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相关论文: Dynamic wormholes, anti-trapped surfaces, and ener…

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Although wormholes can be treated as topological objects in spacetime and from a global point-of-view, a precise definition of what a wormhole throat is and where it can be located can be developed and treated entirely in terms of local…

广义相对论与量子宇宙学 · 物理学 2007-05-23 David Hochberg , Matt Visser

We extend previous proofs that violations of the null energy condition (NEC) are a generic and universal feature of traversable wormholes to completely non-symmetric time-dependent wormholes. We show that the analysis can be phrased purely…

广义相对论与量子宇宙学 · 物理学 2009-10-31 David Hochberg , Matt Visser

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…

广义相对论与量子宇宙学 · 物理学 2011-09-30 David Hochberg , Matt Visser

Wormholes and black holes have traditionally been treated a quite separate objects with relatively little overlap. The possibility of a connection arises in that wormholes, if they exist, might have profound influence on black holes, their…

广义相对论与量子宇宙学 · 物理学 2013-08-27 Matt Visser , David Hochberg

A dynamical theory of traversable wormholes is detailed in spherical symmetry. Generically a wormhole consists of a tunnel of trapped surfaces between two mouths, defined as temporal outer trapping horizons with opposite senses, in mutual…

广义相对论与量子宇宙学 · 物理学 2009-06-30 Sean A. Hayward

We present a new definition of the wormhole throat including the flare-out condition and the traversability for general dynamical spacetimes in terms of null geodesic congruences. We will examine our definition for some examples and see…

广义相对论与量子宇宙学 · 物理学 2015-06-11 Yoshimune Tomikawa , Keisuke Izumi , Tetsuya Shiromizu

In the present work we analyse a dynamical wormhole solution with two fluids system (one isotropic and homogeneous and the other being inhomogeneous and anisotropic in nature) as the matter at the throat. We choose two different forms of…

广义相对论与量子宇宙学 · 物理学 2024-05-10 Dhritimalya Roy , Ayanendu Dutta , Bikram Ghosh , Subenoy Chakraborty

The general form of a stationary, axially symmetric traversable wormhole is discussed. This provides an explicit class of rotating wormholes that generalize the static, spherically symmetric ones first considered by Morris and Thorne. In…

广义相对论与量子宇宙学 · 物理学 2010-11-19 Edward Teo

In quadratic gravity, the junction conditions are six and permit the appearance of double layer thin shells. Double layers arise typically in theories with dipoles, i.e., two opposite charges, such as electromagnetic theories, and appear…

广义相对论与量子宇宙学 · 物理学 2023-05-12 Joao Luís Rosa , Rui André , José P. S. Lemos

A new framework is proposed for general dynamic wormholes, unifying them with black holes. Both are generically defined locally by outer trapping horizons, temporal for wormholes and spatial or null for black and white holes. Thus wormhole…

广义相对论与量子宇宙学 · 物理学 2009-10-31 Sean A. Hayward

Wormhole is defined as the topological structure with the throat connecting two asymptotically flat spaces. In order to have and maintain the structure of the wormhole, there needs the geometrical flare-out condition, i.e., the minimal size…

广义相对论与量子宇宙学 · 物理学 2015-06-15 Sung-Won Kim

We construct solutions of plane symmetric wormholes in the presence of a negative cosmological constant by matching an interior spacetime to the exterior anti-de Sitter vacuum solution. The spatial topology of this plane symmetric wormhole…

广义相对论与量子宇宙学 · 物理学 2009-11-10 José P. S. Lemos , Francisco S. N. Lobo

It is shown that the existence of static, cylindrically symmetric wormholes does not require violation of the weak or null energy conditions near the throat, and cylindrically symmetric wormhole geometries can appear with less exotic…

广义相对论与量子宇宙学 · 物理学 2009-07-30 Kirill A. Bronnikov , José P. S. Lemos

It was argued in literature that traversable wormholes can exist with arbitrarily small violation of null energy conditions. We show that if the amount of exotic material near the wormhole throat tends to zero, either this leads to a horn…

广义相对论与量子宇宙学 · 物理学 2008-11-26 O. B. Zaslavskii

We consider a topologically nontrivial thin-shell wormhole with a throat in the form of a $T^2$ torus. It is shown that: (i)~such a wormhole is stable with respect to excitations of the throat; (ii)~not all energy conditions are violated…

广义相对论与量子宇宙学 · 物理学 2019-02-27 Vladimir Dzhunushaliev , Vladimir Folomeev , Burkhard Kleihaus , Jutta Kunz

In this work we explore the possible existence of static, spherically symmetric and stationary, axisymmetric traversable wormholes coupled to nonlinear electrodynamics. Considering static and spherically symmetric (2+1) and…

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

This paper discusses traversable wormholes that differ slightly but significantly from those of the Morris-Thorne type under the assumption of cylindrical symmetry. The throat is a piecewise smooth cylindrical surface resulting in a shape…

广义相对论与量子宇宙学 · 物理学 2009-11-11 Peter K. F. Kuhfittig

A fundamental property in wormhole physics is the flaring-out condition of the throat, which through the Einstein field equation entails the violation of the null energy condition. In the context of modified theories of gravity, it has also…

广义相对论与量子宇宙学 · 物理学 2012-11-07 Francisco S. N. Lobo

We study geodesic motion near the throats of asymptotically flat, static, spherically~symmetric traversable wormholes supported by a self-gravitating minimally coupled phantom scalar field with an arbitrary self-interaction potential. We…

广义相对论与量子宇宙学 · 物理学 2020-10-20 Ivan Potashov , Julia Tchemarina , Alexander Tsirulev

We present a family of charged, traversable wormhole solutions in the presence of a cosmological constant. In de Sitter spacetime, two types of wormhole throats can exist--referred to as typical and cosmological throat--located at small and…

广义相对论与量子宇宙学 · 物理学 2026-01-13 Hyeong-Chan Kim , Wonwoo Lee
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