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The Optickle Optical Modeling Tool QND Workshop, Hannover Dec 15, 2005

Optickle is a new tool for modeling interferometric systems in the frequency domain. It is written in Matlab and designed for easy integration with other modeling efforts. The tool uses Matlab classes and established methods to calculate the opto-mechanical frequency response. Optickle allows for the construction of arbitrary interferometers with concrete units and various components like losses, coatings, and masses.

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The Optickle Optical Modeling Tool QND Workshop, Hannover Dec 15, 2005

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  1. The Optickle Optical Modeling Tool QND Workshop, Hannover Dec 15, 2005 Robert Ward & Matthew Evans Optickle

  2. Optickle: Frequency Domain IFO Simulation • Optickle is a new frequency domain IFO modeling tool: • Written in Matlab • Matlab allows easy integration to other modeling efforts (a frequency-domain e2e, like LinLIGO) • Easily Extensible • Uses Matlab classes for generality • Uses the methods outlined in T. Corbitt et al: “Mathematical framework for simulation of quantum fields in complex interferometers using the two-photon formalism” (LIGO-P030071-00R) to calculate the IFO opto-mechanical frequency response. • Designed for concrete units (Watts, meters, Hz) Optickle

  3. Optickle example: FP cavity • Includes losses, AR coatings, pickoff fractions, mass • Build an arbitrary IFO using Optickle class methods: • addOptic • addLink • Example: % create model opt = Optickle; % add optics [opt, snIX, nIX_HR, nIX_AR] = ... addOptic(opt, 'IX', 0.005, 00e-6, 0e-3, 0e-6, 0e-6, 4e2, 0, 10); [opt, snEX, nEX_HR, nEX_AR] = ... addOptic(opt, 'EX', 10e-6, 00e-6, 0e-3, 0e-6, 0e-6, 4e2, 0, 10); % add links opt = addLink(opt, snIX, 1, nEX_HR); opt = addLink(opt, snEX, 1, nIX_HR); [mf, mDC1, E_dc] = propFieldsP(opt,f,offsets,Lfield); bm = getIndexP(opt,snEX,'pos',0); b2f = getIndexP(opt,snIX,'b',2); exc = zeros(size(mf,1),length(f)); exc(bm,:) = 1; resp = fmult(mf,exc); mybodeplot(f,resp(b2f,:)); Optickle

  4. Optickle Example: FP cavity • Response of front mirror to back mirror ‘excitation’ • 1 nm detune • finesse ~ 1200 Optickle

  5. Optickle Example: AdLIGO DC Readout GW response, W/m 3pm DARM offset, 70ppm mismatch 40 kg Test Masses 15W Input Power 85 degree detune 70ppm loss mismatch Optickle

  6. Optickle Example: AdLIGO • Easy to create a frequency dependent coupling matrix, useful for, e.g., estimating the contribution of loop noise to DARM. Optickle

  7. Optickle status Current: • Free masses (no pendulum yet) • Carrier and signal sidebands only (no RF sidebands) • No servos • No beamsplitters (-> incorrect radiation pressure at BS) • Plane waves • No input vacuum fields Future: • Validation against theoretical calculations • Pendulum response for masses (quad?) • more high level methods (addSignal, addPD, addRFsideband, etc). • RF detection (no radiation pressure on RF sidebands?) • Vacuum noise • Force to position • servos? • Hermite Gaussian? Optickle

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