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- W3047022872 abstract "We study the model of Einstein-Maxwell theory minimally coupling to a massive charged self-interacting scalar field, parameterized by the quartic and hexic coupling, labelled by $lambda$ and $beta$, respectively. In the absence of scalar field, there is a class of counterexamples to cosmic censorship. Moveover, we investigate the properties of full nonlinear solution with nonzero scalar field, and argue that, by assuming massive charged self-interacting scalar field with sufficiently large charge above one certain bound, these counterexamples can be removed. In particular, this bound on charge for self-interacting scalar field is no longer equal to the weak gravity bound for free scalar case. In the quartic case, the bounds are below free scalar case for $lambda<0$, while above free scalar case for $lambda>0$. Meanwhile, in the hexic case, the bounds are above free scalar case for both $beta>0$ and $beta<0$." @default.
- W3047022872 created "2020-08-10" @default.
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- W3047022872 date "2021-03-01" @default.
- W3047022872 modified "2023-10-18" @default.
- W3047022872 title "Weak cosmic censorship with self-interacting scalar and bound on charge to mass ratio" @default.
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- W3047022872 doi "https://doi.org/10.1007/jhep03(2021)045" @default.
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