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Modified-gravity wormholes without exotic matter

TLDR
In this article, the authors present the most general conditions in the context of modified gravity, in which the matter threading the wormhole throat satisfies all of the energy conditions, and it is the higher order curvature terms, which may be interpreted as a gravitational fluid, that support these nonstandard wormhole geometries.
Abstract
A fundamental ingredient in wormhole physics is the flaring-out condition at the throat which, in classical general relativity, entails the violation of the null energy condition. In this work, we present the most general conditions in the context of modified gravity, in which the matter threading the wormhole throat satisfies all of the energy conditions, and it is the higher order curvature terms, which may be interpreted as a gravitational fluid, that support these nonstandard wormhole geometries. Thus, we explicitly show that wormhole geometries can be theoretically constructed without the presence of exotic matter but are sustained in the context of modified gravity.

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Modified gravity theories on a nutshell: Inflation, bounce and late-time evolution

TL;DR: In this paper, the authors systematically review some standard issues and also the latest developments of modified gravity in cosmology, emphasizing on inflation, bouncing cosmology and late-time acceleration era.
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Echoes of Kerr-like wormholes

TL;DR: In this paper, the waveform of echoes in static and stationary, traversable wormholes in which perturbations are governed by a symmetric effective potential is studied. But the waveforms are dominated by the wormhole quasinormal frequency nearest to the fundamental black hole frequency that controls the primary signal.
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Shadow of a rotating traversable wormhole

TL;DR: In this article, the authors explore the shadow of rotating traversable wormholes within classical general relativity and compare the results with the case of the Kerr black hole, showing that the shadows for small angular momenta are nearly identical; however, with the increasing of the angular momentum, they start to deviate considerably.
Journal ArticleDOI

Energy conditions in modified gravity

TL;DR: In this paper, generalized energy conditions in modified theories of gravity were considered by taking into account the further degrees of freedom related to scalar fields and curvature invariants, where the curvature terms are grouped in a tensor H a b and a coupling g ( Ψ i ) that can be reorganized in effective Einstein field equations, as corrections to the energymomentum tensor of matter.
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Shadows of rotating wormholes

TL;DR: The results obtained here indicate that, through the observations of their shadows, the wormholes which are considered in this work and have reasonable spin can be distinguished from a black hole.
References
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The classical theory of fields

TL;DR: The principle of relativity Relativistic mechanics Electromagnetic fields electromagnetic waves as discussed by the authors The propagation of light The field of moving charges Radiation of electromagnetic waves Particle in a gravitational field The gravitational field equation
Book

Lorentzian Wormholes: From Einstein to Hawking

Matt Visser
TL;DR: In this article, the authors present a taxonomy of wormhole taxonomies, from wormhole to time machine, and from wormholes to time machines, with a focus on wormholes.
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