Standard Solar Models
نویسنده
چکیده
A lot of progress has been made in understanding the robustness of solar model predictions since Neutrino 96 [1]. In this talk, I will first summarize the new ingredients and then give the current best-estimates. Then I will discuss the uncertainties in the predictions. Many of the results given here are adopted from the recent BP98 paper [2]. As we shall see in Section 3, there is excellent agreement between standard solar models calculated by different groups with different codes. If you want to obtain the numerical data that are discussed in this talk, you can copy them from my Web site: http://www.sns.ias.edu/∼jnb .
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