The effect of screening factors and thermonuclear reaction rates in the pre-main sequence evolution of low mass stars

Details The effect of screening factors and thermonuclear reaction rates in the pre-main sequence evolution of low mass stars The effect of screening factors and thermonuclear reaction rates in the pre-main sequence evolution of low mass stars

Sep 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010japa...31..135k&link_type=abstract

Journal of Astrophysics and Astronomy, Volume 31, Issue 3, pp.135-145

Astronomy and Astrophysics

Astrophysics

Low Mass Stars, Thermonuclear Reaction Rates, Electron Screening Factors, Composition Changes

Scientific paper

In understanding the nucleosynthesis of the elements in stars, one of the most important quantities is the reaction rate and it must be evaluated in terms of the stellar temperature T, and its determination involves the knowledge of the excitation function σ( E) of the specific nuclear reaction leading to the final nucleus. In this paper, the effect of thermonuclear reaction rates to the pre-main sequence evolution of low mass stars having masses 0.7, 0.8, 0.9 and 1M&sun; are studied by using our modified Stellar Evolutionary Program.

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