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相关论文: Ghost stars in general relativity

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Recent observations have revealed the structural properties of the dark and luminous mass distribution in spirals. These results led to the vision of a new and amazing scenario. The investigation of single and coadded objects has shown that…

星系天体物理 · 物理学 2015-04-13 Paolo Salucci , Mariafelicia De Laurentis

An experimental detection of graviton is extremely hard problem, however, there are different ways to evaluate a graviton mass if it is non-vanishing. Theories of massive gravity or theories with non-vanishing graviton mass initially have a…

广义相对论与量子宇宙学 · 物理学 2018-06-26 Alexander F. Zakharov , Predrag Jovanovic , Dusko Borka , Vesna Borka Jovanovic

Asymmetric dark matter under certain conditions could form compact star-like objects, which can be searched either through gravitational lensing or by observation of gravitational waves from binaries involving such compact objects. In this…

高能物理 - 唯象学 · 物理学 2023-10-09 Boris Betancourt Kamenetskaia , Anja Brenner , Alejandro Ibarra , Chris Kouvaris

We develop a new approach to building cosmological models, in which small pieces of perturbed Minkowski space are joined together at reflection-symmetric boundaries in order to form a global, dynamical space-time. Each piece of this…

广义相对论与量子宇宙学 · 物理学 2016-04-12 Viraj A. A. Sanghai , Timothy Clifton

We ask if the conventional variable separation techniques in the studying of standard cosmology and the collapsing of extremely dense stars introduce Newton's absolute space-time concepts. If this is the case, then a completely relative…

广义相对论与量子宇宙学 · 物理学 2016-08-31 Ding-fang Zeng , Yi-hong Gao

The description of the heaviest neutron stars observed in Nature depends on the understanding of the physical concepts present in General Relativity and Quantum Chromodynamics. In this work, we review the basic concepts need to describe…

高能物理 - 唯象学 · 物理学 2020-08-11 V. P. Goncalves , L. Lazzari

We discuss various space-time metrics which are compatible with Einstein's equations and a previously suggested cosmology with a finite total mass. In this alternative cosmology the matter density was postulated to be a spatial delta…

广义相对论与量子宇宙学 · 物理学 2015-05-20 L. Clavelli , Gary R. Goldstein

P-stars are compact relativistic stars made of deconfined up and down quarks in a chromomagnetic condensate proposed by us long time ago. P-stars do not admit a critical mass thereby they are able to overcome the gravitational collapse to…

高能天体物理现象 · 物理学 2020-11-10 Paolo Cea

To describe a massive graviton in 4D Minkowski space-time one introduces a quadratic term in the Lagrangian. This term, however, can lead to a readjustment or instability of the background instead of describing a massive graviton on flat…

高能物理 - 理论 · 物理学 2011-07-19 Gregory Gabadadze , Andrei Gruzinov

In this paper, we present a new theory explaining the origin of inertia based on two key ideas: gravity as a spin-1 gauge field theory and the relativity of all kinds of motion. This theory proposes that inertial mass is influenced by the…

综合物理 · 物理学 2024-09-17 Konstantinos I. Tsarouchas

We review some modified gravity models which describe the gravitational dark energy and the possibility of cosmic speed-up. The new consistent version of such theory which contains inverse and HD curvature terms as well as new type of…

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

Assuming static and spherically symmetric spacetimes in the ghost-free bigravity theory, we find a relativistic star solution, which is very close to that in general relativity. The coupling constants are classified into two classes: Class…

广义相对论与量子宇宙学 · 物理学 2016-03-30 Katsuki Aoki , Kei-ichi Maeda , Makoto Tanabe

Astrophysicists distinguish between three different types of compact stars. These are white dwarfs, neutron stars, and black holes. The former contain matter in one of the densest forms found in the Universe. This feature, together with the…

天体物理学 · 物理学 2007-05-23 Fridolin Weber , Andreu Torres i Cuadrat , Alexander Ho , Philip Rosenfield

We propose that the ``isolated'' planetary mass objects observed by Zapatero Osorio et al in the $\sigma$ Orionis cluster might actually be in orbit around invisible stellar mass companions such as mirror stars. Mirror matter is expected to…

天体物理学 · 物理学 2009-10-31 R. Foot , A. Yu. Ignatiev , R. R. Volkas

General Relativity receives quantum corrections relevant at macroscopic distance scales and near event horizons. These arise from the conformal scalar degrees of freedom in the extended effective field theory of gravity generated by the…

广义相对论与量子宇宙学 · 物理学 2012-09-25 Emil Mottola

The simplistic model of the classical spacetime foam is considered, which consists of static wormholes embedded in Minkowski spacetime. We explicitly demonstrate that such a foam structure leads to a topological bias of point-like sources…

天体物理学 · 物理学 2008-11-26 A. A. Kirillov , E. P. Savelova

This paper discusses a generalized model for compact stars, assumed to be anisotropic in nature due to the spherical symmetry and high density. After embedding the four-dimensional spacetime in a five-dimensional flat spacetime, which may…

综合物理 · 物理学 2018-03-09 S. K. Maurya , Debabrata Deb , Saibal Ray , P. K. F. Kuhfittig

Major progresses have been made this last year towards a better knowledge of the invisible mass. Michel Spiro will talk in details about the micro-lensing experiments and their promising results; the ROSAT satellite has provided extended…

天体物理学 · 物理学 2007-05-23 F. Combes , D. Pfenniger

We propose a new classical theory of gravity which is based on the principle of equivalence and assumption that gravity, similarly to electrodynamics, is described by a vector field in Minkowski space-time. We show that such assumptions…

广义相对论与量子宇宙学 · 物理学 2009-04-22 Anatoly A. Svidzinsky

Z-boson exchange interaction induces attractive force between left-handed neutrino and neutron. The Ginzburg-Landau mean field calculation and the Bogoliubov transformation suggest that this attractive force leads to neutrino-neutron pair…

高能物理 - 唯象学 · 物理学 2022-09-13 M. Yoshimura
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