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The distribution of dark energy density in the vicinity of compact static objects is analyzed. Dark energy is assumed to be in the form of a scalar field with three parameters: the background density, the equation of state parameter and the…

广义相对论与量子宇宙学 · 物理学 2020-08-04 M. Tsizh , B. Novosyadlyj , Yu. Kulinich

If dark matter self-annihilates then it may produce an observable signal when its density is high. The details depend on the intrinsic properties of dark matter and how it clusters in space. For example, the density profile of some dark…

高能天体物理现象 · 物理学 2015-06-03 Benjamin C. Bromley

We demonstrate a new technique to search for dark compact objects. When dark matter comprising a dark compact object interacts with photons, the compact object can disperse light traveling though it. As these objects pass between Earth and…

高能物理 - 唯象学 · 物理学 2025-04-09 Joseph Bramante , Melissa D. Diamond , J. Leo Kim

We study the emissivity properties of a geometrically thin, optically thick, steady accretion disc about a static boson star. Starting from a numerical computation of the metric potentials and the rotational velocities of the particles in…

高能物理 - 唯象学 · 物理学 2009-11-07 Diego F. Torres

Dark stars are compact massive objects, described by Einstein gravitational field equations with matter. The type we consider possesses no event horizon, instead, there is a deep gravitational well with a very strong redshift factor.…

星系天体物理 · 物理学 2021-02-17 Igor Nikitin

Dark matter particles may be captured by a star and then thermalized in the star's core. At the end of its life a massive star collapses suddenly and a compact object is formed. The dark matter particles redistribute accordingly. In the…

高能天体物理现象 · 物理学 2015-06-03 Rui-Zhi Yang , Yi-Zhong Fan , Roni Waldman , Jin Chang

In this study, we investigate the image of a rotating compact object (CO) illuminated by a geometrically thin, optically thin disk on the equatorial plane. As the radius of the CO's surface fluctuates, the CO may partially or entirely…

广义相对论与量子宇宙学 · 物理学 2024-11-26 Xiangyu Wang , Xiaobao Wang , Hai-Qing Zhang , Minyong Guo

The light-like limit of the Kerr gravitational field relative to a distant observer moving rectilinearly in an arbitrary direction is an impulsive plane gravitational wave with a singular point on its wave front. By colliding particles with…

广义相对论与量子宇宙学 · 物理学 2009-11-11 C. Barrabes , V. P. Frolov , P. A. Hogan

We investigate realistic models of compact objects, focusing on neutron and strange stars, composed by dense matter and dark energy in the form of a simple fluid or scalar field interacting with matter. For the dark energy component, we use…

广义相对论与量子宇宙学 · 物理学 2023-08-01 Artyom V. Astashenok , Sergey D. Odintsov , Vasilis K. Oikonomou

Compact objects with a light sphere such as black holes and wormholes can reflect light rays like a mirror. This gravitational lensing phenomenon is called retrolensing and it is an interesting tool to survey dark and compact objects with a…

广义相对论与量子宇宙学 · 物理学 2017-03-24 Naoki Tsukamoto , Yungui Gong

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

Very compact objects probe extreme gravitational fields and may be the key to understand outstanding puzzles in fundamental physics. These include the nature of dark matter, the fate of spacetime singularities, or the loss of unitarity in…

广义相对论与量子宇宙学 · 物理学 2021-01-20 Vitor Cardoso , Paolo Pani

Strange stars are one of the hypothetical compact stellar objects that can be formed after a supernova explosion. The existence of these objects relies on the absolute stability of strange {\it collapsed} quark matter with respect to…

高能天体物理现象 · 物理学 2014-11-26 Massimo Mannarelli

The visual distortion effects visible to an observer traveling around and descending to the surface of an extremely compact star are described. Specifically, trips to a ``normal" neutron star, a black hole, and an ultracompact neutron star…

天体物理学 · 物理学 2008-11-26 Robert J. Nemiroff

In the context of the standard model of particle physics, there is a definite upper limit to the density of stable compact stars. However, if there is a deeper layer of constituents, below that of quarks and leptons, stability may be…

天体物理学 · 物理学 2014-10-13 F. Sandin

We find radiation in an infalling frame and present an explicit analytic evidence of the failure of no drama condition by showing that an infalling observer finds an infinite negative energy density at the event horizon. The negative and…

高能物理 - 理论 · 物理学 2014-04-02 Wontae Kim , Edwin J. Son

Black holes are the most compact objects in the Universe. According to general relativity, black holes have a horizon that hides a singularity where Einstein's theory breaks down. Recently, gravitational waves opened the possibility to…

广义相对论与量子宇宙学 · 物理学 2022-12-01 Elisa Maggio

Asymmetric Dark Stars, i.e., compact objects formed from the collapse of asymmetric dark matter could potentially produce a detectable photon flux if dark matter particles self-interact via dark photons that kinetically mix with ordinary…

宇宙学与河外天体物理 · 物理学 2020-12-08 Andrea Maselli , Chris Kouvaris , Kostas D. Kokkotas

Gravitational waves open the possibility to investigate the nature of compact objects and probe the horizons of black holes. Some models of modified gravity predict the presence of horizonless and singularity-free compact objects. Such dark…

广义相对论与量子宇宙学 · 物理学 2023-10-12 Elisa Maggio

Photon spheres play a pivotal role in the imaging of luminous objects near black holes. In this paper, we examine observational appearances of a star freely falling in hairy black holes, which can possess one or two photon spheres outside…

广义相对论与量子宇宙学 · 物理学 2022-07-07 Yiqian Chen , Guangzhou Guo , Peng Wang , Houwen Wu , Haitang Yang
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