Gravitational Waves from Oscillon Preheating
Shuang-Yong Zhou, Edmund J. Copeland, Richard Easther, Hal Finkel, Zong-Gang Mou, Paul M. Saffin
TL;DR
The paper investigates the stochastic gravitational wave background arising from oscillon preheating after inflation, focusing on an oscillon-dominated phase and using an axion monodromy-type potential as a representative model. It shows that isolated, spherically symmetric oscillons do not radiate efficiently, and that GW production during the fully formed oscillon era is suppressed, while violent preheating during oscillon formation can generate a significant background with a spectrum featuring multiple peaks corresponding to oscillon scales. The authors support these conclusions with semi-analytic arguments and detailed lattice simulations, revealing a characteristic four-stage evolution of the GW spectrum and highlighting the high frequencies and low amplitudes expected in such scenarios. The results have implications for the phenomenology of monodromy inflation and offer spectral signatures that, while difficult to detect with current technology, could serve as a diagnostic for post-inflationary dynamics in high-scale inflation models.
Abstract
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.
