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Nonlocal advantage of quantum imaginarity in Schwarzchild spacetime

arXiv Quantum Physics
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⚡ Quantum Brief
Researchers from China examined how Hawking radiation affects quantum imaginarity in Schwarzschild black hole spacetimes, revealing stark differences between accessible and inaccessible regions near event horizons. The study found that nonlocal advantage of quantum imaginarity (NAQI) weakens in physically accessible regions as Hawking temperature rises, potentially disappearing entirely, while remaining absent in inaccessible regions regardless of conditions. Assisted imaginarity distillation shows opposing trends: fidelity decreases with temperature in accessible regions, reducing distillation efficiency, but increases in inaccessible regions, enhancing capability. These findings demonstrate that relativistic effects like Hawking radiation create distinct operational behaviors for quantum resources depending on their location relative to the event horizon. The work bridges quantum information theory and general relativity, offering new insights into quantum phenomena in curved spacetime.
Nonlocal advantage of quantum imaginarity in Schwarzchild spacetime

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Quantum Physics arXiv:2604.03633 (quant-ph) [Submitted on 4 Apr 2026] Title:Nonlocal advantage of quantum imaginarity in Schwarzchild spacetime Authors:Bing Yu, Xiao-Yong Yang, Xiao-Li Hu, Zhi-Xiang Jin, Xiao-Fen Huang View a PDF of the paper titled Nonlocal advantage of quantum imaginarity in Schwarzchild spacetime, by Bing Yu and 4 other authors View PDF HTML (experimental) Abstract:Black hole spacetimes provide a natural setting for quantum systems in curved spacetime, where effects such as Hawking radiation arise from event horizons. In this work, we investigate the impact of the Hawking effect on quantum imaginarity in Schwarzschild spacetime, focusing on nonlocal advantage of quantum imaginarity (NAQI) and assisted imaginarity distillation. For NAQI, it is significantly affected by Hawking radiation, exhibiting a pronounced difference between physically accessible and inaccessible regions. It is suppressed in the physically accessible region with increasing Hawking temperature and may vanish, while remaining absent in the physically inaccessible region across the parameter regime. For assisted imaginarity distillation, the Hawking effect modifies the assisted fidelity in a state-dependent manner. In the physically accessible region, the fidelity generally decreases with increasing temperature, indicating reduced distillation capability, whereas the physically inaccessible region exhibits the opposite monotonic trend, indicating enhanced distillation capability. These results highlight distinct operational behaviors of physically accessible and inaccessible regions under relativistic effects, providing insight into quantum imaginarity in curved spacetime. Comments: Subjects: Quantum Physics (quant-ph); General Relativity and Quantum Cosmology (gr-qc) Cite as: arXiv:2604.03633 [quant-ph] (or arXiv:2604.03633v1 [quant-ph] for this version) https://doi.org/10.48550/arXiv.2604.03633 Focus to learn more arXiv-issued DOI via DataCite (pending registration) Submission history From: Zhixiang Jin [view email] [v1] Sat, 4 Apr 2026 08:07:25 UTC (1,319 KB) Full-text links: Access Paper: View a PDF of the paper titled Nonlocal advantage of quantum imaginarity in Schwarzchild spacetime, by Bing Yu and 4 other authorsView PDFHTML (experimental)TeX Source view license Current browse context: quant-ph new | recent | 2026-04 Change to browse by: gr-qc References & Citations INSPIRE HEP NASA ADSGoogle Scholar Semantic Scholar export BibTeX citation Loading... BibTeX formatted citation × loading... Data provided by: Bookmark Bibliographic Tools Bibliographic and Citation Tools Bibliographic Explorer Toggle Bibliographic Explorer (What is the Explorer?) Connected Papers Toggle Connected Papers (What is Connected Papers?) Litmaps Toggle Litmaps (What is Litmaps?) scite.ai Toggle scite Smart Citations (What are Smart Citations?) Code, Data, Media Code, Data and Media Associated with this Article alphaXiv Toggle alphaXiv (What is alphaXiv?) Links to Code Toggle CatalyzeX Code Finder for Papers (What is CatalyzeX?) DagsHub Toggle DagsHub (What is DagsHub?) GotitPub Toggle Gotit.pub (What is GotitPub?) Huggingface Toggle Hugging Face (What is Huggingface?) ScienceCast Toggle ScienceCast (What is ScienceCast?) Demos Demos Replicate Toggle Replicate (What is Replicate?) Spaces Toggle Hugging Face Spaces (What is Spaces?) Spaces Toggle TXYZ.AI (What is TXYZ.AI?) Related Papers Recommenders and Search Tools Link to Influence Flower Influence Flower (What are Influence Flowers?) Core recommender toggle CORE Recommender (What is CORE?) Author Venue Institution Topic About arXivLabs arXivLabs: experimental projects with community collaborators arXivLabs is a framework that allows collaborators to develop and share new arXiv features directly on our website. Both individuals and organizations that work with arXivLabs have embraced and accepted our values of openness, community, excellence, and user data privacy. arXiv is committed to these values and only works with partners that adhere to them. Have an idea for a project that will add value for arXiv's community? Learn more about arXivLabs. Which authors of this paper are endorsers? | Disable MathJax (What is MathJax?)

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Source: arXiv Quantum Physics