arXiv · 2402.16152
Gravitational Waves from Kinetic Preheating
Abstract
We study gravitational wave production during kinetic preheating after inflation with a focus on scenarios that arise in $\alpha$-attractor models where a scalar dilaton-like inflaton is kinetically coupled to a second scalar field. We present high-resolution lattice simulations of three $\alpha$-attractor models for a range of parameters to probe regions where preheating is efficient. We find that preheating in these models can be extremely violent, resulting in gravitational wave energy densities that can be constrained by cosmic microwave background measurements of the effective number of relativistic species, $N_{\rm eff}$
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
Peter Adshead, John T. Giblin Jr, Avery Tishue. 2024-02-25. Gravitational Waves from Kinetic Preheating. https://arxiv.org/abs/2402.16152
Cite the original work for its findings. Save a collection to share your selection of sources.