Table 3: Value of the orbital frequencies at the parametric resonance radii for the first five orders n in the general relativistic case. The results are given for a $1.4~{M_\odot}$ neutron star rotating at 300 and $600~{\rm Hz}$ respectively. The value to the left of the symbol / corresponds to the absolute value sign taken to be - and on the right to be +.
rank n Orbital frequency $\nu(r,a_*)$ (Hz)

Vertical Radial

$\nu_*=600$ Hz $\nu_*=300$ Hz $\nu_*=600$ Hz $\nu_*=300$ Hz

1 -- / 200 -- / 100 1596 / 220 1332 / 106

2 -- / 301 -- / 150 1196 / 330 800 / 159

3 1695 / 361 885 / 180 980 / 392 573 / 190

4 1175 / 401 597 / 200 870 / 432 480 / 210

5 988 / 430 498 / 214 808 / 459 433 / 223

**Table 3:** Value of the orbital frequencies at the parametric resonance radii for the first five orders n in the general relativistic case. The results are given for a $1.4~{M_\odot}$ neutron star rotating at 300 and $600~{\rm Hz}$ respectively. The value to the left of the symbol / corresponds to the absolute value sign taken to be - and on the right to be +.
rank n	Orbital frequency $\nu(r,a_*)$ (Hz)
	Vertical	Radial
	$\nu_*=600$ Hz	$\nu_*=300$ Hz	$\nu_*=600$ Hz	$\nu_*=300$ Hz
1	-- / 200	-- / 100	1596 / 220	1332 / 106
2	-- / 301	-- / 150	1196 / 330	800 / 159
3	1695 / 361	885 / 180	980 / 392	573 / 190
4	1175 / 401	597 / 200	870 / 432	480 / 210
5	988 / 430	498 / 214	808 / 459	433 / 223

Source LaTeX | All tables | In the text

	1 Introduction
	2 The initial conditions
	3 Linear analysis
	4 Simplified analysis
	5 Numerical simulations
	6 Conclusion
	References
	Online Material
	Appendix A: Eigenvalue problem for the Lagrangian displacement
	Appendix B: Approximate solution to the Schrödinger type equation
	Appendix C: Derivation of the resonance conditions