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Constraints on axionlike particles and non-Newtonian gravity from measuring the difference of Casimir forces

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dc.contributor.author Klimchitskaya G.
dc.contributor.author Mostepanenko V.
dc.date.accessioned 2018-04-05T07:10:44Z
dc.date.available 2018-04-05T07:10:44Z
dc.date.issued 2017
dc.identifier.issn 2470-0010
dc.identifier.uri http://dspace.kpfu.ru/xmlui/handle/net/130642
dc.description.abstract © 2017 American Physical Society. We derive constraints on the coupling constants of axionlike particles to nucleons and on the Yukawa-type corrections to Newton's gravitational law from the results of recent experiment on measuring the difference of Casimir forces between a Ni-coated sphere and Au and Ni sectors of a structured disc. Over the wide range of axion masses from 2.61 meV to 0.9 eV the obtained constraints on the axion-to-nucleon coupling are up to a factor of 14.6 stronger than all previously known constraints following from experiments on measuring the Casimir interaction. The constraints on non-Newtonian gravity found here are also stronger than all that following from the Casimir- and Cavendish-type experiments over the interaction range from 30 nm to 5.4 μm. They are up to a factor of 177 stronger than the constraints derived recently from measuring the difference of lateral forces. Our constraints confirm previous somewhat stronger limits obtained from the isoelectronic experiment, where the contribution of the Casimir force was nullified.
dc.relation.ispartofseries Physical Review D
dc.title Constraints on axionlike particles and non-Newtonian gravity from measuring the difference of Casimir forces
dc.type Article
dc.relation.ispartofseries-issue 12
dc.relation.ispartofseries-volume 95
dc.collection Публикации сотрудников КФУ
dc.source.id SCOPUS24700010-2017-95-12-SID85022336678


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  • Публикации сотрудников КФУ Scopus [24551]
    Коллекция содержит публикации сотрудников Казанского федерального (до 2010 года Казанского государственного) университета, проиндексированные в БД Scopus, начиная с 1970г.

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