Creation of quantized particles, gravitons and scalar perturbations by the expanding universe

Quantum creation processes during the very rapid early expansion of the universe are believed to give rise to temperature anisotropies and polarization patterns in the CMB radiation. These have been observed by satellites such as COBE, WMAP, and PLANCK, and by bolometric instruments placed near the...

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Main Author: Parker, Leonard
Format: Text
Language:unknown
Published: arXiv 2015
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Online Access:https://dx.doi.org/10.48550/arxiv.1503.00359
https://arxiv.org/abs/1503.00359
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spelling ftdatacite:10.48550/arxiv.1503.00359 2023-05-15T18:23:07+02:00 Creation of quantized particles, gravitons and scalar perturbations by the expanding universe Parker, Leonard 2015 https://dx.doi.org/10.48550/arxiv.1503.00359 https://arxiv.org/abs/1503.00359 unknown arXiv https://dx.doi.org/10.1088/1742-6596/600/1/012001 arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ General Relativity and Quantum Cosmology gr-qc FOS Physical sciences article-journal Article ScholarlyArticle Text 2015 ftdatacite https://doi.org/10.48550/arxiv.1503.00359 https://doi.org/10.1088/1742-6596/600/1/012001 2022-04-01T12:15:05Z Quantum creation processes during the very rapid early expansion of the universe are believed to give rise to temperature anisotropies and polarization patterns in the CMB radiation. These have been observed by satellites such as COBE, WMAP, and PLANCK, and by bolometric instruments placed near the South Pole by the BICEP collaborations. The expected temperature anisotropies are well-confirmed. The B-mode polarization patterns in the CMB are currently under measurement jointly by the PLANCK and BICEP groups to determine the extent to which the B-modes can be attributed to gravitational waves from the creation of gravitons in the earliest universe. It was during 1962 that I proved that quanta of the minimally-coupled scalar field were created by the general expanding FLRW universe. This was relevant also to the creation of quantized perturbations of the gravitational field, since these perturbations satisfied linear field equations that could be quantized in the same way as the minimally-coupled scalar field equation. In fact, in 1946, E.M. Lifshitz had considered the classical Einstein gravitational field in FLRW expanding universes and had shown that the classical linearized Einstein field equations reduced, in what is now known as the Lifshitz gauge, to two separate classical minimally-coupled massless scalar field equations. These field equations of Lifshitz, when quantized, correspond to the field equations for massless gravitons, one equation for each of the two independent polarization components of the spin-2 massless graviton. I will discuss this further in this article.1 1 Plenary Lecture given September 2, 2014 at the ERE2014 Conference in Valencia, Spain : Plenary Lecture given September 2, 2014 at the ERE2014 Conference in Valencia, Spain To appear in the Proceedings of the ERE2014 Conference Text South pole DataCite Metadata Store (German National Library of Science and Technology) South Pole
institution Open Polar
collection DataCite Metadata Store (German National Library of Science and Technology)
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topic General Relativity and Quantum Cosmology gr-qc
FOS Physical sciences
spellingShingle General Relativity and Quantum Cosmology gr-qc
FOS Physical sciences
Parker, Leonard
Creation of quantized particles, gravitons and scalar perturbations by the expanding universe
topic_facet General Relativity and Quantum Cosmology gr-qc
FOS Physical sciences
description Quantum creation processes during the very rapid early expansion of the universe are believed to give rise to temperature anisotropies and polarization patterns in the CMB radiation. These have been observed by satellites such as COBE, WMAP, and PLANCK, and by bolometric instruments placed near the South Pole by the BICEP collaborations. The expected temperature anisotropies are well-confirmed. The B-mode polarization patterns in the CMB are currently under measurement jointly by the PLANCK and BICEP groups to determine the extent to which the B-modes can be attributed to gravitational waves from the creation of gravitons in the earliest universe. It was during 1962 that I proved that quanta of the minimally-coupled scalar field were created by the general expanding FLRW universe. This was relevant also to the creation of quantized perturbations of the gravitational field, since these perturbations satisfied linear field equations that could be quantized in the same way as the minimally-coupled scalar field equation. In fact, in 1946, E.M. Lifshitz had considered the classical Einstein gravitational field in FLRW expanding universes and had shown that the classical linearized Einstein field equations reduced, in what is now known as the Lifshitz gauge, to two separate classical minimally-coupled massless scalar field equations. These field equations of Lifshitz, when quantized, correspond to the field equations for massless gravitons, one equation for each of the two independent polarization components of the spin-2 massless graviton. I will discuss this further in this article.1 1 Plenary Lecture given September 2, 2014 at the ERE2014 Conference in Valencia, Spain : Plenary Lecture given September 2, 2014 at the ERE2014 Conference in Valencia, Spain To appear in the Proceedings of the ERE2014 Conference
format Text
author Parker, Leonard
author_facet Parker, Leonard
author_sort Parker, Leonard
title Creation of quantized particles, gravitons and scalar perturbations by the expanding universe
title_short Creation of quantized particles, gravitons and scalar perturbations by the expanding universe
title_full Creation of quantized particles, gravitons and scalar perturbations by the expanding universe
title_fullStr Creation of quantized particles, gravitons and scalar perturbations by the expanding universe
title_full_unstemmed Creation of quantized particles, gravitons and scalar perturbations by the expanding universe
title_sort creation of quantized particles, gravitons and scalar perturbations by the expanding universe
publisher arXiv
publishDate 2015
url https://dx.doi.org/10.48550/arxiv.1503.00359
https://arxiv.org/abs/1503.00359
geographic South Pole
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genre South pole
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op_relation https://dx.doi.org/10.1088/1742-6596/600/1/012001
op_rights arXiv.org perpetual, non-exclusive license
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
op_doi https://doi.org/10.48550/arxiv.1503.00359
https://doi.org/10.1088/1742-6596/600/1/012001
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