Schwarzschild-like Wormholes in Asymptotically Safe Gravity
arXiv:2108.07912 · doi:10.3390/universe7090332
Abstract
In this paper, we analyze the Schwarzschild-like wormhole in the Asymptotically Safe Gravity(ASG) scenario. The ASG corrections are implemented via renormalization group methods, which, as consequence, provides a new tensor as a source to improved field equations, and promotes the Newton's constant into a running coupling constant. In particular, we check whether the radial energy conditions are satisfied and compare with the results obtained from the usual theory. We show that only in the particular case of the wormhole being asymptotically flat(Schwarzschild Wormholes) that the radial energy conditions are satisfied at the throat, depending on the chosen values for its radius . In contrast, in the general Schwarzschild-like case, there is no possibility of the energy conditions being satisfied nearby the throat, as in the usual case. After that, we calculate the radial state parameter, , in , in order to verify what type of cosmologic matter is allowed at the wormhole throat, and we show that in both cases there is the possibility of the presence of exotic matter, phantom or quintessence-like matter. Finally, we give the solutions for all regions of space. Interestingly, we find that Schwarzschild-like Wormholes with excess of solid angle of the sphere in the asymptotic limit have the possibility of having non-exotic matter as source for certain values of the radial coordinate . Furthermore, it was observed that quantum gravity corrections due the ASG necessarily imply regions with phantom-like matter, both for Schwarzschild and for Schwarzschild-like wormholes. This reinforces the supposition that a phantom fluid is always present for wormholes in this context.
arXiv commentRevised with minor changes and new references.16 pages, 4 figures
References in corpus (60)
- Nonperturbative Evolution Equation for Quantum Gravity
- Renormalization group improved black hole spacetimes
- Phantom energy traversable wormholes
- Fixed points of quantum gravity
- Renormalization Group Flow of Quantum Gravity in the Einstein-Hilbert Truncation
- Wormholes supported by a phantom energy
- Ultraviolet Fixed Point and Generalized Flow Equation of Quantum Gravity
- Morris-Thorne wormholes with a cosmological constant
- Asymptotic safety in higher-derivative gravity
- Non-Trivial Ultraviolet Fixed Point in Quantum Gravity
- The Running Gravitational Couplings
- On the renormalization group flow of f(R)-gravity
- Spacetime Structure of an Evaporating Black Hole in Quantum Gravity
- Asymptotically Safe Lorentzian Gravity
- Asymptotic Safety of Gravity Coupled to Matter
- Renormalization group improved gravitational actions: a Brans-Dicke approach
- Renormalization Group Flow in Scalar-Tensor Theories. I
- Traversable wormholes in Einstein-Dirac-Maxwell theory
- Casimir Wormholes
- Top mass from asymptotic safety
- Quantum Gravity at Astrophysical Distances?
- Running Newton Constant, Improved Gravitational Actions, and Galaxy Rotation Curves
- Traversable Wormholes in General Relativity
- Plane symmetric traversable wormholes in an anti-de Sitter background
- Traversable Wormholes Supported by GUP Corrected Casimir Energy
- Aspects of asymptotic safety for quantum gravity
- A class of nonlocal truncations in Quantum Einstein Gravity and its renormalization group behavior
- Non-minimal coupling in Higgs-Yukawa model with asymptotically safe gravity
- Curvature dependence of quantum gravity
- Dynamical renormalization of black-hole spacetimes
- A proper fixed functional for four-dimensional Quantum Einstein Gravity
- R=0 spacetimes and self-dual Lorentzian wormholes
- Cosmological Perturbations in Renormalization Group Derived Cosmologies
- Asymptotically safe inflation from quadratic gravity
- Dark Matter meets Quantum Gravity
- From renormalization group flows to cosmology
- Quantum Improved Schwarzschild-(A)dS and Kerr-(A)dS Space-times
- Renormalization Group Flow in Scalar-Tensor Theories. II
- Running boundary actions, Asymptotic Safety, and black hole thermodynamics
- as the critical dimensionality of asymptotically safe interactions
- Solutions to the reconstruction problem in asymptotic safety
- Towards conditions for black-hole singularity-resolution in asymptotically safe quantum gravity
- Gravitational collapse in Quantum Einstein Gravity
- Cosmological bounds on the field content of asymptotically safe gravity-matter models
- Cosmic Censorship in Quantum Einstein Gravity
- Bouncing and emergent cosmologies from ADM RG flows
- Self--dual Lorentzian wormholes in n--dimensional Einstein gravity
- Asymptotically Safe Gravity with Fermions
- Functional Renormalization Group flows on Friedman-Lema\^ıtre-Robertson-Walker backgrounds
- Asymptotically anti-de Sitter wormholes
- Traversable Casimir Wormholes in D Dimensions
- Cylindrically and axially symmetric wormholes. Throats in vacuum?
- Scalar-Tensor gravity with system-dependent potential and its relation with Renormalization Group extended General Relativity
- Traversability of quantum improved wormhole solution
- On the cutoff identification and the quantum improvement in asymptotically safe gravity
- Gravitational bending angle with finite distances by Casimir wormholes
- Geodesic congruences in quantum improved spacetimes
- Fixed points and infrared completion of quantum gravity
- Casimir Wormholes in (2+1) Dimensions with Applications to the Graphene
- Ellis-Bronnikov Wormholes in Asymptotically Safe Gravity