Please use this identifier to cite or link to this item: http://hdl.handle.net/123456789/5040
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dc.contributor.authorGupta, Nitin-
dc.date.accessioned2023-08-22T12:58:57Z-
dc.date.available2023-08-22T12:58:57Z-
dc.date.issued2022-
dc.identifier.citationAnnals of Physics, 443(1), 168941.en_US
dc.identifier.urihttps://doi.org/10.1016/j.aop.2022.168941-
dc.identifier.urihttp://hdl.handle.net/123456789/5040-
dc.descriptionOnly IISER Mohali authors are available in the record.en_US
dc.description.abstractWe study the indirect detection of Cosmological Constant from an open quantum system of interacting spins, weakly interacting with a thermal bath, a massless scalar field minimally coupled with the static de Sitter background, by computing the spectroscopic shifts. By assuming pairwise interaction between spins, we construct states using a generalization of the superposition principle. The corresponding spectroscopic shifts, caused by the effective Hamiltonian of the system due to Casimir Polder interaction, are seen to play a crucial role in predicting a very tiny value of the Cosmological Constant, in the static patch of de Sitter space, which is consistent with the observed value from the Planck measurements of the cosmic microwave background (CMB) anisotropies.en_US
dc.language.isoen_USen_US
dc.publisherScience Directen_US
dc.subjectCosmologyen_US
dc.subjectOpen quantum systemen_US
dc.subjectQuantum entanglementen_US
dc.titleIndirect detection of Cosmological Constant from interacting open quantum systemen_US
dc.typeArticleen_US
Appears in Collections:Research Articles

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