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Cosmological Black Holes

by Cosimo Stornaiolo , 2001
"... In this letter we propose the existence of low density black holes and discuss its compatibility with the cosmological observations. The origin of these black holes can be traced back to the collapse of long wavelength cosmological perturbations during the matter dominated era, when the densities ar ..."
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In this letter we propose the existence of low density black holes and discuss its compatibility with the cosmological observations. The origin of these black holes can be traced back to the collapse of long wavelength cosmological perturbations during the matter dominated era, when the densities

Abstract Cosmological Black Holes as Models of Cosmological Inhomogeneities

by Megan L. Mcclure, Megan L. Mcclure , 2006
"... Since cosmological black holes modify the density and pressure of the surrounding universe, and introduce heat conduction, they produce simple models of cosmologi-cal inhomogeneities that can be used to study the eect of inhomogeneities on the universe's expansion. In this thesis, new cosmologi ..."
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Since cosmological black holes modify the density and pressure of the surrounding universe, and introduce heat conduction, they produce simple models of cosmologi-cal inhomogeneities that can be used to study the eect of inhomogeneities on the universe's expansion. In this thesis, new

Perturbations of rotating cosmological black holes

by Zoltán Perjés , 2002
"... Charged, rotating black hole solutions of Einstein’s gravitational equations are investigated in the presence of a cosmological constant. A pair of wave equations governing the electromagnetic and gravitational perturbations are derived. PACS Numbers: 04.70.-s, 97.60.Lf, 04.20.Jb 1 I. ..."
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Charged, rotating black hole solutions of Einstein’s gravitational equations are investigated in the presence of a cosmological constant. A pair of wave equations governing the electromagnetic and gravitational perturbations are derived. PACS Numbers: 04.70.-s, 97.60.Lf, 04.20.Jb 1 I.

Cosmological Black Holes as Seeds of Voids in Galaxy Distribution

by S. Capozziello, M. Funaro, C. Stornaiolo, Angelo Via Cinthia , 2004
"... A&A manuscript no. (will be inserted by hand later) Your thesaurus codes are: missing; you have not inserted them ..."
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A&A manuscript no. (will be inserted by hand later) Your thesaurus codes are: missing; you have not inserted them

Cosmological black holes as voids progenitors. I. Simulations.

by M. Serpico, G. Longo, C. Stornaiolo , 2005
"... Accepted xxxxxxx; received xxxxxxx; in original form 2005 July 12 ..."
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Accepted xxxxxxx; received xxxxxxx; in original form 2005 July 12

Cosmology, Black Holes and Shock Waves Beyond the Hubble Length

by Joel Smoller, Blake Temple , 2003
"... We construct exact, entropy satisfying shock wave solutions of the Einstein equations for a perfect fluid which extend the Oppeheimer-Snyder (OS) model to the case of non-zero pressure, inside the Black Hole. These solutions put forth a new Cosmological Model in which the expanding Friedmann-Roberts ..."
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We construct exact, entropy satisfying shock wave solutions of the Einstein equations for a perfect fluid which extend the Oppeheimer-Snyder (OS) model to the case of non-zero pressure, inside the Black Hole. These solutions put forth a new Cosmological Model in which the expanding Friedmann

The Search for Cosmological Black Holes: A Surface Brightness Variability Test

by Geraint F. Lewis, Rodrigo A. Ibata , 2000
"... Recently it has been suggested that the majority of dark matter in the universe resides in the form of Jupiter mass black holes distributed cosmologically. This population makes itself apparent by microlensing high redshift quasars and introducing pronounced variability into their observed light cur ..."
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Recently it has been suggested that the majority of dark matter in the universe resides in the form of Jupiter mass black holes distributed cosmologically. This population makes itself apparent by microlensing high redshift quasars and introducing pronounced variability into their observed light

COSMOLOGICAL/BLACK-HOLE UNIFIED THEORY AS A CONSTRAINED SYSTEM

by J. A. Nietoa, G. Avilab
"... ar ..."
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Preprint typeset using L ATEX style emulateapj v. 14/09/00 COSMOLOGICAL BLACK HOLE SPIN EVOLUTION BY MERGERS AND ACCRETION

by Emanuele Berti, Marta Volonteri , 2008
"... Using recent results from numerical relativity simulations of black hole mergers, we revisit previous studies of cosmological black hole spin evolution. We show that mergers are very unlikely to yield large spins, unless alignment of the spins of the merging holes with the orbital angular momentum i ..."
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Using recent results from numerical relativity simulations of black hole mergers, we revisit previous studies of cosmological black hole spin evolution. We show that mergers are very unlikely to yield large spins, unless alignment of the spins of the merging holes with the orbital angular momentum

Quantum Gravity

by Lee Smolin , 2004
"... We describe the basic assumptions and key results of loop quantum gravity, which is a background independent approach to quantum gravity. The emphasis is on the basic physical principles and how one deduces predictions from them, at a level suitable for physicists in other areas such as string theor ..."
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integral quantizations, coupling to matter, extensions to supergravity and higher dimensional theories, as well as applications to black holes, cosmology and Plank scale phenomenology. We describe the near term prospects for observational tests of quantum theories of gravity and the expectations that loop
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