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相关论文: Ghost stars in general relativity

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In this paper, we discuss the existence of ghost star models in the Einstein-Maxwell framework. In order to explore these objects, we put forward the idea of Zeldovich and Novikov by keeping in mind that the energy density of such models…

广义相对论与量子宇宙学 · 物理学 2025-03-25 Tayyab Naseer , K. Hassan , M. Sharif

We present static axially symmetric fluid distributions not producing gravitational field outside their boundaries (i.e. fluid sources which match smoothly on the boundary surface to Minkowski space-time). These solutions provide further…

广义相对论与量子宇宙学 · 物理学 2025-06-06 L. Herrera , J. L. Hernandez-Pastora , J. Ospino , A. Di Prisco

Ghost stars are compact configurations characterized by an arbitrarily small total mass. Such objects require regions of negative energy density -a condition typically regarded as unphysical within the context of conventional stellar…

广义相对论与量子宇宙学 · 物理学 2026-01-01 Alberto Guilabert , Ernesto Fuenmayor , Pedro Bargueño , Ernesto Contreras

The existence of cosmological compact objects with very strong gravity is a prediction of General Relativity and an exact solution of the Einstein equations. These objects are called black holes and recently we had the first observations of…

广义相对论与量子宇宙学 · 物理学 2022-12-09 Ioannis Antoniou

Strange stars ought to exist in the universe according to the strange quark matter hypothesis, which states that matter made of roughly equal numbers of up, down, and strange quarks could be the true ground state of baryonic matter rather…

高能天体物理现象 · 物理学 2023-04-20 Shu-Hua Yang , Chun-Mei Pi , Xiao-Ping Zheng , Fridolin Weber

The energy in the ghost-free massive gravity theory is calculated via explicitly resolving the initial value constraints for spherically symmetric deformations of flat space. It turns out that the energy is positive in some cases, but in…

高能物理 - 理论 · 物理学 2014-09-25 Mikhail S. Volkov

In the present work we study the gravitational effects of condensed dark matter on strange stars. We consider self-interacting dark matter particles with properties consistent with current observational constraints, and dark matter inside…

广义相对论与量子宇宙学 · 物理学 2017-08-02 Grigoris Panotopoulos , Ilidio Lopes

We conjecture the possibility of negative mass objects (NMOs) existing in the sky. It is shown that they may not be so exotic as usually expected. We show that NMOs appear as solutions of standard gravitational equations if we consider the…

广义相对论与量子宇宙学 · 物理学 2026-05-28 Shin'ichi Nojiri , S. D. Odintsov

We propose a theoretically consistent modification of gravity in the infrared, which is compatible with all current experimental observations. This is an analog of Higgs mechanism in general relativity, and can be thought of as arising from…

高能物理 - 理论 · 物理学 2009-11-10 Nima Arkani-Hamed , Hsin-Chia Cheng , Markus A. Luty , Shinji Mukohyama

Neutron Stars (NSs) are compact stellar objects that are stable solutions in General Relativity. Their internal structure is usually described using an equation of state that involves the presence of ordinary matter and its interactions.…

高能天体物理现象 · 物理学 2020-12-18 M. Ángeles Pérez-García , J. Silk

A new solution for the endpoint of gravitational collapse is proposed. By extending the concept of Bose-Einstein condensation to gravitational systems, a cold, compact object with an interior de Sitter condensate phase and an exterior…

广义相对论与量子宇宙学 · 物理学 2023-02-16 Pawel O. Mazur , Emil Mottola

We consider the infrared modification of gravity by ghost condensate. Naively, in this scenario one expects sizeable modification of gravity at distances of order 1000 km, provided that the characteristic time scale of the theory is of the…

高能物理 - 唯象学 · 物理学 2009-11-10 S. L. Dubovsky

Gravitational vacuum condensate stars, also known as gravastars, have been proposed as an alternative to black holes. Their interior contains a perfect fluid with an equation of state akin to that of a cosmological constant. For this…

广义相对论与量子宇宙学 · 物理学 2023-08-16 P. P. Avelino

The generic properties of compact objects made of two different fluids of dark matter are studied in a scale invariant approach. We investigate compact objects with a core-shell structure, where the two fluids are separated, and with mixed…

广义相对论与量子宇宙学 · 物理学 2023-03-01 Marie Cassing , Alexander Brisebois , Muhammad Azeem , Jürgen Schaffner-Bielich

Observations by the MACHO collaboration suggest that a significant proportion of the galactic halo dark matter is in the form of compact objects with typical masses $M\sim 0.5M_{\odot}$. One of the current mysteries is the nature and origin…

天体物理学 · 物理学 2008-11-26 R. Foot

Adopting the phantom (ghost) scalar field description of dark energy, we construct a general class of exact interior solutions describing mixed relativistic stars containing both ordinary matter and dark energy in different proportions. The…

广义相对论与量子宇宙学 · 物理学 2011-06-24 Stoytcho S. Yazadjiev

We consider 2d Maxwell system defined on the Rindler space with metric ds^2=\exp(2a\xi)\cdot(d\eta^2-d\xi^2) with the goal to study the dynamics of the ghosts. We find an extra contribution to the vacuum energy in comparison with Minkowski…

广义相对论与量子宇宙学 · 物理学 2010-12-09 Ariel R. Zhitnitsky

We show that the Novikov coordinates can be obtained in a direct and physically transparent way from the radial geodesics of massive particles with negative energy in the Schwarzschild spacetime. These geodesics form a complete congruence…

广义相对论与量子宇宙学 · 物理学 2026-01-27 Jaume de Haro

We study the properties of compact objects in a particular 4D Horndeski theory originating from higher dimensional Einstein-Gauss-Bonnet gravity. Remarkably, an exact vacuum solution is known. This compact object differs from general…

广义相对论与量子宇宙学 · 物理学 2022-03-02 Christos Charmousis , Antoine Lehébel , Evangelos Smyrniotis , Nikolaos Stergioulas

The observed excess of gravitational forces in galaxies and galactic clusters is usually referred as the existence of "dark matter particles" of unknown origin. An alternative explanation of the dark matter effect is presented here by…

宇宙学与河外天体物理 · 物理学 2011-10-04 Arkady Z. Dolginov
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