Results 11 to 20 of about 658,118 (329)
Solar neutrinos: beyond standard solar models [PDF]
After a short survey of the physics of solar neutrinos, giving an overview of hydrogen burning reactions, predictions of standard solar models and results of solar neutrino experiments, we discuss the solar-model-independent indications in favour of non-standard neutrino properties.
V. Castellani +4 more
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Updating standard solar models [PDF]
We present an updated version of our standard solar model (SSM) where helium and heavy elements diffusion is included and the improved OPAL equation of state (Rogers 1994, Rogers Swenson \& Iglesias 1996) is used. In such a way the EOS is consistent with the adopted opacity tables, from the same Livermore group, an occurrence which should further ...
F. Ciacio, S. Degl’Innocenti, B. Ricci
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New results on standard solar models [PDF]
We describe the current status of solar modelling and focus on the problems originated with the introduction of solar abundance determinations with low CNO abundance values. We use models computed with solar abundance compilations obtained during the last decade, including the newest published abundances by Asplund and collaborators.
Aldo M. Serenelli, Aldo M. Serenelli
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LaTex file, 9 pages, 2 figures. Invited talk at Neutrino 98, Tokayama, Japan, June 1998.
John N. Bahcall
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Solar Neutrinos and The Standard Solar Model [PDF]
To appear in the Proceedings of the 1997 ITEP Winter School on particle ...
Arnon Dar
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Reexamination of standard solar model to the solar neutrino problems [PDF]
We examine the calculation of the solar neutrino flux based on the standard solar model (SSM). It is found that the solar neutrino data (KAMIOKANDE experiment) can be well described by the SSM with careful employment of nuclear data of $^7Be (p, ) ^{8} B$.
K. Fukasaku, Tomohiro Fujita
+6 more sources
A Look on Non-Standard Solar Models [PDF]
AbstractA short review of some of the non–standard models proposed in these last two decades is presented. Their main physical assumptions are shown, as well as the way they meet or do not meet the various observational constraints.
A. Maeder
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The Relevance of Nuclear Reactions for Standard Solar Models Construction [PDF]
The fundamental processes by which nuclear energy is generated in the Sun have been known for many years. However, continuous progress in areas such as neutrino experiments, stellar spectroscopy and helioseismic data and techniques requires ever more accurate and precise determination of nuclear reaction cross sections, a fundamental physical input for
F.L. Villante, Aldo Serenelli
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Are Standard Solar Models Reliable? [PDF]
4 pages, latex file. Revised numbers for Table 1.
John N. Bahcall +3 more
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10,000 Standard Solar Models: A Monte Carlo Simulation [PDF]
** John N. Bahcall passed away on August 17, 2005.
John N. Bahcall +2 more
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