Quantum Fisher Information in Curved Spacetime: Dirac Particles in Noisy Channels around a Schwarzschild Black Hole
Cookey Iyen, Muhammad Sanusi Liman, Benedict O. Ayomanor, Emem-obong Solomon James, Yame Mwanzang Philemon, Babatunde James Falaye

TL;DR
This paper investigates how quantum Fisher information behaves for entangled Dirac particles in curved spacetime near a Schwarzschild black hole, revealing that squeezing can mitigate noise effects and enhance quantum parameter estimation.
Contribution
It introduces an analysis of QFI dynamics under noisy channels in curved spacetime, highlighting the protective role of squeezing against decoherence in relativistic quantum systems.
Findings
QFI with respect to θ becomes resistant to Hawking temperature at high squeezing.
QFI decay is slower with increased squeezing, indicating error mitigation.
QFI with respect to φ shows transient spikes unaffected by Hawking temperature.
Abstract
Quantum information processing promises significant advantages over classical methods but remains vulnerable to decoherence induced by environmental interactions and spacetime effects. This work investigates the behavior of Quantum Fisher Information (QFI) as a diagnostic tool for entanglement and parameter estimation in a three-qubit entangled Dirac system subjected to dissipative noisy channels in the curved spacetime of a Schwarzschild black hole. In particular, we examine the influence of the squeezed generalized amplitude damping (SGAD) channel, along with its subchannels -- generalized amplitude damping (GAD) and amplitude damping (AD) -- on the QFI with respect to entanglement weight () and phase () parameters. Our results show that under strong squeezing (), the QFI with respect to becomes completely resistant to variations in the Hawking…
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