The effective f-number
For a Gaussian beam incident on a focusing lens, define \(D_{\mathrm{beam}}=2\omega_L\) using the 1/e² beam radius \(\omega_L\) at the lens. The effective f-number is
\[ N\equiv f/\#=\frac{f}{D_{\mathrm{beam}}}=\frac{f}{2\omega_L} \]A smaller \(N\) means a wider converging cone and tighter focusing; a larger \(N\) means a gentler, more paraxial cone.
Relation to numerical aperture
With refractive index \(n\) around the focus and cone half-angle \(\alpha\),
\[ \mathrm{NA}_{\mathrm{eff}} =n\sin\alpha =n\sin\!\left[\arctan\!\left(\frac{1}{2N}\right)\right] \approx\frac{n}{2N} \]The last form is the small-angle approximation. In air, \(N=2\) gives \(\mathrm{NA}_{\mathrm{eff}}\approx0.24\).
Use the illuminated diameter
A lens datasheet usually computes f-number from its clear aperture. That is the correct effective value only when the beam fills the aperture. If the beam underfills the lens, use \(2\omega_L\): the effective NA is lower and the effective f-number is higher than the datasheet value.
A practical design check
For \(N\gtrsim2\), equivalently \(\mathrm{NA}_{\mathrm{eff}}\lesssim0.25\) in air, paraxial Gaussian formulas are generally reliable for design. Below that, use them as a first-order estimate and consider a vector diffraction model when accurate high-NA focal fields matter.