pith. machine review for the scientific record. sign in

arxiv: 1505.06831 · v3 · submitted 2015-05-26 · 🌀 gr-qc · hep-th

Recognition: unknown

Can extra dimensional effects allow wormholes without exotic matter?

Authors on Pith no claims yet
classification 🌀 gr-qc hep-th
keywords on-branewormholesmattereffectiveenergyconditionexistenceexotic
0
0 comments X
read the original abstract

We explore the existence of Lorentzian wormholes in the context of an effective on-brane, scalar-tensor theory of gravity. In such theories, the timelike convergence condition, which is always violated for wormholes, has contributions, via the field equations,from on-brane matter as well as from an effective geometric stress energy generated by a bulk-induced radion field. It is shown that, for a class of wormholes, the required on-brane matter, as seen by an on-brane observer in the Jordan frame, is not exotic and does not violate the Weak Energy Condition. The presence of the effective geometric stress energy in addition to on-brane matter, is largely responsible for creating this intriguing possibility. Thus, if such wormholes are ever found to exist in the Universe, they would clearly provide pointers towards the existence of a warped extra dimension as proposed in the two-brane model of Randall and Sundrum.

This paper has not been read by Pith yet.

discussion (0)

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

Forward citations

Cited by 2 Pith papers

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

  1. Perturbations in the parametrized wormhole spacetime and their related quasinormal modes

    gr-qc 2026-05 conditional novelty 5.0

    Observationally constrained galactic wormhole models show quasinormal mode damping rates more sensitive to galactic compactness than deformation parameters, while oscillation frequencies remain comparatively stable.

  2. Can wormholes have vanishing Love numbers?

    gr-qc 2026-05 unverdicted novelty 5.0

    For a specific R=0 wormhole, the magnetic Love number for ℓ=2 vanishes to linear order in the regularization parameter under static axial gravitational perturbations.