Plasma effects in the solar core and the solar neutrino problem

V.N. Tsytovich; R. Bingham; U. de Angelis; A. Forlani; M.R. Occorsio

doi:10.1016/0927-6505(96)00020-5

Plasma effects in the solar core and the solar neutrino problem

V.N. Tsytovich, R. Bingham, U. de Angelis, A. Forlani, M.R. Occorsio

Research output: Contribution to journal › Article › peer-review

8 Citations (Scopus)

Abstract

In this paper we review recent corrections to the theory of photon transport in a dense hot plasma (similar to conditions in the solar interior) and show that previous calculations overestimate the solar opacity. We also identify new effects which have never been taken into account. It is shown that these can significantly reduce the opacity and can therefore change the prediction of the solar neutrino flux from Standard Solar Models.

Original language	English
Pages (from-to)	197-203
Number of pages	7
Journal	Astroparticle Physics
Volume	5
Issue number	2
DOIs	https://doi.org/10.1016/0927-6505(96)00020-5
Publication status	Published - Aug 1996

Keywords

solar modelling
solar neutrinos
hot plasma
solar neutrino flux

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10.1016/0927-6505(96)00020-5

Cite this

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title = "Plasma effects in the solar core and the solar neutrino problem",

abstract = "In this paper we review recent corrections to the theory of photon transport in a dense hot plasma (similar to conditions in the solar interior) and show that previous calculations overestimate the solar opacity. We also identify new effects which have never been taken into account. It is shown that these can significantly reduce the opacity and can therefore change the prediction of the solar neutrino flux from Standard Solar Models.",

keywords = "solar modelling, solar neutrinos, hot plasma, solar neutrino flux",

author = "V.N. Tsytovich and R. Bingham and Angelis, \{U. de\} and A. Forlani and M.R. Occorsio",

year = "1996",

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AU - Tsytovich, V.N.

AU - Bingham, R.

AU - Angelis, U. de

AU - Forlani, A.

AU - Occorsio, M.R.

PY - 1996/8

Y1 - 1996/8

N2 - In this paper we review recent corrections to the theory of photon transport in a dense hot plasma (similar to conditions in the solar interior) and show that previous calculations overestimate the solar opacity. We also identify new effects which have never been taken into account. It is shown that these can significantly reduce the opacity and can therefore change the prediction of the solar neutrino flux from Standard Solar Models.

AB - In this paper we review recent corrections to the theory of photon transport in a dense hot plasma (similar to conditions in the solar interior) and show that previous calculations overestimate the solar opacity. We also identify new effects which have never been taken into account. It is shown that these can significantly reduce the opacity and can therefore change the prediction of the solar neutrino flux from Standard Solar Models.

KW - solar modelling

KW - solar neutrinos

KW - hot plasma

KW - solar neutrino flux

U2 - 10.1016/0927-6505(96)00020-5

DO - 10.1016/0927-6505(96)00020-5

M3 - Article

SN - 0927-6505

VL - 5

SP - 197

EP - 203

JO - Astroparticle Physics

JF - Astroparticle Physics

IS - 2

ER -

Plasma effects in the solar core and the solar neutrino problem

Abstract

Keywords

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