The Early universe - INSPIRE

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The Early universe

Andrew R. Liddle
(
- Sussex U.
)

Dec, 1996

32 pages

Published in:

ASP Conf.Ser. 126 (1997) 31

Contribution to:

1st Moroccan International Astronomy School: From Quantum Fluctuations to Cosmological Structures (Casa 96 Cosmology School)

e-Print:

astro-ph/9612093 [astro-ph]

Report number:

SUSSEX-AST-96-12-1

View in:

ADS Abstract Service

reference search18 citations

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Abstract: (arXiv)

An introductory account is given of the modern understanding of the physics of the early Universe. Particular emphasis is placed on the paradigm of cosmological inflation, which postulates a period of accelerated expansion during the Universe's earliest stages. Inflation provides a possible origin for structure in the Universe, such as microwave background anisotropies, galaxies and galaxy clusters; these observed structures can therefore be used to test models of inflation. A brief account is given of other early Universe topics, namely baryogenesis, topological defects, dark matter candidates and primordial black holes.

talk: Casablanca 1996/12/01
astrophysics: model
inflationary universe
cosmic radiation: background
cosmic radiation: anisotropy
density: perturbation
gravitational radiation
baryon: production
topology: defect
astrophysics: missing-mass

References(41)

Figures(0)

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