In Hořava-Lifshitz gravity, fermionic compact objects reach black-hole compactness above a minimum fermion mass, potentially explaining lower-mass-gap detections and serving as cold dark matter.
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Short-range correlations soften neutron-star equations of state with quadratic vector self-interactions but stiffen them with an added fourth-order term, producing corresponding shifts in maximum masses that persist when a dark-matter fluid is included.
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Vanishing Compactness Gap and Fermionic Compact Dark Matter in Ho\v{r}ava-Lifshitz Gravity
In Hořava-Lifshitz gravity, fermionic compact objects reach black-hole compactness above a minimum fermion mass, potentially explaining lower-mass-gap detections and serving as cold dark matter.
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Effects of short-range correlations at high densities on neutron stars with and without DM content: role of the repulsive self-interaction
Short-range correlations soften neutron-star equations of state with quadratic vector self-interactions but stiffen them with an added fourth-order term, producing corresponding shifts in maximum masses that persist when a dark-matter fluid is included.