Pith. sign in

REVIEW 1 cited by

New black hole solutions with a dynamical traceless nonmetricity tensor in Metric-Affine Gravity

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 2210.05998 v2 pith:4KCNWMCR submitted 2022-10-12 gr-qc hep-th

classification gr-qchep-th
keywords tensorblackdynamicalgravityholemetric-affinenonmetricityshear
verification ladder T0 review T1 audit T2 compute T3 formal

Signed reviews

No signed human review yet.

0 comments
read the original abstract

In the framework of Metric-Affine Gravity, the existing correspondence between the Einstein tensor and the energy-momentum tensor of matter provided by General Relativity is extended towards a post-Riemannian description in terms of the torsion and nonmetricity fields, which are sourced by the spin, dilation and shear currents of matter. In this work, we focus on the dynamical role of the traceless part of the nonmetricity tensor and its intrinsic connection with shears, defining a model which encloses a new black hole solution endowed with shear charges. We show that the extension in the presence of dynamical torsion and Weyl vector leads to the broadest family of static and spherically symmetric black hole solutions with spin, dilation and shear charges in Metric-Affine Gravity so far.

Discussion (0). Continue with ORCID to comment.

Forward citations

Cited by 1 Pith paper

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

  1. Stability in Cubic Metric-Affine Gravity

    gr-qc 2024-11 conditional novelty 6.0 of 10

    Cubic-order curvature, torsion, and nonmetricity invariants can remove the vector and axial instabilities of quadratic metric-affine gravity and allow Reissner-Nordstrom-like black holes with massive tensor modes.

Pith tools