Results 121 to 130 of about 15,594 (146)

Cosmological textures

General 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
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Texture: A cosmological topological defect

Physical 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.
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String and texture defects in particle cosmology

2021
This thesis was scanned from the print manuscript for digital preservation and is copyright the author. Researchers can access this thesis by asking their local university, institution or public library to make a request on their behalf. Monash staff and postgraduate students can use the link in the References field.
openaire   +1 more source

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  

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