Early evolutionary tracks of low-mass stellar objects in modified gravity. (arXiv:2007.13451v2 [gr-qc] UPDATED)
<a href="http://arxiv.org/find/gr-qc/1/au:+Wojnar_A/0/1/0/all/0/1">Aneta Wojnar</a>
Using a simple model of low-mass stellar objects we have shown modified
gravity impact on their early evolution, such as Hayashi tracks, radiative core
development, effective temperature, masses, and luminosities. We have also
suggested that the upper mass’ limit of fully convective stars on the Main
Sequence might be different than commonly adopted.
Using a simple model of low-mass stellar objects we have shown modified
gravity impact on their early evolution, such as Hayashi tracks, radiative core
development, effective temperature, masses, and luminosities. We have also
suggested that the upper mass’ limit of fully convective stars on the Main
Sequence might be different than commonly adopted.
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