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Oscillations, Waves, and Interactions - GWDG

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288 Schreiber<br />

<strong>and</strong> it is currently believed that the respective mirror coatings exhibit some minute<br />

non-isotropy, causing the cavity Q to be different for the two senses of propagation.<br />

For a model accounting for dispersive frequency detuning <strong>and</strong> hole burning [12] the<br />

bias due to the corresponding null shift offset becomes<br />

∆f0 = c<br />

2P ·<br />

�<br />

ξ Zi(ξ)<br />

L(ξ)<br />

η Zi(0) G<br />

�<br />

· ∆I , (7)<br />

with ξ the cavity detuning from line center, Z(ξ) the imaginary part of the dispersion<br />

function, G the gain, <strong>and</strong> ∆I the observed difference in intensity. Equation (7) also<br />

shows that it is very important to keep the gain constant, which is very difficult for a<br />

gas laser in the presence of gain medium degradation through outgassing inside the<br />

cavity.<br />

6.2 Backscatter coupling<br />

In the presence of strong backscattering, light of one sense of propagation is coupled<br />

into the beam travelling into the opposite direction. According to Ref. [9] the beat<br />

frequency disappears if the experienced rotation rate falls below a threshold value of<br />

ωL = cλ2√rs . (8)<br />

32πAd<br />

A is the area enclosed by the cavity, d the diameter of the beam, <strong>and</strong> rs the amount<br />

of backscatter contribution of the mirror. In the most general case the shifted beat<br />

frequency then becomes<br />

∆f = 4A<br />

�<br />

ω<br />

λP<br />

2 − ω2 L , (9)<br />

where ω is the experienced rate of rotation of the gyro. For ring lasers of the size<br />

of C-II or smaller, ωL can be of a significant amount, however far from locking up<br />

with the Earth rate as the only source of rotation, while neither G nor any of the<br />

UG ring lasers ever showed much evidence for the presence of backscatter at all. For<br />

this situation the contribution to backscatter is best expressed as<br />

∆fbs = c<br />

2P (ρ2 sin(ψ + ɛ2) + ρ1 sin(ψ + ɛ1)) , (10)<br />

where ɛ1 <strong>and</strong> ɛ2 are the respective backscatter phase angles <strong>and</strong> ρ1 <strong>and</strong> ρ2 the corresponding<br />

backscatter amplitudes. Following Ref. [12] one can write<br />

ρ1 = rsλ<br />

�<br />

I1<br />

, ρ2 =<br />

4d I2<br />

rsλ<br />

�<br />

I2<br />

, (11)<br />

4d I1<br />

with I1, I2 the respective intensities of the two beams. As one can see from Eqs. (10)<br />

<strong>and</strong> (11) together, the effect of backscattering reduces with growing size of the cavity<br />

<strong>and</strong> lower scattering amplitude. In particular, the reduction of backscattering<br />

through a limited acceptance angle of the solid angle where all the light was scattered<br />

into, seems to be a very effective process.

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