The attractor mechanism as a distillation procedure
P\'eter L\'evay, Szil\'ard Szalay

TL;DR
This paper explores the attractor mechanism in black hole solutions through the lens of three-qubit entangled states, revealing how moduli stabilization and entropy relate to quantum state distillation in both BPS and non-BPS cases.
Contribution
It introduces a detailed analysis of the attractor flow as a three-qubit state distillation process, extending previous work to non-BPS solutions and linking quantum entanglement properties to black hole entropy.
Findings
Non-BPS solutions exhibit a transition from complex to GHZ states at the horizon.
The amplitude magnitudes correlate with black hole entropy.
Flat directions cause errors that disrupt the uniform entanglement structure.
Abstract
In a recent paper it has been shown that for double extremal static spherically symmetric BPS black hole solutions in the STU model the well-known process of moduli stabilization at the horizon can be recast in a form of a distillation procedure of a three-qubit entangled state of GHZ-type. By studying the full flow in moduli space in this paper we investigate this distillation procedure in more detail. We introduce a three-qubit state with amplitudes depending on the conserved charges the warp factor, and the moduli. We show that for the recently discovered non-BPS solutions it is possible to see how the distillation procedure unfolds itself as we approach the horizon. For the non-BPS seed solutions at the asymptotically Minkowski region we are starting with a three-qubit state having seven nonequal nonvanishing amplitudes and finally at the horizon we get a GHZ state with merely four…
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