# Quantum speed limit time for the damped Jaynes-Cummings and Ohmic-like dephasing models in Schwarzschild spacetime

## TL;DR

This paper investigates how relativistic effects in Schwarzschild spacetime influence the quantum speed limit time for damped Jaynes-Cummings and Ohmic-like dephasing models, highlighting the role of Hawking radiation and quantum coherence.

## Contribution

It analyzes the impact of relativistic effects on quantum speed limits in curved spacetime for specific open quantum system models, considering Hawking radiation influence.

## Key findings

- Quantum coherence is affected by Hawking radiation.
- Speed limit time decreases with distance in Jaynes-Cummings model.
- Speed limit time increases with distance in Ohmic-like dephasing model.

## Abstract

Quantum theory sets the bound on the minimal evolution time between initial and final states of the quantum system. This minimal evolution time can be used to specify the maximal speed of the evolution in open and closed quantum systems. Quantum speed limit is one of the interesting issue in the theory of open quantum systems. One may investigate the influence of the relativistic effect on the quantum speed limit time. When several observers are placed in different inertial or non-inertial frames, or in Schwarzschild space-time, the relativistic effect should be taken into account. In this work, the quantum speed limit time in Schwarzschild space-time will be studied for two various model consist of damped Jaynes-Cummings and Ohmic-like dephasing. First, it will be observed that how quantum coherence is affected by Hawking radiation. According to the dependence of quantum speed limit time on quantum coherence and the dependence of quantum coherence on relative distance of quantum system to event horizon $R_{0}$, it will be represented that the quantum speed limit time in Schwarzschild space-time is decreased by increasing $R_{0}$ for damped Jaynes-Cummings model and conversely, It is increased by increasing $R_{0}$ for Ohmic-like dephasing model .