Traversable wormhole solutions with non-exotic fluid in framework of f(Q) gravity

نویسندگان

چکیده

The presence of exotic matter for the existence wormhole geometry has been an unavoidable problem in GR. In recent studies researchers have tried to deal with this issue using modified gravity theories where WH is explained by extra curvature terms and NEC's are not violated signifying standard geometry. present article we trying find solutions traversable wormholes normal throat within framework symmetric teleparallel $f(Q)$ $Q$ non metricity scalar which defines gravitational interaction. We will examine geometries three forms function $f(Q)$. First linear form $f(Q)=\alpha Q$, second a -linear Q^2 + \beta$ third one more general quadratic \beta Q \gamma$ $\alpha$, $\beta$ $\gamma$ being constants. For all cases shape taken as $b(r) = {\frac{r_{0}\ln(r+1)}{\ln({r_0}+1)}}$ $r_0$ radius. A special variable redshift considered discussion. All energy conditions then examined stability

برای دانلود باید عضویت طلایی داشته باشید

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

The traversable wormhole with classical scalar fields

We study the Lorentzian static traversable wormholes coupled to quadratic scalar fields. We also obtain the solutions of the scalar fields and matters in the wormhole background and find that the minimal size of the wormhole should be quantized under the appropriate boundary conditions for the positive nonminimal massive scalar field.

متن کامل

Self-consistent Wormhole Solutions of Semiclassical Gravity

We present the first results of a self-consistent solution of the semiclassical Einstein field equations corresponding to a Lorentzian wormhole coupled to a quantum scalar field. The specific solution presented here represents a wormhole connecting two asymptotically spatially flat regions. In general, the diameter of the wormhole throat, in units of the Planck length, can be arbitrarily large,...

متن کامل

Quantum field theory constrains traversable wormhole geometries.

Recently a bound on negative energy densities in four-dimensional Minkowski spacetime was derived for a minimally coupled, quantized, massless, scalar field in an arbitrary quantum state. The bound has the form of an uncertainty principle-type constraint on the magnitude and duration of the negative energy density seen by a timelike geodesic observer. When spacetime is curved and/or has boundar...

متن کامل

Stable phantom energy traversable wormhole models

A possible candidate for the present accelerated expansion of the Universe is “phantom energy”, which possesses an equation of state of the form ω ≡ p/ρ < −1, consequently violating the null energy condition. As this is the fundamental ingredient to sustain traversable wormholes, this cosmic fluid presents us with a natural scenario for the existence of these exotic geometries. In this context,...

متن کامل

Geometric structure of the generic static traversable wormhole throat

Traversable wormholes have traditionally been viewed as intrinsically topological entities in some multiply connected spacetime. Here, we show that topology is too limited a tool to accurately characterize a generic traversable wormhole: in general one needs geometric information to detect the presence of a wormhole, or more precisely to locate the wormhole throat. For an arbitrary static space...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

ژورنال

عنوان ژورنال: International Journal of Geometric Methods in Modern Physics

سال: 2021

ISSN: ['0219-8878', '1793-6977']

DOI: https://doi.org/10.1142/s0219887822500190