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dc.contributor.authorAlexeyev, S. O.en
dc.contributor.authorRannu, K. A.en
dc.contributor.authorDyadina, P. I.en
dc.contributor.authorLatosh, B. N.en
dc.contributor.authorTuryshev, S. G.en
dc.date.accessioned2021-08-31T15:03:22Z-
dc.date.available2021-08-31T15:03:22Z-
dc.date.issued2015-
dc.identifier.citationObservational limits on Gauss-Bonnet and Randall-Sundrum gravities / S. O. Alexeyev, K. A. Rannu, P. I. Dyadina, et al. — DOI 10.1134/S1063776115060011 // Journal of Experimental and Theoretical Physics. — 2015. — Vol. 120. — Iss. 6. — P. 966-973.en
dc.identifier.issn10637761-
dc.identifier.otherFinal2
dc.identifier.otherAll Open Access, Green3
dc.identifier.otherhttps://www.scopus.com/inward/record.uri?eid=2-s2.0-84938846672&doi=10.1134%2fS1063776115060011&partnerID=40&md5=836197583f76a0c3a3828da3145aeb0d
dc.identifier.otherhttp://arxiv.org/pdf/1501.04217m
dc.identifier.urihttp://elar.urfu.ru/handle/10995/102371-
dc.description.abstractWe discuss the possibilities of experimental search for the new physics predicted by the Gauss-Bonnet and the Randall-Sundrum theories of gravity. The effective four-dimensional spherically symmetrical solutions of these theories are analyzed. We consider these solutions in the weak-field limit and in the process of the primordial black hole evaporation. We show that the predictions of the discussed models are the same as of general relativity. Hence, current experiments are not applicable for such search, and therefore different methods of observation and higher accuracy are required. © 2015, Pleiades Publishing, Inc.en
dc.format.mimetypeapplication/pdfen
dc.language.isoenen
dc.publisherMaik Nauka-Interperiodica Publishingen
dc.rightsinfo:eu-repo/semantics/openAccessen
dc.sourceJ. Exp. Theor. Phys.2
dc.sourceJournal of Experimental and Theoretical Physicsen
dc.subjectGENERAL RELATIVITYen
dc.subjectNEW PHYSICSen
dc.subjectPRIMORDIAL BLACK HOLESen
dc.subjectRANDALL-SUNDRUMen
dc.subjectRELATIVITYen
dc.titleObservational limits on Gauss-Bonnet and Randall-Sundrum gravitiesen
dc.typeArticleen
dc.typeinfo:eu-repo/semantics/articleen
dc.typeinfo:eu-repo/semantics/publishedVersionen
dc.identifier.rsi23996930-
dc.identifier.doi10.1134/S1063776115060011-
dc.identifier.scopus84938846672-
local.contributor.employeeAlexeyev, S.O., Sternberg Astronomical Institute, Moscow State University, Moscow, 119991, Russian Federation
local.contributor.employeeRannu, K.A., Sternberg Astronomical Institute, Moscow State University, Moscow, 119991, Russian Federation
local.contributor.employeeDyadina, P.I., Physics Department, Moscow State University, Moscow, 119991, Russian Federation
local.contributor.employeeLatosh, B.N., Faculty of Natural and Engineering Science, Dubna International University, Dubna, Moscow oblast, 141980, Russian Federation, Physics Department, Institute for Natural Sciences, Ural Federal University, Yekaterinburg, 620002, Russian Federation
local.contributor.employeeTuryshev, S.G., Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109-0899, United States
local.description.firstpage966-
local.description.lastpage973-
local.issue6-
local.volume120-
dc.identifier.wos000358650800005-
local.contributor.departmentSternberg Astronomical Institute, Moscow State University, Moscow, 119991, Russian Federation
local.contributor.departmentPhysics Department, Moscow State University, Moscow, 119991, Russian Federation
local.contributor.departmentFaculty of Natural and Engineering Science, Dubna International University, Dubna, Moscow oblast, 141980, Russian Federation
local.contributor.departmentPhysics Department, Institute for Natural Sciences, Ural Federal University, Yekaterinburg, 620002, Russian Federation
local.contributor.departmentJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109-0899, United States
local.identifier.purec9a83a54-0e91-4652-b851-587e2f46e350uuid
local.identifier.pure550942-
local.identifier.eid2-s2.0-84938846672-
local.identifier.wosWOS:000358650800005-
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