Pith. sign in

REVIEW 2 cited by

Lorentz-Violating Vector Fields Slow the Universe Down

Not yet reviewed by Pith; the record is open.

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv hep-th/0407149 v3 pith:DUM4FUSJ submitted 2004-07-17 hep-th astro-phgr-qchep-ph

classification hep-thastro-phgr-qchep-ph
keywords vectorfielduniverseconstantdensityenergylorentz-violatingnewton
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
read the original abstract

We consider the gravitational effects of a single, fixed-norm, Lorentz-violating timelike vector field. In a cosmological background, such a vector field acts to rescale the effective value of Newton's constant. The energy density of this vector field precisely tracks the energy density of the rest of the universe, but with the opposite sign, so that the universe experiences a slower rate of expansion for a given matter content. This vector field similarly rescales Newton's constant in the Newtonian limit, although by a different factor. We put constraints on the parameters of the theory using the predictions of primordial nucleosynthesis, demonstrating that the norm of the vector field should be less than the Planck scale by an order of magnitude or more.

Discussion (0). Continue with ORCID to comment.

Forward citations

Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Better early than never: A new test for superluminal gravitational wave polarizations

    gr-qc 2025-01 conditional novelty 6.0 of 10

    A backward search in time from known gravitational wave detections could detect or constrain superluminal non-tensor polarizations, and the authors argue this is feasible with current detectors.

  2. Cosmological implications of Bumblebee theory on an FLRW background

    gr-qc 2025-12 unverdicted novelty 3.0 of 10

    Bumblebee theory on an FLRW background yields a cosmological model whose single free parameter is fitted to supernovae observations, producing deceleration and dark energy behaviors that are compared to Lambda-CDM.

Pith tools