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Spectral characteristics of ultrashort pulses in Kerr-lens - TU Wien

Spectral characteristics of ultrashort pulses in Kerr-lens - TU Wien

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= (11)<br />

= (12)<br />

It should be noted, that <strong>in</strong> these equations w, — w8 = 1, and there is the pair-wise <strong>in</strong>teraction <strong>of</strong> the spectral<br />

components with<strong>in</strong> the wide enough generation spectrum.<br />

There are two ma<strong>in</strong> mechanisms <strong>of</strong> the generation <strong>of</strong> the <strong>in</strong>itial seed at the Stokes frequency for Eqs. (3). The<br />

first one is the spontaneous Raman scatter<strong>in</strong>g with the <strong>in</strong>crements <strong>of</strong> the scattered <strong>in</strong>tensity growth<br />

2 2 S<br />

wpw8n8 gj<br />

Xi nfl. ' (13)<br />

irc2 [1—exp(—_)]<br />

where n8 is the <strong>in</strong>dex <strong>of</strong> refraction at Stokes frequency, T is the temperature, and kB is the Boltzmann's constant<br />

13<br />

With this seed signal, the stimulated Raman scatter<strong>in</strong>g results <strong>in</strong> appearance and growth <strong>of</strong> spectral replicas <strong>of</strong><br />

the ma<strong>in</strong> oscillation pulse, shifted to the lower frequencies by the Raman frequencies 1Z.<br />

More significant source for Stokes component's amplification, however, is the broad-band pulse field itself. When<br />

the pulse pulse spectrum is wide enough to become comparable with the Raman frequency shift, the lower-frequency<br />

part <strong>of</strong> the spectrum can play a role <strong>of</strong> the Stokes component seed with respect to the higher-frequency part <strong>of</strong> the<br />

spectrum. The stimulated Raman scatter<strong>in</strong>g then transfers the energy form the higher-frequency components to the<br />

lower-frequency ones, result<strong>in</strong>g <strong>in</strong> the cont<strong>in</strong>uous red-shift <strong>of</strong> the pulse spectrum as a whole. As the field amplitude<br />

<strong>of</strong> the laser pulse significantly exceeds the spontaneous seed, the second mechanism strongly dom<strong>in</strong>ates over the first<br />

one. However, we <strong>in</strong>cluded both mechanisms <strong>in</strong> our model, because their <strong>in</strong>fluence on the pulse spectrum is quite<br />

different.<br />

Later on it is convenient to normalize the time to the <strong>in</strong>verse ga<strong>in</strong> bandwidth tg 2.25 fs and the <strong>in</strong>tensity to<br />

/9', result<strong>in</strong>g <strong>in</strong> the normalization <strong>of</strong> the field energy to (flt9)1. As already po<strong>in</strong>ted out, we analyzed the described<br />

above model <strong>in</strong> two ways: on the basis <strong>of</strong> distributed and discrete-element approaches. In the framework <strong>of</strong> the<br />

distributed model, we didn't consider the propagation through the <strong>in</strong>dividual laser element and supposed that the<br />

pulse envelope is formed by the overall net-dispersion <strong>in</strong> the cavity. As result we have a split-step scheme describ<strong>in</strong>g<br />

<strong>ultrashort</strong> pulse propagation from z to z + 1 transits:<br />

a(z', t)<br />

=f ...f a(z, t')C(t — t')L (t' t") A (t" — t"') G (t"<br />

— t") dt'dt"dt'"dt', (14)<br />

a(z+1,t)=a(z',t)exp (— 2 _iIa(zI,t)I2, (15)<br />

\ 1+oia(z',t)I I<br />

a(z + 1) = a(z)exp<br />

(_rf<br />

fa(z, t')2 dt' — Tcav/Tr — + Pamax (1 exp FTcav/Tr — F))<br />

where r = t9/(E3fl) = 0.00079 is the normalized ga<strong>in</strong> saturation parameter. The Green's functions A, L, C describe<br />

spectral bands <strong>of</strong> ga<strong>in</strong>, reabsorption and output loss, respectively (note, that the dispersion is already is <strong>in</strong>cluded <strong>in</strong><br />

(16)<br />

Proc. SPIE Vol. 4752 19<br />

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