Quark stars modeled with MIT bag and CFL equations of state in f(R,Lm,T) gravity are predicted to emit gravitational wave echoes at 7.5-11 kHz, with the exact frequency depending on the coupling parameter gamma.
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Compact stars with gravitational wave echoes in $f(R,L_{m},T)$ gravitational theory
Quark stars modeled with MIT bag and CFL equations of state in f(R,Lm,T) gravity are predicted to emit gravitational wave echoes at 7.5-11 kHz, with the exact frequency depending on the coupling parameter gamma.