Carson et al. 1974

Carson, T.R., D. Ezer, and R. Stothers, 1974: Solar neutrinos and the influence of radiative opacities on solar models. Astrophys. J., 194, 743-744, doi:10.1086/153296.

Use of new radiative opacities based on the hot Thomas-Fermi model of the atom yields a predicted solar meutrino flux which is still considerably larger than the flux observed in Davis's ³⁷Cl experiment.

• Download PDF (Document is 152 kB; scanned, no OCR)
• PDF documents require a special viewer such as the free Adobe Reader.

Citation Styles

Show: ACP, AGU, AMS, ApJ, JQSRT, Science style

Carson, T.R., Ezer, D., and Stothers, R.: Solar neutrinos and the influence of radiative opacities on solar models, Astrophys. J., 194, 743-744, doi:10.1086/153296, 1974.

Carson, T.R., D. Ezer, and R. Stothers (1974), Solar neutrinos and the influence of radiative opacities on solar models, Astrophys. J., 194, 743-744, doi:10.1086/153296.

Carson, T.R., D. Ezer, and R. Stothers, 1974: Solar neutrinos and the influence of radiative opacities on solar models. Astrophys. J., 194, 743-744, doi:10.1086/153296.

Carson, T.R., Ezer, D., & Stothers, R. 1974, Astrophys. J., 194, 743, doi:10.1086/153296.

Carson TR, Ezer D, Stothers R. Solar neutrinos and the influence of radiative opacities on solar models, Astrophys J 1974;194:743-744. doi:10.1086/153296.

T.R. Carson, D. Ezer, R. Stothers, Astrophys. J. 194, 743-744, doi:10.1086/153296 (1974).