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Cosmological textures

open access: closedGeneral Relativity and Gravitation, 1987
Can the spatially closed Friedmann-Robertson-Walker universe (FRW) look like the flat or the open ones? In this paper the topological defects called textures, which are nonlocalized and stable solutions of classical equations of motion on a spatial manifold with compact dimensions, have been the effect responsible for the simulation of flat or open FRW
Richard L. Davis
openaire   +3 more sources

Texture: A cosmological topological defect

open access: closedPhysical Review D, 1987
The notions of phase transition and causality, combined with the standard cosmological model, lead to the appearance of topological defects in the early Universe. The most familiar types of defects are solitons, strings, and domain walls. Another type---textures---can exist when the spatial universe is compact.
Richard L. Davis
openaire   +3 more sources

Cosmology with the Laser Interferometer Space Antenna

Living Reviews in Relativity, 2023
Germano Nardini
exaly  

Cosmology and fundamental physics with the Euclid satellite

Living Reviews in Relativity, 2018
Luca Amendola   +2 more
exaly  

Cosmology and Fundamental Physics with the Euclid Satellite

Living Reviews in Relativity, 2013
Luca Amendola   +2 more
exaly  

Testing general relativity in cosmology

Living Reviews in Relativity, 2018
Mustapha Ishak
exaly  

Physics, Astrophysics and Cosmology with Gravitational Waves

Living Reviews in Relativity, 2009
Bernard F Schutz
exaly  

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