Pith. sign in

REVIEW 4 cited by

Horava-Lifshitz gravity: a status report

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 1010.3218 v2 pith:IS2BQLLO submitted 2010-10-15 hep-th gr-qc

Horava-Lifshitz gravity: a status report

classification hep-th gr-qc
keywords theorygravityhorava-lifshitzattentionattractedbeenbriefconsistency
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
0 comments
read the original abstract

This is intended to be a brief introduction and overview of Horava-Lifshitz gravity. The motivation and all of the various version of the theory (to date) are presented. The dynamics of the theory are discussed in some detail, with a focus on low energy viability and consistency, as these have been the issues that attracted most of the attention in the literature so far. Other properties of the theory and developments within its framework are also covered, such as: its relation to Einstein-aether theory, cosmology, and future perspectives.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 4 Pith papers

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

  1. Einstein-aether Elliptic Charges and the First Law of Asymptotically AdS Black Holes

    gr-qc 2026-06 unverdicted novelty 6.0

    Einstein-aether theory admits an elliptic charge arising from a symmetry of the reduced action that explains the misalignment contribution to the first law for asymptotically AdS universal horizons.

  2. Metric affine gravity with dynamical chronology protection

    gr-qc 2026-04 unverdicted novelty 6.0

    A new metric-affine gravity toy model dynamically generates a global time function via projective invariance breaking to enforce stable causality, recovering mimetic gravity and yielding a broader dark sector.

  3. Quantizing non-projectable Ho\v{r}ava gravity with Lagrangian path integral

    hep-th 2025-12 unverdicted novelty 6.0

    Develops a Lagrangian path integral formulation for non-projectable Hořava gravity and computes one-loop divergences in (2+1) dimensions, verifying cancellation of linear-in-frequency terms to extract beta functions f...

  4. Space- vs Time-dependence in taming the infrared instability of projectable Ho\v{r}ava Gravity

    hep-th 2026-04 unverdicted novelty 5.0

    Higher-derivative corrections in projectable Hořava gravity do not yield static planar-symmetric solutions that can serve as endpoints for the Minkowski infrared instability.