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Published on: May 9, 2021
Gravitational Waves from Oscillons after Inflation
Stefan Antusch1,2, Francesco Cefalà1, Stefano Orani1
1Deparment of Physics, University of Basel, Klingelbergstr. 82, CH-4056 Basel, Switzerland.
Oscillons in asymmetric potentials significantly boost gravitational wave production after inflation. This enhanced signal improves detection prospects for gravitational wave astronomy, especially in low-scale inflation models.
Area of Science:
- Cosmology
- Gravitational Wave Physics
- Particle Physics
Background:
- Preheating after cosmic inflation is a crucial period for generating primordial gravitational waves.
- Scalar field potentials with asymmetric minima are common in inflationary models.
- Oscillons, localized large-amplitude oscillations, can form during preheating.
Purpose of the Study:
- To investigate gravitational wave production during preheating with asymmetric scalar field potentials.
- To analyze the specific role and impact of oscillons in these asymmetric scenarios.
- To compare findings with previous studies on symmetric potentials.
Main Methods:
- Numerical simulations of scalar field dynamics during preheating.
- Analysis of the resulting gravitational wave spectrum.
- Comparison of results for asymmetric versus symmetric potentials.
Main Results:
- Oscillons in asymmetric potentials generate a pronounced peak in the gravitational wave spectrum.
- This peak significantly exceeds the spectrum predicted by linear preheating.
- The amplitude enhancement is substantial compared to symmetric potential scenarios.
Conclusions:
- Asymmetric potentials and oscillons play a critical role in gravitational wave production during preheating.
- The enhanced gravitational wave signal offers improved observational prospects for detectors.
- This finding has significant implications for testing low-scale inflation models.
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