Description
We present the audible axion mechanism extended by a period of supercooling that delays the onset of axion oscillations. While the original setup relies on a large axion decay constant and coupling to a dark Abelian gauge field to produce sizable gravitational wave signals, in this talk we discuss how supercooling opens up the testable parameter space and reduces the required coupling to $\alpha \gtrsim 1$.
Added to that, we showcase that the emission of gravitational waves via the axion coupling to the Standard Model photon in the presence of Schwinger pair production becomes possible, generating a strong signal in the $\mu$Hz or ultra-high frequency range.
Primary authors
Christopher Gerlach
(Johannes Gutenberg-Universität Mainz)
Daniel Schmitt
(Goethe University Frankfurt am Main)
Prof.
Pedro Schwaller
(Johannes Gutenberg-Universität Mainz)