Falsifying cosmological models based on a non-linear electrodynamics

dc.contributor.authorOvgun, Ali
dc.contributor.authorLeon, Genly
dc.contributor.authorMagana, Juan
dc.contributor.authorJusufi, Kimet
dc.date.accessioned2026-02-06T18:51:19Z
dc.date.issued2018
dc.departmentDoğu Akdeniz Üniversitesi
dc.description.abstractRecently, the nonlinear electrodynamics (NED) has been gaining attention to generate primordial magnetic fields in the Universe and also to resolve singularity problems. Moreover, recent works have shown the crucial role of the NED on the inflation. This paper provides a new approach based on a new model of NED as a source of gravitation to remove the cosmic singularity at the big bang and explain the cosmic acceleration during the inflation era on the background of stochastic magnetic field. Also, we found a realization of a cyclic Universe, free of initial singularity, due to the proposed NED energy density. In addition, we explore whether a NED field without or with matter can be the origin of the late-time acceleration. For this we obtain explicit equations for H(z) and perform a MCMC analysis to constrain the NED parameters by using 31 observational Hubble data (OHD) obtained from cosmic chronometers covering the red-shift range 0 < z < 1.97; and with the joint-light-analysis (JLA) SNIa compilation consisting in 740 data points in the range 0.01 < z < 1.2. All our constraints on the current magnetic field give B-0 similar to 10(-31) cm(-1), which are larger than the upper limit 10(-33) cm(-1) by the Planck satellite implying that NED cosmologies could not be suitable to explain the Universe late-time dynamics. However, the current data is able to falsify the scenario at late times. Indeed, one is able to reconstruct the deceleration parameter q(z) using the best fit values of the parameters obtained from OHD and SNIa data sets. If the matter component is not included, the data sets predict an accelerated phase in the early Universe, but a non accelerated Universe is preferred in the current epoch. When a matter component is included in the NED cosmology, the data sets predict a q(z) dynamics similar to that of the standard model. Moreover, both cosmological data favor up to 2 sigma confidence levels an accelerating expansion in the current epoch, i.e., the Universe passes of a decelerated phase to an accelerated stage at redshift similar to 0.6. Therefore, although the NED cosmology with dust matter predict a value B-0 higher than the one measured by Planck satellite, it is able to drive a late-time cosmic acceleration which is consistent with our dynamical systems analysis and it is preferred by OHD and SNIa data sets.
dc.description.sponsorshipChilean FONDECYT Grant [3170035]; FONDECYT Grant [3160674]; Department of Mathematics at Universidad Catolica del Norte
dc.description.sponsorshipThis work was supported by the Chilean FONDECYT Grant No. 3170035 (AO) and FONDECYT Grant No. 3160674 (JM). GL thanks to Department of Mathematics at Universidad Catolica del Norte for warm hospitality and financial support. A. O. is grateful to Prof. Douglas Singleton for hosting him at the California State University, Fresno and also A. O. would like to thank Prof. Leonard Susskind and Stanford Institute for Theoretical Physics for hospitality.
dc.identifier.doi10.1140/epjc/s10052-018-5936-4
dc.identifier.issn1434-6044
dc.identifier.issn1434-6052
dc.identifier.issue6
dc.identifier.orcid0000-0002-9889-342X
dc.identifier.orcid0000-0003-1750-4769
dc.identifier.orcid0000-0002-1152-6548
dc.identifier.scopus2-s2.0-85048287478
dc.identifier.scopusqualityQ1
dc.identifier.urihttps://doi.org/10.1140/epjc/s10052-018-5936-4
dc.identifier.urihttps://hdl.handle.net/11129/15283
dc.identifier.volume78
dc.identifier.wosWOS:000434419800006
dc.identifier.wosqualityQ2
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.language.isoen
dc.publisherSpringer
dc.relation.ispartofEuropean Physical Journal C
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanı
dc.rightsinfo:eu-repo/semantics/openAccess
dc.snmzKA_WoS_20260204
dc.subjectMagnetic-Fields
dc.subjectIntermediate Inflation
dc.subjectDark Energy
dc.subjectLambda
dc.subjectSingularities
dc.subjectParameters
dc.subjectUniverse
dc.titleFalsifying cosmological models based on a non-linear electrodynamics
dc.typeArticle

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