Anisotropic bianchi type-ii modified holographic ricci dark energy model in scale-covariant theory of gravitation
| dc.contributor.author | Ram S.; Chandel S.; Verma M.K. | |
| dc.date.accessioned | 2025-05-23T11:26:53Z | |
| dc.description.abstract | In 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.doi | https://doi.org/10.1139/cjp-2020-0443 | |
| dc.identifier.uri | http://172.23.0.11:4000/handle/123456789/10809 | |
| dc.relation.ispartofseries | Canadian Journal of Physics | |
| dc.title | Anisotropic bianchi type-ii modified holographic ricci dark energy model in scale-covariant theory of gravitation |