Hubble tension is routinely presented as a mismatch between the Hubble
constant H_0 determined locally and a value inferred from the flat LCDM
cosmology. In essence, the tension boils down to a disagreement between two
numbers. Here, assuming the tension is cosmological in origin, we predict that
within flat LCDM there should be other inferred values of H_0, and that a
"running of H_0 with redshift" can be expected. These additional determinations
of H_0 may be traced to a difference between the effective equation of state
(EoS) of the Universe and the current standard model. We introduce a diagnostic
that flags such a running of H_0.
Description
[2011.02858] Running Hubble Tension and a H0 Diagnostic
%0 Generic
%1 krishnan2020running
%A Krishnan, Chethan
%A Colgain, Eoin O
%A Sheikh-Jabbari, M. M.
%A Yang, Tao
%D 2020
%K journal_club
%T Running Hubble Tension and a H0 Diagnostic
%U http://arxiv.org/abs/2011.02858
%X Hubble tension is routinely presented as a mismatch between the Hubble
constant H_0 determined locally and a value inferred from the flat LCDM
cosmology. In essence, the tension boils down to a disagreement between two
numbers. Here, assuming the tension is cosmological in origin, we predict that
within flat LCDM there should be other inferred values of H_0, and that a
"running of H_0 with redshift" can be expected. These additional determinations
of H_0 may be traced to a difference between the effective equation of state
(EoS) of the Universe and the current standard model. We introduce a diagnostic
that flags such a running of H_0.
@misc{krishnan2020running,
abstract = {Hubble tension is routinely presented as a mismatch between the Hubble
constant H_0 determined locally and a value inferred from the flat LCDM
cosmology. In essence, the tension boils down to a disagreement between two
numbers. Here, assuming the tension is cosmological in origin, we predict that
within flat LCDM there should be other inferred values of H_0, and that a
"running of H_0 with redshift" can be expected. These additional determinations
of H_0 may be traced to a difference between the effective equation of state
(EoS) of the Universe and the current standard model. We introduce a diagnostic
that flags such a running of H_0.},
added-at = {2020-11-09T07:08:00.000+0100},
author = {Krishnan, Chethan and Colgain, Eoin O and Sheikh-Jabbari, M. M. and Yang, Tao},
biburl = {https://www.bibsonomy.org/bibtex/23136422f91459b5c5acff6e5a842561a/bhvzchhn},
description = {[2011.02858] Running Hubble Tension and a H0 Diagnostic},
interhash = {65e000308c15e61b49bb0c399339c505},
intrahash = {3136422f91459b5c5acff6e5a842561a},
keywords = {journal_club},
note = {cite arxiv:2011.02858Comment: 6 pages, 5 plots},
timestamp = {2020-11-09T07:08:00.000+0100},
title = {Running Hubble Tension and a H0 Diagnostic},
url = {http://arxiv.org/abs/2011.02858},
year = 2020
}