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- Author: Raymond Davis Jr
- Publisher: CRC Press
- ISBN-10: 0813340373
- ISBN-13: 9780813340371
- Format: 15.2 x 22.9 x 2.8 cm, softcover
- Language: English
- SAVE -10% with code: EXTRA
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Description
A variety of evolutionary sequences of models for the solar interior has been computed, corresponding to variations in input data, to obtain some idea of the uncertainties involved in predicting a solar neutrino flux. It is concluded that the neutrino flux can be estimated to within a factor of 2, the primary uncertainty being the initial homogeneous solar composition; detailed results are given. With a preferred value of the heavy-element-to-hydrogen ratio Z/X = 0.028, the helium content necessary to fit a model to the observed solar luminosity is found to be Y = 0.27.
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- Author: Raymond Davis Jr
- Publisher: CRC Press
- ISBN-10: 0813340373
- ISBN-13: 9780813340371
- Format: 15.2 x 22.9 x 2.8 cm, softcover
- Language: English English
A variety of evolutionary sequences of models for the solar interior has been computed, corresponding to variations in input data, to obtain some idea of the uncertainties involved in predicting a solar neutrino flux. It is concluded that the neutrino flux can be estimated to within a factor of 2, the primary uncertainty being the initial homogeneous solar composition; detailed results are given. With a preferred value of the heavy-element-to-hydrogen ratio Z/X = 0.028, the helium content necessary to fit a model to the observed solar luminosity is found to be Y = 0.27.
Reviews