On rate of Universe expansion
Lennur Ya. Arifov
Abstract
It is offered another method how to describe contemporary stage of the Universe evolution. The method is based upon classical Einstein equations without a dark energy and other hypothetical fields.
Create a lesson
Related papers
Model dependent analytic spin torsion corrections to Blandford Znajek energy extraction in Einstein Cartan gravity
Jingxu Wu, Liangyu Luo, Zhenzhou Lei et al.
Relational GNS Fusion and an Idempotent Gauge-Gravity Fixed Point
G. J. Verbiest
Testing the running vacuum model in light of DESI-DR2 Measurements
Lamiae Kardaddech, Safae Dahmani, Amine Bouali et al.
Reheating after the Higgs Inflation
Manda Malekpour, Kourosh Nozari
Observational viability of Herglotz f(R,T) gravity: A multi-probe Bayesian analysis
Vishal M C, Sankarsan Tarai
Coherent Oscillations of Protons in Hydrogen-loaded Metals
G. Modanese