Formulas for GW damping and heating effects are derived for arbitrary ℓ ≥ 2, with enhanced effects suggesting higher modes are unlikely to be observed in astrophysical GW signals.
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Gravitational wave interactions with matter: beyond quadrupolar perturbations
Formulas for GW damping and heating effects are derived for arbitrary ℓ ≥ 2, with enhanced effects suggesting higher modes are unlikely to be observed in astrophysical GW signals.