An analytic approach to the connection between stellar structure parameters and the neutrino emission rate in a simple stellar model

✍ Scribed by H. J. Haubold; A. M. Mathai

• Publisher: John Wiley and Sons
• Year: 1986
• Tongue: English
• Weight: 511 KB
• Volume: 307
• Category: Article
• ISSN: 0004-6337
• DOI: 10.1002/asna.2113070102

✦ Synopsis

In order to obtain the internal structurc of a main-sequence star such as the Suqusually one has to solve the detailed structure equations numerically. This paper is an attempt to construct analytic models for the stellar nuclear energy generation. We give closed-form analytic results for the stellar luminosity and stellar neutrino emissidn rate when the radial matter density of the spherical star under consideration is linear. For thc numerical estimation of the neutrino flux of a specified stellar nuclear reaction we take into account parameters of the standard solar model. The present paper gives for the first time the connection between stellar structure parameters and neutrino fluxes in an analytic stellar model.