrinos is higher than the standard solar model predicts due to the influx of fresh material from the peripheral layers to the solar core.

Keywords

neutrino experiments

solar and atmospheric neutrinos

PACS

96.50.Vg Energetic particles

96.50.sb Composition, energy spectra and interactions

25.40.Lw Radiative capture

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

96.60.Jw Solar interior

96.60.Vg Particle emission, solar wind

Subjects

Nuclear physics

Astrophysics and astroparticles

Dates

Issue 10 (October 2008)

Received 3 June 2008 , accepted for publication 16 September 2008

Published 6 October 2008



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