New Horizons in Gravity: Dark Energy and Condensate Stars
Emil Mottola

TL;DR
This paper proposes that quantum effects, particularly from the trace anomaly, can replace classical black holes with gravastar configurations, resolving paradoxes and suggesting dark energy may be a large-scale quantum condensate.
Contribution
It introduces a model where quantum vacuum effects create a gravastar instead of a black hole, linking dark energy to a macroscopic quantum condensate.
Findings
Quantum effects can eliminate classical event horizons.
Gravastar models resolve black hole paradoxes.
Dark energy may originate from a cosmological quantum condensate.
Abstract
Black holes are an apparently unavoidable prediction of classical General Relativity, at least if matter obeys the strong energy condition rho + 3p > 0. However quantum vacuum fluctuations generally violate this condition, as does the eq. of state of cosmological dark energy. When quantum effects are considered, black holes lead to a number of thermodynamic paradoxes associated with the Hawking temperature and assumption of black hole entropy, which are briefly reviewed. It is argued that the largest quantum effects arise from the conformal scalar degrees of freedom generated by the trace anomaly of the stress-energy tensor in curved space. At event horizons these can have macroscopically large backreaction effects on the geometry, potentially removing the classical event horizon of black hole and cosmological spacetimes, replacing them with a quantum phase boundary layer, where the…
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