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dc.contributor.authorOkcu, Ozgur
dc.contributor.authorAydiner, Ekrem
dc.date.accessioned2022-07-04T16:21:53Z
dc.date.available2022-07-04T16:21:53Z
dc.date.issued2022
dc.identifier.citationOkcu O., Aydiner E., "Investigating bounds on the extended uncertainty principle metric through astrophysical tests", EPL, cilt.138, sa.3, 2022
dc.identifier.issn0295-5075
dc.identifier.othervv_1032021
dc.identifier.otherav_e1291a39-6ee6-4509-ab23-6378b7894125
dc.identifier.urihttp://hdl.handle.net/20.500.12627/185052
dc.identifier.urihttps://doi.org/10.1209/0295-5075/ac6976
dc.description.abstractIn this paper, we consider the gravitational tests for the extended uncertainty principle (EUP) metric, which is a large-scale quantum correction to Schwarzschild metric. We calculate gravitational redshift, geodetic precession, Shapiro time delay, precession of Mercury and S2 star's orbits. Using the results of experiments and observations, we obtain the lower bounds for the EUP fundamental length scale L-*. We obtain the smallest bound L-* 9 x 10(-2) m for gravitational redshift, and the largest bound L-* similar to 4 x 10(10) m for the precession of S2's orbit. Copyright (C) 2022 EPLA
dc.language.isoeng
dc.subjectTemel Bilimler
dc.subjectFizik
dc.subjectTemel Bilimler (SCI)
dc.subjectDisiplinlerarası Fizik ve İlgili Bilim ve Teknoloji Alanları
dc.subjectFİZİK, MULTİDİSİPLİNER
dc.titleInvestigating bounds on the extended uncertainty principle metric through astrophysical tests
dc.typeMakale
dc.relation.journalEPL
dc.contributor.departmentİstanbul Teknik Üniversitesi , ,
dc.identifier.volume138
dc.identifier.issue3
dc.contributor.firstauthorID3432193


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