Relationship between magnetic field and anisotropy parameter in gravitation theories
dc.authorid | Aktaş, Can / 0000-0002-0603-7862 | |
dc.authorid | Aygün, Sezgin / 0000-0002-2969-4195 | |
dc.contributor.author | Aktaş, Can | |
dc.contributor.author | Aygün, Sezgin | |
dc.contributor.author | Sahoo, Pradyumn Kumar | |
dc.date.accessioned | 2025-01-27T21:00:11Z | |
dc.date.available | 2025-01-27T21:00:11Z | |
dc.date.issued | 2018 | |
dc.department | Çanakkale Onsekiz Mart Üniversitesi | |
dc.description.abstract | The magnetized strange quark matter (MSQM) solutions are obtained for a Marder type universe using constant deceleration parameter. The exact solutions of field equations are obtained for f(R,T) = R 2f(T) model given by [T. Harko et al., Phys. Rev. D 84, 024020 (2011)] with cosmological term. Also, we have obtained General Relativity (GR) solutions for MSQM distributions. For t -> infinity, we get the dark energy model, i.e. p -> -B-c, rho -> B-c and omega = -1. However, for t -> infinity, we find the cosmological constant A as negative in f (R, T) theory and GR. These results agree with [S. Aygun et al., Astrophys. Space Sci. 361, 380 (2016); C. Aktas and S. Aygun, Chinese T. Phys. 55, 71 (2017); P. K. Sahoo et al., Mod. Phys. Lett. A 32, 1750105 (2017)] in f(R,T) theory. The physical consequences of our obtained models are discussed at the end. | |
dc.description.sponsorship | Canakkale Onsekiz Mart University, The Scientific Research Coordination Unit [FBA-2018-1435] | |
dc.description.sponsorship | We thank the anonymous referee for careful reading of the paper and helpful comments and suggestions. This work was supported by Canakkale Onsekiz Mart University, The Scientific Research Coordination Unit, Project No. FBA-2018-1435. | |
dc.identifier.doi | 10.1142/S0217732318501353 | |
dc.identifier.issn | 0217-7323 | |
dc.identifier.issn | 1793-6632 | |
dc.identifier.issue | 24 | |
dc.identifier.scopus | 2-s2.0-85052438588 | |
dc.identifier.scopusquality | Q2 | |
dc.identifier.uri | https://doi.org/10.1142/S0217732318501353 | |
dc.identifier.uri | https://hdl.handle.net/20.500.12428/26958 | |
dc.identifier.volume | 33 | |
dc.identifier.wos | WOS:000440824600001 | |
dc.identifier.wosquality | Q2 | |
dc.indekslendigikaynak | Web of Science | |
dc.indekslendigikaynak | Scopus | |
dc.language.iso | en | |
dc.publisher | World Scientific Publ Co Pte Ltd | |
dc.relation.ispartof | Modern Physics Letters A | |
dc.relation.publicationcategory | info:eu-repo/semantics/openAccess | |
dc.rights | info:eu-repo/semantics/closedAccess | |
dc.snmz | KA_WoS_20250125 | |
dc.subject | Magnetized strange quark matter | |
dc.subject | f(R,T) theory | |
dc.subject | deceleration parameter | |
dc.subject | anisotropy parameter | |
dc.title | Relationship between magnetic field and anisotropy parameter in gravitation theories | |
dc.type | Article |