arXiv · hep-th/9603077
Gravitational Meissner Effect
Abstract
The gravitational analogue of the electromagnetic Meissner effect is investigated. Starting from the post-Newtonian approximation to general relativity we arrive at gravitational London equations, predicting a gravitational Meissner effect. Applied to neutron stars we arrive at a London penetration depth of 12km, which is about the size of a neutron star.
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R. P. Lano. 1996-03-12. Gravitational Meissner Effect. https://arxiv.org/abs/hep-th/9603077
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