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2015

White Dwarf Critical Tests for Modified Gravity

Jain, Rajeev Kumar, Kouvaris, Chris, Nielsen, Niklas Grønlund

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Scalar-tensor theories of gravity can lead to modifications of the gravitational force inside astrophysical objects.

We exhibit that compact stars such as white dwarfs provide a unique set-up to test beyond Horndeski theories of ${\rm G}^3$ type.
We obtain stringent and independent constraints on the parameter $\Upsilon$ characterizing the deviations from Newtonian gravity using the mass-radius relation, the Chandrasekhar mass limit and the maximal rotational frequency of white dwarfs.
We find that white dwarfs impose stronger constraints on $\Upsilon$ than red and brown dwarfs.

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