Rough initial data for the spherically symmetric Einstein-Maxwell-scalar field system with a positive cosmological constant trigger mass inflation at the Cauchy horizon for every sub-extremal Reissner-Nordstrom-de Sitter black hole.
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Mass inflation from rough initial data for the spherically symmetric Einstein-Maxwell-scalar field system with $\Lambda$
Rough initial data for the spherically symmetric Einstein-Maxwell-scalar field system with a positive cosmological constant trigger mass inflation at the Cauchy horizon for every sub-extremal Reissner-Nordstrom-de Sitter black hole.