Numerical simulations show oscillons form and dominate for an extended period in Palatini gravity with non-minimal coupling, producing ultra-high-frequency gravitational waves potentially accessible to future detectors.
Frolov,DEFROST: a new code for simulating preheating after inflation,Journal of Cosmology and Astroparticle Physics2008(2008) 009
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Oscillon Formation in Palatini Modified Gravity Theories
Numerical simulations show oscillons form and dominate for an extended period in Palatini gravity with non-minimal coupling, producing ultra-high-frequency gravitational waves potentially accessible to future detectors.