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In this paper, we explore the properties of white dwarfs with the modified TOV equation in Einstein-$\Lambda$ gravity, the equilibrium configurations predict a maximum mass limit for white dwarfs same as the Chandrasekhar limit when we consider $\Lambda$ to be very small($\Lambda<10^{-16}$ m$^{-2}$), by increasing $\Lambda$, the maximum mass and radius of white dwarf are reduced.
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2016
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G. H. Bordbar, S. H. Hendi, B. Eslam Panah, Neutron stars in Einstein- Λ \Lambda gravity: the cosmological constant effects , Eur. Phys. J. Plus 131
2016
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2016
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2017
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2017
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