activity
20102022
most citedGeneration of genuine tripartite entanglement for continuous variables in de Sitter space

22 citations · 67 across the 6 of their papers we have counts for

collaborators

13 papers

gr-qc202213 cited

Generation of quantum coherence for continuous variables between causally disconnected regions in dilaton spacetime

Qinglong Xiao, Cuihong Wen, Jiliang Jing +1

We study the dynamics of Gaussian quantum coherence under the background of a Garfinkle-Horowitz-Strominger dilaton black hole. It is shown that the dilaton field has evident effec…

quant-ph2021

Quantum speedup dynamics process in Schwarzschild space-time

Kai Xu, Han-Jie Zhu, Guo-Feng Zhang +2

Quantum speed limit time (QSLT) can be used to characterize the intrinsic minimal time interval for a quantum system evolving from an initial state to a target state. We investigat…

gr-qc20208 cited

Estimating the Unruh effect via entangled many-body probes

Jieci Wang, Li Zhang, Songbai Chen +1

We study the estimation of parameters in a quantum metrology scheme based on entangled many-body Unruh-DeWitt detectors. It is found that the precision for the estimation of Unruh…

quant-ph20198 cited

Synchronization and estimation of gravity-induced time difference for quantum clocks

Jieci Wang, Tonghua Liu, Jiliang Jing +1

It has recently been reported [\textit{PNAS} \textbf{114}, 2303 (2017)] that, under an operational definition of time, quantum clocks would get entangled through gravitational effe…

gr-qc201922 cited

Generation of genuine tripartite entanglement for continuous variables in de Sitter space

Jieci Wang, Cuihong Wen, Songbai Chen +1

We study the distribution of quantum entanglement for continuous variables among causally disconnected open charts in de Sitter space. It is found that genuine tripartite entanglem…

gr-qc2019

Shadow of a rotating squashed Kaluza-Klein black hole

Fen Long, Jieci Wang, Songbai Chen +1

We study the shadow of a rotating squashed Kaluza-Klein (KK) black hole and the shadow is found to possess distinct properties from those of usual rotating black holes. It is shown…