Phenomenology of gravitational aether as a solution to the old cosmological constant problem

Siavash Aslanbeigi, Georg Robbers, Brendan Z. Foster, Kazunori Kohri, and Niayesh Afshordi
Phys. Rev. D 84, 103522 – Published 18 November 2011

Abstract

One of the deepest and most long-standing mysteries in physics has been the huge discrepancy between the observed vacuum density and our expectations from theories of high energy physics, which has been dubbed the old cosmological constant problem. One proposal to address this puzzle at the semiclassical level is to decouple quantum vacuum from spacetime geometry via a modification of gravity that includes an incompressible fluid, known as gravitational aether. In this paper, we discuss classical predictions of this theory along with its compatibility with cosmological and experimental tests of gravity. We argue that deviations from general relativity (GR) in this theory are sourced by pressure or vorticity. In particular, the theory predicts that the gravitational constant for radiation is 33% larger than that of nonrelativistic matter, which is preferred by (most) cosmic microwave background (CMB), Ly-α forest, and Li7 primordial abundance observations, while being consistent with other cosmological tests at 2σ level. It is further shown that all parametrized post-newtonian parameters have the standard GR values aside from the anomalous coupling to pressure ζ4, which has not been directly measured. A more subtle prediction of this model (assuming irrotational aether) is that the (intrinsic) gravitomagnetic effect is 33% larger than GR prediction. This is consistent with current limits from LAGEOS and Gravity Probe B at 2σ level.

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  • Received 20 June 2011

DOI:https://doi.org/10.1103/PhysRevD.84.103522

© 2011 American Physical Society

Authors & Affiliations

Siavash Aslanbeigi1,2,*, Georg Robbers3, Brendan Z. Foster4, Kazunori Kohri5,6, and Niayesh Afshordi1,2,†

  • 1Perimeter Institute for Theoretical Physics, 31 Caroline St. N., Waterloo, ON, N2L 2Y5,Canada
  • 2Department of Physics and Astronomy, University of Waterloo, Waterloo, ON, N2L 3G1, Canada
  • 3Max Planck Institute for Astrophysics, Karl-Schwarzschild-Str. 1, 85741 Garching, Germany
  • 4Foundational Questions Institute, PO Box 3022, New York, New York 10163, USA
  • 5Cosmophysics group, Theory Center, IPNS, KEK, and The University for Advanced Study (Sokendai), Tsukuba 305-0801, Japan
  • 6Department of Physics, Tohoku University, Sendai 980-8578, Japan

  • *saslan4igi@perimeterinstitute.ca
  • nafshordi@perimeterinstitute.ca

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Issue

Vol. 84, Iss. 10 — 15 November 2011

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