Abstract
This article summarizes the theoretical work by Shiv S. Kumar in the years 1958–1963 on very low-mass degenerate objects, which he called “black dwarfs” and which we know today as “brown dwarfs”. He found that there exists a limiting mass below which a contracting star cannot reach the hydrogen-burning main-sequence stage. He predicted that after a warm phase in their early life time objects below this mass cool down and evolve to a completely quantum mechanically degenerate configuration and never go through a normal stellar evolution. After his pioneering theoretical prediction, he had to wait more than 30 years until observations confirmed these ideas.
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Joergens, V. (2014). The Theoretical Prediction of the Existence of Brown Dwarfs by Shiv S. Kumar. In: Joergens, V. (eds) 50 Years of Brown Dwarfs. Astrophysics and Space Science Library, vol 401. Springer, Cham. https://doi.org/10.1007/978-3-319-01162-2_1
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DOI: https://doi.org/10.1007/978-3-319-01162-2_1
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