Abstract

We describe a spacetime endowed with a non-metricity tensor which effectively serves as a model of a spacetime foam. We explore the consequences of the non-metricity in several f(R) theories.

Highlights

  • It has been argued by Wheeler [1, 2] that the spacetime may have a nontrivial structure over small scales

  • This nontrivial structure is characterized by uctuations of the metric and the topology

  • We have proposed an effective description of the spacetime foam in terms of the non-metricity tensor

Read more

Summary

Introduction

It has been argued by Wheeler [1, 2] that the spacetime may have a nontrivial structure over small scales. The topological changes are usually referred to as spacetime defects (or spacetime foam). It is not dif cult to convince oneself that a spacetime with changing topology over small scales is hard to describe or even intractable. It seems, natural to take an effective perspective, where the spacetime foam is described by an intrinsic geometrical property of the spacetime manifold. We add one appendix with technical details about the stability of the solutions

Non-metricity and defects
The single defect case
New action for defects and gravity
Weyl vector and the addition of dynamics
Conservation of energy–momentum tensor
Some cosmological implications
Conclusions
Full Text
Published version (Free)

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call