Gravitational waves from oscillon preheating

Oscillons are long-lived, localized excitations of nonlinear scalar fields which may be copiously produced during preheating after inflation, leading to a possible oscillon-dominated phase in the early Universe. For example, this can happen after axion monodromy inflation, on which we run our simula...

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Main Authors: Zhou, Shuang-Yong, Copeland, Edmund J., Easther, Richard, Finkel, Hal, Mou, Zong-Gang, Saffin, Paul M.
Format: Article
Published: Springer 2013
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Online Access:https://eprints.nottingham.ac.uk/42150/
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author Zhou, Shuang-Yong
Copeland, Edmund J.
Easther, Richard
Finkel, Hal
Mou, Zong-Gang
Saffin, Paul M.
author_facet Zhou, Shuang-Yong
Copeland, Edmund J.
Easther, Richard
Finkel, Hal
Mou, Zong-Gang
Saffin, Paul M.
author_sort Zhou, Shuang-Yong
building Nottingham Research Data Repository
collection Online Access
description Oscillons are long-lived, localized excitations of nonlinear scalar fields which may be copiously produced during preheating after inflation, leading to a possible oscillon-dominated phase in the early Universe. For example, this can happen after axion monodromy inflation, on which we run our simulations. We investigate the stochastic gravitational wave background associated with an oscillon-dominated phase. An isolated oscillon is spherically symmetric and does not radiate gravitational waves, and we show that the flux of gravitational radiation generated between oscillons is also small. However, a significant stochastic gravitational wave background may be generated during preheating itself (i.e, when oscillons are forming), and in this case the characteristic size of the oscillons is imprinted on the gravitational wave power spectrum, which has multiple, distinct peaks.
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spelling nottingham-421502020-05-04T16:39:30Z https://eprints.nottingham.ac.uk/42150/ Gravitational waves from oscillon preheating Zhou, Shuang-Yong Copeland, Edmund J. Easther, Richard Finkel, Hal Mou, Zong-Gang Saffin, Paul M. Oscillons are long-lived, localized excitations of nonlinear scalar fields which may be copiously produced during preheating after inflation, leading to a possible oscillon-dominated phase in the early Universe. For example, this can happen after axion monodromy inflation, on which we run our simulations. We investigate the stochastic gravitational wave background associated with an oscillon-dominated phase. An isolated oscillon is spherically symmetric and does not radiate gravitational waves, and we show that the flux of gravitational radiation generated between oscillons is also small. However, a significant stochastic gravitational wave background may be generated during preheating itself (i.e, when oscillons are forming), and in this case the characteristic size of the oscillons is imprinted on the gravitational wave power spectrum, which has multiple, distinct peaks. Springer 2013-10-03 Article PeerReviewed Zhou, Shuang-Yong, Copeland, Edmund J., Easther, Richard, Finkel, Hal, Mou, Zong-Gang and Saffin, Paul M. (2013) Gravitational waves from oscillon preheating. Journal of High Energy Physics, 2013 . 26/1-26/18. ISSN 1029-8479 Cosmology of Theories beyond the SM Solitons Monopoles and Instantons Nonperturbative Effects http://link.springer.com/article/10.1007%2FJHEP10%282013%29026 doi:10.1007/JHEP10(2013)026 doi:10.1007/JHEP10(2013)026
spellingShingle Cosmology of Theories beyond the SM
Solitons Monopoles and Instantons
Nonperturbative Effects
Zhou, Shuang-Yong
Copeland, Edmund J.
Easther, Richard
Finkel, Hal
Mou, Zong-Gang
Saffin, Paul M.
Gravitational waves from oscillon preheating
title Gravitational waves from oscillon preheating
title_full Gravitational waves from oscillon preheating
title_fullStr Gravitational waves from oscillon preheating
title_full_unstemmed Gravitational waves from oscillon preheating
title_short Gravitational waves from oscillon preheating
title_sort gravitational waves from oscillon preheating
topic Cosmology of Theories beyond the SM
Solitons Monopoles and Instantons
Nonperturbative Effects
url https://eprints.nottingham.ac.uk/42150/
https://eprints.nottingham.ac.uk/42150/
https://eprints.nottingham.ac.uk/42150/