dorsal/arxiv
View SchemaA General Relativistic Generalization of Bell Inequality
| Authors | Vladan Pankovic |
|---|---|
| Categories | |
| ArXiv ID | quant-ph/0506129 |
| URL | https://arxiv.org/abs/quant-ph/0506129 |
Abstract
In this work a general relativistic generalization of Bell inequality is suggested. Namely,it is proved that practically in any general relativistic metric there is a generalization of Bell inequality.It can be satisfied within theories of local (subluminal) hidden variables, but it cannot be satisfied in the general case within standard quantum mechanical formalism or within theories of nonlocal (superluminal) hidden variables. It is shown too that within theories of nonlocal hidden variables but not in the standard quantum mechanical formalism a paradox appears in the situation when one of the correlated subsystems arrives at a Schwarzschild black hole. Namely, there is no way that black hole horizon obstructs superluminal influences between spin of the subsystem without horizon and spin of the subsystem within horizon,or simply speaking,there is none black hole horizon nor "no hair" theorem for subsystems with correlated spins. It implies that standard quantum mechanical formalism yields unique consistent and complete description of the quantum mechanical phenomenons.
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"abstract": "In this work a general relativistic generalization of Bell inequality is\nsuggested. Namely,it is proved that practically in any general relativistic\nmetric there is a generalization of Bell inequality.It can be satisfied within\ntheories of local (subluminal) hidden variables, but it cannot be satisfied in\nthe general case within standard quantum mechanical formalism or within\ntheories of nonlocal (superluminal) hidden variables. It is shown too that\nwithin theories of nonlocal hidden variables but not in the standard quantum\nmechanical formalism a paradox appears in the situation when one of the\ncorrelated subsystems arrives at a Schwarzschild black hole. Namely, there is\nno way that black hole horizon obstructs superluminal influences between spin\nof the subsystem without horizon and spin of the subsystem within horizon,or\nsimply speaking,there is none black hole horizon nor \"no hair\" theorem for\nsubsystems with correlated spins. It implies that standard quantum mechanical\nformalism yields unique consistent and complete description of the quantum\nmechanical phenomenons.",
"arxiv_id": "quant-ph/0506129",
"authors": [
"Vladan Pankovic"
],
"categories": [
"quant-ph"
],
"title": "A General Relativistic Generalization of Bell Inequality",
"url": "https://arxiv.org/abs/quant-ph/0506129"
},
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