Schwarzschild-de Sitter black hole as a correlated qubit system via entropic identification

TL;DR

This paper models the thermodynamics of Schwarzschild-de Sitter black holes as a two-qubit correlated system, revealing constraints on quantum correlations influenced by gravity.

Contribution

It introduces a novel approach to represent multi-horizon black holes as correlated qubits using entropic identification, linking gravitational effects to quantum correlations.

Findings

Black hole entropy modeled as entangled qubits

Correlation bounds are more stringent than Araki-Lieb inequality

Reduced density matrices constructed for black hole horizons

Abstract

The thermodynamic behaviours of multi-horizon black holes such as a Schwarzschild-de Sitter black hole have been one of the long-standing mysteries in gravitational physics since they involve quantum natures in gravitational systems and that the search for quantum gravity has not reached its conclusion. In this work, we seeked for a possibility of realising the Schwarzschild-de Sitter black hole as a correlated qubit system, where each of the event horizon is treated as a qubit and both of them are correlated in a way that two qubits could be. By identifying the entropies of subsystems to those of qubits, we successfully constructed the reduced density matrices of the two subsystems as well as the density matrix for the Schwarzschild-de Sitter black hole, modelled as 2-correlating qubits. Moreover, our results suggested that when the gravitational effect has its role in the qubit systems, supposedly like black holes, the correlation between qubits are constrained with a lower bound more stringent than the so-called Araki-Lieb triangle inequality.