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Anisotropic bianchi type-ii modified holographic ricci dark energy model in scale-covariant theory of gravitation

dc.contributor.authorRam S.; Chandel S.; Verma M.K.
dc.date.accessioned2025-05-23T11:26:53Z
dc.description.abstractIn this paper, we obtain an anisotropic Bianchi type-II space–time with dark matter and modified holographic Ricci dark energy in the scale-covariant theory of gravitation. Exact solutions of the field equations are obtained by assuming (i) a negative constant value of the deceleration parameter, (ii) the component s11of the shear tensor s ji is proportional to the mean Hubble parameter, and (iii) the gauge function f is proportional to a power function of the average scale factor. We have also discussed some important physical aspects of the model, which is in agreement with the modern cosmological observations. © 2021 The Author(s).
dc.identifier.doihttps://doi.org/10.1139/cjp-2020-0443
dc.identifier.urihttp://172.23.0.11:4000/handle/123456789/10809
dc.relation.ispartofseriesCanadian Journal of Physics
dc.titleAnisotropic bianchi type-ii modified holographic ricci dark energy model in scale-covariant theory of gravitation

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