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P010010-00-R - LIGO - California Institute of Technology

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167<br />

The broadband RF sideband phases are then (modulo 2π)<br />

φ ± + = ±π (5.44)<br />

φ ± s = ±2π (5.45)<br />

φ ± − = ±α = ± Ωbbδ<br />

c<br />

where δ is the macroscopic asymmetry l1 − l2.<br />

(5.46)<br />

The power and signal cavities are both relatively short (<strong>of</strong> order 10 m), which<br />

corresponds to a free spectral range <strong>of</strong> roughly 10 MHz. Even with an unlikely finesse<br />

<strong>of</strong> 1<strong>00</strong>0, the bandwidth <strong>of</strong> these cavities wouldn’t be much less than 10 kHz (for typical<br />

numbers, the bandwidth <strong>of</strong> the power/signal coupled cavity tends to be roughly 1<strong>00</strong><br />

kHz). This allows the assumption that the transmission for the DC RF sidebands and<br />

their noise sidebands is constant over the bandwidth <strong>of</strong> interest, so the dependence<br />

on the frequency <strong>of</strong> the noise sideband ±ω can be ignored.<br />

The transmissivity for the RF sidebands is derived in Appendix B.3.<br />

t± = ±tprmAbstsem sin(α ′ )g ±<br />

ifo<br />

ifo = e−i(φdt+η ± s +η ±<br />

+ )/2<br />

g ±<br />

tD±<br />

tD± = 1 − rprmAbs cos(α ′ )e −iη±<br />

+ − rsemAbs cos(α ′ )e −i(η± s +φdt) +<br />

rprmrsemA 2 bse −i(η±<br />

+ +η± s +φdt)<br />

where the primed α is defined to include the η phase as<br />

α ′ = α ∓ η ± −<br />

(5.47)<br />

(5.48)<br />

(5.49)<br />

(5.50)<br />

The approach used in this thesis is to modify the length <strong>of</strong> the signal cavity to

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