Dark Energy or local acceleration?
General Relativity and Quantum Cosmology
2017-08-29 v1
Abstract
We find that an observer with a suitable acceleration relative to the frame comoving whit the cosmic fluid, in the context of the FRW decelerating universe, measures the same cosmological redshift as the LambdaCDM model. The estimated value of this acceleration is beta = 1.4x10^-9m/s^2. The problem of a too high peculiar velocity can be solved assuming, for the observer, a sort of helical motion.
Cite
@article{arxiv.1610.05663,
title = {Dark Energy or local acceleration?},
author = {Antonio Feoli and Elmo Benedetto},
journal= {arXiv preprint arXiv:1610.05663},
year = {2017}
}