Table 3: Gravitational wave frequencies (in Hz) computed from the calculated data for GNH3, APR and BPAL12 EOSs: the $f_{\rm npm}$ denotes the frequency at which the non-point-mass effects start to be important, $f_{\rm 20}, f_{\rm 25}$ and $f_{\rm 40}$ are the so-called break-frequencies (see text), whereas $f_{\rm end}$ is the GW frequency on the final orbit.
EOS $f_{\rm npm}$ $f_{\rm 20}$ $f_{\rm 25}$ $f_{\rm 40}$ $f_{\rm end}$

GNH3 500 567 657 792 806

APR 700 615 762 1025 1132

BPAL12 1050 615 785 1160 1270

**Table 3:** Gravitational wave frequencies (in Hz) computed from the calculated data for GNH3, APR and BPAL12 EOSs: the $f_{\rm npm}$ denotes the frequency at which the non-point-mass effects start to be important, $f_{\rm 20}, f_{\rm 25}$ and $f_{\rm 40}$ are the so-called break-frequencies (see text), whereas $f_{\rm end}$ is the GW frequency on the final orbit.
EOS	$f_{\rm npm}$	$f_{\rm 20}$	$f_{\rm 25}$	$f_{\rm 40}$	$f_{\rm end}$
GNH3	500	567	657	792	806
APR	700	615	762	1025	1132
BPAL12	1050	615	785	1160	1270

Source LaTeX | All tables | In the text

	1 Introduction
	2 Description of the equations of state
	3 Numerical method
	4 Numerical results
	5 Concluding remarks
	References