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Forecasts tighten bounds on the bounce energy scale in bouncing cosmology, suggesting significant implications for early Universe gravitational wave detection.
We exploit forecast sensitivities to high frequency gravitational waves (HFGWs) from superconducting LC circuits, traditional resonant cavity and superconducting radio frequency (SRF) cavities with electromagnetic and mechanical modes to derive the first projections of the bounce energy scale within the generic bouncing cosmology framework over the frequency window $1\,$kHz f10\,GHz. In comparison with existing astrophysical limits (spanning 10⁻¹⁷\,Hz f1\,kHz and based on Planck/BICEP, PTA, and aLIGO/LISA) our HFGW forecasts yield substantially tighter constraints across a broad region of parameter space. This work unifies constraints from cosmological observations and quantum measurement experiments, providing comprehensive coverage of the early Universe gravitational wave spectrum from 10⁻¹⁷\,Hz to 10\,GHz and thereby probing the cosmic initial non singularity at ultra high energy scales.
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Changhong Li (2025) studied this question.
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