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2017

A Vacuum Phase Transition Solves $H_0$ Tension

Di Valentino, Eleonora, Linder, Eric, Melchiorri, Alessandro

Understand

Taking the Planck cosmic microwave background data and the more direct Hubble constant measurement data as unaffected by systematic offsets, the values of the Hubble constant $H_0$ interpreted within the $\Lambda$CDM cosmological constant and cold dark matter cosmological model are in $\sim 3.3 \sigma$ tension.

We show that the Parker vacuum metamorphosis model, physically motivated by quantum gravitational effects and with the same number of parameters as $\Lambda$CDM, can remove the $H_0$ tension, and can give an improved fit to data (up to $\Delta\chi^2=-7.5$).
It also ameliorates tensions with weak lensing data and the high redshift Lyman alpha forest data.
We separately consider a scale dependent scaling of the gravitational lensing amplitude, such as provided by modified gravity, neutrino mass, or cold dark energy, motivated by the somewhat different cosmological parameter estimates for low and high CMB multipoles.

Built on

A.A. Starobinsky, Phys. Lett. B 91, 99 (1980)
1980
Earlier work this paper cites.
L. Parker and A. Raval, Phys. Rev. D 62, 083503 (2000) [arXiv:gr-qc/0003103]
2000
Earlier work this paper cites.
A. Sakharov, Sov. Phys. Dokl. 12, 1040 (1968) [Gen. Rel. Grav. 32, 365 (2000)]
2000
Earlier work this paper cites.
A. Lewis and S. Bridle, Phys. Rev. D 66
2002
Earlier work this paper cites.
E.V. Linder, Phys. Rev. Lett. 90, 091301 (2003) [arXiv:astro-ph/0208512]
2003
Earlier work this paper cites.
L. Parker and D.A.T. Vanzella, Phys. Rev. D 69, 104009 (2004) [arXiv:gr-qc/0312108]
2004
Earlier work this paper cites.
R.R. Caldwell, W. Komp, L. Parker, D.A.T. Vanzella, Phys. Rev. D 73, 023513 (2006) [arXiv:astro-ph/0507622]
2006
Earlier work this paper cites.
R. de Putter, E.V. Linder, JCAP 0810, 042 (2008) [arXiv:0808.0189]
Original
2008
Earlier work this paper cites.
E. Calabrese, A. Slosar, A. Melchiorri, G. F. Smoot and O. Zahn, Phys. Rev. D 77
Original
2008
Earlier work this paper cites.
F. Beutler et al
Original
2011
Earlier work this paper cites.