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相关论文: A wormhole-generated physical universe with refine…

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A crucial aspect of wormhole (WH) physics is the inclusion of exotic matter, which requires violating the null energy condition. Here, we explore the potential for WHs to be sustained by quark matter under conditions of extreme density…

广义相对论与量子宇宙学 · 物理学 2024-08-20 Sneha Pradhan , Zinnat Hassan , P. K. Sahoo

We consider the quantum analogues of wormholes obtained by Carlini and Miji\'c (CM), who analytically continued closed universe models. To obtain wormholes when the strong energy condition ($\gamma>2/3$) is satisfied, we are able to…

广义相对论与量子宇宙学 · 物理学 2009-09-25 A. Carlini , D. H. Coule , D. M. Solomons

We present a complete quantum mechanical description of a flat FRW universe with equation of state p=\rho. We find a detailed correspondence with our heuristic picture of such a universe as a dense black hole fluid. Features of the geometry…

高能物理 - 理论 · 物理学 2009-11-10 T. Banks , W. Fischler , L. Mannelli

We model spacetime foam by a gas of virtual wormholes. Then applying an external field one may change the density of virtual wormholes and try to organize a wormhole-like structure in space. The relation between an additional distribution…

广义相对论与量子宇宙学 · 物理学 2014-05-14 E. P. Savelova , A. A. Kirillov

We investigate wormhole solutions using the modified gravity model $f(Q,T)$ with viscosity and aim to find a solution for the existence of wormholes mathematically without violating the energy conditions. We show that there is no need to…

广义相对论与量子宇宙学 · 物理学 2024-10-08 S. Davood Sadatian , S. Mohamad Reza Hosseini

An oscillating universe cycles through a series of expansions and contractions. We propose a model in which ``phantom'' energy with a supernegative pressure ($p < - \rho$) grows rapidly and dominates the late-time expanding phase. The…

天体物理学 · 物理学 2008-03-29 Katherine Freese , Matthew G. Brown , William H. Kinney

A new kind of evolution for cyclic models in which the Hubble parameter oscillates and keeps positive has been explored in a specific $f(R,T)$ gravity reconstruction. A singularity-free cyclic universe with negative varying cosmological…

广义相对论与量子宇宙学 · 物理学 2019-02-11 Nasr Ahmed , Sultan Z. Alamri

We discuss the modified gravity which may produce the current cosmic aceleration of the universe and eliminates the need for dark energy. It is shown that such models where the action quickly grows with the decrease of the curvature define…

高能物理 - 理论 · 物理学 2009-09-17 Shin'ichi Nojiri , Sergei D. Odintsov

Some novel regular spacetimes are considered that show a non-stationary wormhole structure. A Simpson-Visser-like procedure is applied to reconstruct these regular spacetimes, free of time-like and space-like singularities. Such a procedure…

广义相对论与量子宇宙学 · 物理学 2025-08-13 G. Alencar , R. Dárlla , Shin'ichi Nojiri , Sergei D. Odintsov , Diego Sáez-Chillón Gómez

In this paper we attempt to examine the possibility of construction of a traversable wormhole on the Randall-Sundrum braneworld with ordinary matter employing the Kuchowicz potential as one of the metric potentials. In this scenario, the…

广义相对论与量子宇宙学 · 物理学 2022-03-31 Rikpratik Sengupta , Shounak Ghosh , Mehedi Kalam , Saibal Ray

Observations of distant supernovae indicate that the Universe is now in a phase of accelerated expansion the physical cause of which is a mystery. Formally, this requires the inclusion of a term acting as a negative pressure in the…

We wish to demonstrate how the presence of a dynamic cosmological parameter, plus a model of the universe as a quantum computer can be combined to give us a picture of early universe inflationary physics which is quite non linear, with a…

数学物理 · 物理学 2011-11-10 A. W. Beckwith

It is shown that in the presence of virtual wormholes, the vacuum is unstable, which leads to a series of phase transitions in the early Universe. Then the standard Kibble scenario predicts the formation of defects such as domain walls. An…

广义相对论与量子宇宙学 · 物理学 2024-02-02 A. A. Kirillov , E. P. Savelova

We considered the generation of gravitational waves by the binary system associated with a wormhole. In the Newtonian limit, the gravitational potential of a wormhole requires the effective mass of the wormhole taking into account radial…

广义相对论与量子宇宙学 · 物理学 2023-11-08 Sung-Won Kim

Spacetime wormholes are evidently an essential component of the construction of a time machine. Within the context of general relativity, such objects require, for their formation, exotic matter -- matter that violates at least one of the…

广义相对论与量子宇宙学 · 物理学 2024-06-13 Mengqi Lu , Jiayue Yang , Robert B. Mann

Wormholes are extremely attractive objects for research, and although many mathematical and physical properties of these objects have been discovered and studied in the recent decades, there remain many unsolved problems and opportunities…

广义相对论与量子宇宙学 · 物理学 2023-11-14 Kirill A. Bronnikov , Sergey V. Sushkov

A model of induced gravity with Higgs potential is analysed for the FLRW cosmology. Conditions of acceleration and signatures for the primeval universe along with the inflation are discussed. It is shown that the scalar-field excitations…

广义相对论与量子宇宙学 · 物理学 2015-03-17 Nils M. Bezares-Roder , Hemwati Nandan , Umananda Dev Goswami

The present work deals with a spherically symmetric space-time which is asymptotically (at spatial infinity) FRW space-time and represents wormhole configuration: The matter component is divided into two parts--(a) dissipative but…

广义相对论与量子宇宙学 · 物理学 2015-01-27 Supriya Pan , Subenoy Chakraborty

A non-singular cosmology is derived in modified gravity (MOG) with a varying gravitational coupling strength $G(t)=G_N\xi(t)$. Assuming that the curvature $k$, the cosmological constant $\Lambda$ and $\rho$ vanish at $t=0$, we obtain a…

广义相对论与量子宇宙学 · 物理学 2007-10-24 J. W. Moffat

We examine the compatibility of the mirror matter concept with the non-orientable wormholes. If any particle (or classical object) is traversing through the non-orientable wormhole, it turns into a corresponding mirror particle and vice…

广义相对论与量子宇宙学 · 物理学 2014-08-04 V. I. Dokuchaev , Yu. N. Eroshenko