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The Role of Quantum Mechanics in Modern Cosmology
I will briefly review, in simple terms, the crucial role of quantum mechanics in modern inflationary cosmology. Quantum processes throughout the inflationary epoch determine the subsequent evolution of our Universe, including the formation of its large-scale structures (galaxies, clusters, voids, .....
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Lenguaje: | eng |
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2022
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Acceso en línea: | https://dx.doi.org/10.1007/978-3-031-05625-3_2 http://cds.cern.ch/record/2847755 |
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author | Veneziano, Gabriele |
author_facet | Veneziano, Gabriele |
author_sort | Veneziano, Gabriele |
collection | CERN |
description | I will briefly review, in simple terms, the crucial role of quantum mechanics in modern inflationary cosmology. Quantum processes throughout the inflationary epoch determine the subsequent evolution of our Universe, including the formation of its large-scale structures (galaxies, clusters, voids, ...). In the inflationary scenario the role of the hot big bang of pre-inflationary cosmology is completely overturned: it is played by the instant at which the Universe, after having been cooled down to practically zero temperature, suddenly “reheats” through an irreversible quantum process. Therefore, an unavoidable consequence of inflation is that the hot big bang is neither associated with a singularity nor with the beginning of time. At the end I will offer some more speculative ideas, mostly based on string theory, on what may have preceded inflation and about whether time had a beginning. |
id | cern-2847755 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2022 |
record_format | invenio |
spelling | cern-28477552023-01-30T10:29:56Zdoi:10.1007/978-3-031-05625-3_2http://cds.cern.ch/record/2847755engVeneziano, GabrieleThe Role of Quantum Mechanics in Modern CosmologyAstrophysics and AstronomyI will briefly review, in simple terms, the crucial role of quantum mechanics in modern inflationary cosmology. Quantum processes throughout the inflationary epoch determine the subsequent evolution of our Universe, including the formation of its large-scale structures (galaxies, clusters, voids, ...). In the inflationary scenario the role of the hot big bang of pre-inflationary cosmology is completely overturned: it is played by the instant at which the Universe, after having been cooled down to practically zero temperature, suddenly “reheats” through an irreversible quantum process. Therefore, an unavoidable consequence of inflation is that the hot big bang is neither associated with a singularity nor with the beginning of time. At the end I will offer some more speculative ideas, mostly based on string theory, on what may have preceded inflation and about whether time had a beginning.oai:cds.cern.ch:28477552022 |
spellingShingle | Astrophysics and Astronomy Veneziano, Gabriele The Role of Quantum Mechanics in Modern Cosmology |
title | The Role of Quantum Mechanics in Modern Cosmology |
title_full | The Role of Quantum Mechanics in Modern Cosmology |
title_fullStr | The Role of Quantum Mechanics in Modern Cosmology |
title_full_unstemmed | The Role of Quantum Mechanics in Modern Cosmology |
title_short | The Role of Quantum Mechanics in Modern Cosmology |
title_sort | role of quantum mechanics in modern cosmology |
topic | Astrophysics and Astronomy |
url | https://dx.doi.org/10.1007/978-3-031-05625-3_2 http://cds.cern.ch/record/2847755 |
work_keys_str_mv | AT venezianogabriele theroleofquantummechanicsinmoderncosmology AT venezianogabriele roleofquantummechanicsinmoderncosmology |