Abstract
The structure of the inhomogeneities in the expanding quasi-uniform Friedmann–Robertson–Walker Universe is the result of a long stage of growth of small initial fluctuations. Such fluctuations in cosmological models should be set initially. They cannot be attributed to statistical density fluctuations of particles.
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© 2012 Cambridge International Science Publishing
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Khlopov, M. (2012). New Physics in Formation of the Large-Scale Structure. In: Fundamentals of Cosmic Particle Physics. Cambridge International Science Publishing, Cambridge. https://doi.org/10.1007/978-1-907343-72-8_8
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DOI: https://doi.org/10.1007/978-1-907343-72-8_8
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Publisher Name: Cambridge International Science Publishing, Cambridge
Print ISBN: 978-1-907343-48-3
Online ISBN: 978-1-907343-72-8
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