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• W2000741943 abstract "We perform a Bayesian grid-based analysis of the solar l = 0, 1, 2 and 3 p modes obtained via BiSON in order to deliver the first Bayesian asteroseismic analysis of the solar composition problem. We do not find decisive evidence to prefer either of the contending chemical compositions, although the revised solar abundances (AGSS09) are more probable in general. We do find indications for systematic problems in standard stellar evolution models, unrelated to the consequences of inadequate modelling of the outer layers on the higher order modes. The seismic observables are best fitted by solar models that are several hundred million years older than the meteoritic age of the Sun. Similarly, meteoritic age calibrated models do not adequately reproduce the observed seismic observables. Our results suggest that these problems will affect any asteroseismic inference that relies on a calibration to the Sun." @default.
• W2000741943 created "2016-06-24" @default.
• W2000741943 creator A5025013267 @default.
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• W2000741943 date "2013-04-12" @default.
• W2000741943 modified "2023-10-14" @default.
• W2000741943 title "Bayesian seismology of the Sun" @default.
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• W2000741943 doi "https://doi.org/10.1093/mnras/stt477" @default.
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