Reissner-Nordstrom metric in the Friedman-Robertson-Walker universe
Changjun Gao,Shuang-Nan Zhang +1 more
TLDR
In this article, the authors obtained the metric for a Reissner-Nordstrom black hole in the background of the Friedman-Robertson-Walker universe and verified it and discussed the influence of the evolution of the universe on the size of the black hole.About:
This article is published in Physics Letters B.The article was published on 2004-08-12 and is currently open access. It has received 47 citations till now. The article focuses on the topics: De Sitter universe & Big Rip.read more
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Influence of global cosmological expansion on local dynamics and kinematics
Matteo Carrera,Domenico Giulini +1 more
TL;DR: In this article, the influence of global cosmological expansion on local systems is reviewed, where "local" is taken to mean that the sizes of the considered systems are much smaller than cosmologically relevant scales.
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Cosmological expansion and local physics
Valerio Faraoni,Audrey Jacques +1 more
TL;DR: In this paper, the interplay between cosmological expansion and local attraction in a gravitationally bound system is revisited in various regimes, including weakly gravitating Newtonian systems, and various exact solutions describing a relativistic central object embedded in a Friedmann universe.
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Does the mass of a black hole decrease due to the accretion of phantom energy
TL;DR: In this article, the authors used exact solutions describing black holes in a background Friedmann-Robertson-Walker universe, and found that the physical black hole mass may instead increase due to the accretion of phantom energy.
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Evolving Black Hole Horizons in General Relativity and Alternative Gravity
TL;DR: In this article, the authors discuss the known phenomenology of apparent and trapping horizons for analytical solutions of General Relativity and alternative theories of gravity, focusing on spherically symmetric inhomogeneities in a background cosmological spacetime.
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Making sense of the bizarre behavior of horizons in the McVittie spacetime
TL;DR: The behavior of the apparent (black hole and cosmological) horizons of the McVittie spacetime is discussed in this paper using an analogy to the Schwarzschild-de Sitter-Kottler spacetime.
References
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MAXIMA-1: A measurement of the cosmic microwave background anisotropy on angular scales of 10′-5°
Shaul Hanany,Shaul Hanany,Peter A. R. Ade,Amedeo Balbi,Amedeo Balbi,J. J. Bock,Julian Borrill,Julian Borrill,A. Boscaleri,P. de Bernardis,Pedro G. Ferreira,Pedro G. Ferreira,Viktor Hristov,Andrew H. Jaffe,Andrew E. Lange,Andrew E. Lange,Adrian T. Lee,Adrian T. Lee,Philip Daniel Mauskopf,Calvin B. Netterfield,Sang-Yun Oh,Enzo Pascale,Bahman Rabii,Paul L. Richards,George F. Smoot,Radek Stompor,C. D. Winant,Jiun-Huei Proty Wu +27 more
TL;DR: In this article, the authors presented a map and an angular power spectrum of the anisotropy of the cosmic microwave background (CMB) from the first flight of MAXIMA.
Journal ArticleDOI
MAXIMA-1: A Measurement of the Cosmic Microwave Background Anisotropy on angular scales of 10 arcminutes to 5 degrees
Shaul Hanany,P. A. R. Ade,Amedeo Balbi,J. J. Bock,J. Borrill,A. Boscaleri,P. de Bernardis,Pedro G. Ferreira,V. V. Hristov,Andrew H. Jaffe,Andrew E. Lange,Aaron Lee,P. D. Mauskopf,Calvin B. Netterfield,Sang-Yun Oh,Enzo Pascale,Bahman Rabii,Paul L. Richards,G. F. Smoot,R. Stompor,C. D. Winant,Jiun-Huei Proty Wu +21 more
TL;DR: In this article, the authors presented a map and an angular power spectrum of the anisotropy of the cosmic microwave background (CMB) from the first flight of MAXIMA.
Journal ArticleDOI
The Mass-Particle in an Expanding Universe
Journal ArticleDOI
The Effect of Cosmological Expansion on Self-Gravitating Ensembles of Particles
TL;DR: Galactic clusters evolution in universe with zero rest mass particles, showing size dependence on cosmic dust energy density as discussed by the authors, showing that the size of the clusters depends on the amount of dust energy.