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Hybrid neutron stars among mass gap objects are excluded by twin stars at $1.4\,M_\odot$
We investigate the question whether compact objects in the so-called mass gap ($2.5 < M/M_\odot < 5.0$) can be neutron stars or hybrid stars. Using a generic hybrid star equation of state with a first-order deconfinement transition, we map the allowed parameter space in a Seidov-type diagram and con
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