<script type="text/javascript">
<!--
document.write('<div id="oa_widget"></div>');
document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=undefined&type=result"></script>');
-->
</script>

COPY SCRIPT

For further information contact us at helpdesk@openaire.eu

Solar Models and Solar Neutrinos

Name: Solar Models and Solar Neutrinos
Creator: Bahcall, John N.
Keywords: model: solar, talk: Venice 2003/03/11, neutrino: solar, cross section, p nucleus: interaction, Astrophysics (astro-ph), FOS: Physical sciences, beryllium, Astrophysics, nucleus nucleus: nuclear reaction

descriptionPublicationkeyboard_double_arrow_right Article , Preprint , Other literature type , Conference object 01 Jan 2005Embargo end date: 01 Jan 2003 Germany Publisher:World Scientific Pub Co Pte LtdJournal:Neutrino Physics

Authors: Bahcall, John N.;

doi: 10.1142/9789812773906_0006 , 10.1088/0031-8949/2005/t121/006 , 10.48550/arxiv.astro-ph/0310030 , 10.48550/arxiv.hep-ph/0412068

arXiv: http://arxiv.org/abs/astro-ph/0310030 , http://arxiv.org/abs/hep-ph/0412068

Solar Models and Solar Neutrinos

- Summary
- Subjects
- Metrics

Abstract

I summarize 40 years of development of the standard solar model that is used to predict solar neutrino fluxes and then describe the current uncertainties in the predictions. I will also attempt to explain why it took so long, about three and a half decades, to reach a consensus view that new physics is being learned from solar neutrino experiments.

Invited talk at the XXIII Physics in Collisions Conference (PIC03), Zeuthen, Germany, June 2003, 18 pages, LaTeX, 6 eps and ps figures. PSN THAT05

Country

Germany

Related Organizations

Deutsches Elektronen-Synchrotron DESY
Germany
Institute for Advanced Study
United States
Helmholtz Association of German Research Centres
Germany

Keywords

model: solar, talk: Venice 2003/03/11, neutrino: solar, cross section, p nucleus: interaction, Astrophysics (astro-ph), FOS: Physical sciences, beryllium, Astrophysics, nucleus nucleus: nuclear reaction, neutrino: flux, neutrino p: interaction, numerical calculations: interpretation of experiments, High Energy Physics - Phenomenology, High Energy Physics - Phenomenology (hep-ph), chlorine, talk: Zeuthen 2003/06/26, history, neutrino: oscillation, Nuclear Experiment (nucl-ex), Nuclear Experiment

Impact byBIP!

	citations This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).	18
	popularity This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.	Top 10%
	influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).	Average
	impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.	Top 10%