A horizonless gravastar with a mock horizon emerges from the Tolman-Oppenheimer-Volkoff equations if matter at high pressure transitions to a negative energy-density state.
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Black hole mimickers as relativistic stars calculated from the Tolman-Oppenheimer-Volkoff equations
A horizonless gravastar with a mock horizon emerges from the Tolman-Oppenheimer-Volkoff equations if matter at high pressure transitions to a negative energy-density state.