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相关论文: Stable phantom energy traversable wormhole models

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It has recently been shown that traversable wormholes may be supported by phantom energy. In this work phantom wormhole geometries are modelled by matching an interior traversable wormhole solution, governed by the equation of state…

广义相对论与量子宇宙学 · 物理学 2009-11-11 Francisco S. N. Lobo

It has been suggested that a possible candidate for the present accelerated expansion of the Universe is ''phantom energy''. The latter possesses an equation of state of the form $\omega\equiv p/\rho<-1$, consequently violating the null…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Francisco S. N. Lobo

A possible cause of the late-time cosmic acceleration is an exotic fluid with an equation of state lying within the phantom regime, i.e., $w=p/\rho <-1$. The latter violates the null energy condition, which is a fundamental ingredient in…

广义相对论与量子宇宙学 · 物理学 2013-04-12 Francisco S. N. Lobo , Foad Parsaei , Nematollah Riazi

A possible candidate for the late time accelerated expanding Universe is phantom energy, which possesses rather bizarre properties, such as the prediction of a Big Rip singularity and the violation of the null energy condition. The latter…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Remo Garattini , Francisco S. N. Lobo

It is generally agreed that the acceleration of the Universe can best be explained by the presence of dark or phantom energy. The equation of state of the latter shows that the null energy condition is violated. Such a violation is the…

广义相对论与量子宇宙学 · 物理学 2014-11-20 Mubasher Jamil , Peter K. F. Kuhfittig , Farook Rahaman , Sk. A Rakib

We extend the notion of phantom energy--which is generally accepted for homogeneously distributed matter with $w<-1$ in the universe--on inhomogeneous spherically symmetric spacetime configurations. A spherically symmetric distribution of…

广义相对论与量子宇宙学 · 物理学 2009-11-11 S. V. Sushkov

In this paper we derive new static phantom traversable wormholes by assuming a shape function with a quadratic dependence on the radial coordinate r. We mainly focus our study on wormholes sustained by exotic matter with positive energy…

广义相对论与量子宇宙学 · 物理学 2017-10-11 Mauricio Cataldo , Fabian Orellana

We have examined the possible construction of a stationary, spherically symmetric and spatially inhomogeneous wormhole spacetime supported by the phantom energy. The later is supposed to be represented by the modified Chaplygin gas equation…

广义相对论与量子宇宙学 · 物理学 2009-03-27 Mubasher Jamil , M. Umar Farooq , Muneer Ahmad Rashid

It has been argued that wormholes are as good a prediction of Einstein's theory as black holes but the theoretical construction requires a reverse strategy, specifying the desired geometric properties of the wormhole and leaving open the…

广义相对论与量子宇宙学 · 物理学 2017-02-15 Peter K. F. Kuhfittig

This study aims to investigate the viability of a viable logarithmic f(R) gravity for inflation in giving wormhole solutions. We consider a static and spherically symmetric spacetime and two different shape functions. We found that the…

广义相对论与量子宇宙学 · 物理学 2022-06-27 Yusmantoro , Rian Julianto

Exact solutions of traversable wormholes are found under the assumption of spherical symmetry and the existence of a {\it non-static} conformal symmetry, which presents a more systematic approach in searching for exact wormhole solutions.…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Christian G. Boehmer , Tiberiu Harko , Francisco S. N. Lobo

The solutions of traversable wormholes and their geometries are investigated in higher-curvature gravity with boundary terms for each case under the presence of anisotropic, isotropic and barotropic fluids in detail. For each case, the…

广义相对论与量子宇宙学 · 物理学 2023-10-03 M. Ilyas , Kazuharu Bamba

We have found a simple exact solution of spherically-symmetrical Einstein equations describing a wormhole for an inhomogeneous distribution of the phantom energy. The equation of state is linear but highly anisotropic: while the radial…

广义相对论与量子宇宙学 · 物理学 2009-11-11 O. B. Zaslavskii

In this paper we study the possibility of sustaining an evolving wormhole via exotic matter made of phantom energy in the presence of a cosmological constant. We derive analytical evolving wormhole geometries by supposing that the radial…

广义相对论与量子宇宙学 · 物理学 2009-01-16 Mauricio Cataldo , Sergio del Campo , Paul Minning , Patricio Salgado

In this paper, we investigate the model-independent traversable wormholes from baryon acoustic oscillations. Firstly, we place the statistical constraints on the average dark energy equation of state $\omega_{av}$ by only using BAO data.…

广义相对论与量子宇宙学 · 物理学 2023-08-07 Deng Wang

The discovery that the Universe is undergoing an accelerated expansion has suggested the existence of an evolving equation of state. This paper discusses various wormhole solutions in a spherically symmetric spacetime with an equation of…

广义相对论与量子宇宙学 · 物理学 2011-03-15 Peter K. F. Kuhfittig

The firm observational confirmation of the late-time acceleration of the universe expansion has proposed a major challenge to the theoretical foundations of cosmology and the explanation of the acceleration mechanism requires the…

广义相对论与量子宇宙学 · 物理学 2016-04-20 D Wang , Xin-He Meng

We investigate static and spherically symmetric traversable wormhole solutions in the framework of $f(Q)$ gravity by considering a power-law model of the form $f(Q)=\gamma(-Q)^m$. By adopting an anisotropic matter distribution and imposing…

广义相对论与量子宇宙学 · 物理学 2026-05-11 Jaydeep Goswami , Rupam Jyoti Borah , Umananda Dev Goswami

We propose wormholes solutions by assuming space dependent equation of state parameter. Our models show that the existence of wormholes is supported by arbitrary small quantities of averaged null energy condition (ANEC) violating phantom…

广义相对论与量子宇宙学 · 物理学 2009-04-24 F. Rahaman , M. Kalam , S. Chakraborty

It is well known that phantom energy, which is characterized by the equation of state $p=\omega\rho$, $\omega <-1$, can support Morris-Thorne wormholes since it leads to a violation of the null energy condition. The purpose of this note is…

广义相对论与量子宇宙学 · 物理学 2021-03-02 Peter K. F. Kuhfittig
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