Are Standard Solar Models Reliable?
- 13 January 1997
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review Letters
- Vol. 78 (2), 171-174
- https://doi.org/10.1103/physrevlett.78.171
Abstract
The sound speeds of solar models that include element diffusion agree with helioseismological measurements to a rms discrepancy of better than throughout almost the entire Sun. Models that do not include diffusion, or in which the interior of the Sun is assumed to be significantly mixed, are effectively ruled out by helioseismology. Standard solar models predict the measured properties of the Sun more accurately than is required for applications involving solar neutrinos.
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This publication has 37 references indexed in Scilit:
- Transport in the Sun and the Solar Neutrino ProblemPhysical Review Letters, 1996
- Standard neutrino spectrum fromdecayPhysical Review C, 1996
- How well do we (and will we) know solar neutrino fluxes and oscillation parameters?Physical Review D, 1996
- Status of the Solar Neutrino PuzzlePhysical Review Letters, 1995
- Two solar neutrino problemsPhysics Letters B, 1994
- Neutrinos from the Sun: Experimental results confronted with solar modelsPhysical Review D, 1994
- Future solar neutrino spectroscopy and neutrino propertiesPhysics Letters B, 1994
- Astrophysical solutions are incompatible with the solar neutrino dataPhysical Review D, 1994
- New look at the solar neutrino problemPhysical Review Letters, 1993
- Solution of the solar-neutrino problemPhysical Review Letters, 1990