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Optickle for the PRFPMI at the 40m

attachment:Optickle_prfpmi_40m.zip

• In the folder 40m_PRFPMI the parameters have been set to mimic the state that the smoo_prfpmi script gets us to. See Rana's ilog entry.

• The initial conditions are such that the arms are on resonance, the MICH is at 0.8 of a bright fringe, the PRC is at resonance for the carrier (power builds up in the PRC).
• Transmission of the signal recycling mirror is set to 1 in the opt40.m parameter file.
• Slightly cleaned up version of Kirk's: attachment:powfab.zip
  • (unzip into the directory where you want your powfab Optickle files)
• Added a spob detector to opt40.m. Changed the losses of the optics to be more accurate (from 1ppm). to PR = 60ppm, SR = 60ppm, BS = 100ppm, ITMX = 100ppm, ITMY = 100ppm, ETMX = 100ppm, ETMY = 100ppm. attachment:smoo_PRFPMI.tar.gz

Optickle and Looptickle files for the DRFPMI at the 40m

Get the last version of Optickle and Looptickle http://lhocds.ligo-wa.caltech.edu:8000/advligo/ISC_Modeling_Software

OPTICKLE

Configuration files for Optickle: attachment:Optickle40m_DRFPM.zip

Run cfg40m to create an "opt" file, then run tickle

LOOPTICKLE

attachment:Looptickle40m_DRFPM.zip

"test40m.m" is the script which produces the noise budget.

N.B.: Filters and gains are the ones defined in Stefan's model "demo40m.m", TUNING NEEDS TO BE DONE.

Documentation

• [http://www.ligo.caltech.edu/docs/G/G070728-00/G070728-00.pdf Matt's document, "Optickle"]

• [http://www.ligo.caltech.edu/~rward/presentations/QND/Optickle.pdf Rob & Matt's talk, "The Optickle Optical Modeling Tool"]

• [http://www.ligo.caltech.edu/docs/P/P030071-00.pdf LIGO-P030071-00-R, Mathematical framework for simulation of quantum fields in complex interferometers. using the two-photon formalism]