<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

Open Questions in Stellar Nuclear Physics: I

Name: Open Questions in Stellar Nuclear Physics: I
Creator: Moshe Gai
Keywords: Nuclear Theory (nucl-th), High Energy Physics - Phenomenology, High Energy Physics - Phenomenology (hep-ph), Nuclear Theory, 13. Climate action, Astrophysics (astro-ph), 0103 physical sciences, FOS: Physical sciences, 14. Life underwater, Astrophysics

descriptionPublicationkeyboard_double_arrow_right Article , Preprint , Other literature type 01 Jan 2004Embargo end date: 01 Jan 2004Publisher:AIPJournal:AIP Conference Proceedings, volume 726, pages 109-110 (issn: 0094-243X,

Authors: Moshe Gai;

doi: 10.1063/1.1805924 , 10.1063/1.1805945 , 10.48550/arxiv.astro-ph/0405100

arXiv: http://arxiv.org/abs/astro-ph/0405100

Open Questions in Stellar Nuclear Physics: I

- Summary
- Subjects
- Metrics

Abstract

No doubt, among the most exciting discoveries of the third millennium thus far are {\bf Oscillations of Massive Neutrinos} and {\bf Dark Energy} that leads to an accelerated expansion of the Universe. Accordingly, Nuclear Physics is presented with two extraordinary challenges: the need for precise (5% or better) prediction of solar neutrino fluxes within the Standard Solar Model, and the need for an accurate (5% or better) understanding of stellar evolution and in particular of Type Ia super nova that are used as cosmological standard candle. In contrast, much confusion is found in the field with contradicting data and strong statements of accuracy that can not be supported by current data. We discuss an experimental program to address these challenges and disagreements.

Work Supported by USDOE Grant No. DE-FG02-94ER40870. To appear in StuFiesta, Cocoyoc, Mexico, April 19-22, 2004

Related Organizations

University of Connecticut
United States

Keywords

Nuclear Theory (nucl-th), High Energy Physics - Phenomenology, High Energy Physics - Phenomenology (hep-ph), Nuclear Theory, Astrophysics (astro-ph), FOS: Physical sciences, Astrophysics

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).	1
	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.	Average
	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.	Average