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FINESSE FINESSE Frequency Domain Interferometer Simulation Andreas Freise European Gravitational Observatory 17. March 2004
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FINESSE Frequency Domain Interferometer Simulation

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FINESSE Frequency Domain Interferometer Simulation. Andreas Freise European Gravitational Observatory 17 . March 2004. Possible Outputs of FINESSE. light power, field amplitudes eigenmodes, beam shape error/control signals (modulation-demodulation) - PowerPoint PPT Presentation
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Page 1: FINESSE Frequency Domain Interferometer Simulation

FINESSEFINESSE

Frequency Domain Interferometer Simulation

Andreas Freise

European Gravitational Observatory

17. March 2004

Page 2: FINESSE Frequency Domain Interferometer Simulation

5. September 2003 Andreas Freise

Page 3: FINESSE Frequency Domain Interferometer Simulation

5. September 2003 Andreas Freise

light power, field amplitudes

eigenmodes, beam shape

error/control signals

(modulation-demodulation)

transfer functions, sensitivities,

noise couplings

alignment error signals, mode

matching, etc.

Possible Outputs of FINESSE

Page 4: FINESSE Frequency Domain Interferometer Simulation

5. September 2003 Andreas Freise

Plane Waves – Frequency Domain

Coupling of light fields:

Set of linear equations: solved numerically

Page 5: FINESSE Frequency Domain Interferometer Simulation

5. September 2003 Andreas Freise

Frequency Domain

Simple cavity: two mirrors + one space (4 nodes)

Light source (laser)

Output signal (detector)

Page 6: FINESSE Frequency Domain Interferometer Simulation

5. September 2003 Andreas Freise

Frequency Domain

one Fourier frequency

one complex output signal

Page 7: FINESSE Frequency Domain Interferometer Simulation

5. September 2003 Andreas Freise

Static response

phase modulation = sidebands

3 fields, 3 beat signals

Page 8: FINESSE Frequency Domain Interferometer Simulation

5. September 2003 Andreas Freise

Frequency Response

infenitesimal phase modulation

9 frequencies, 13 beat signals

Page 9: FINESSE Frequency Domain Interferometer Simulation

5. September 2003 Andreas Freise

Gaussian Beam Parameters

Compute cavity eigenmodes

start node

Trace beam and set beam parameters

Page 10: FINESSE Frequency Domain Interferometer Simulation

5. September 2003 Andreas Freise

Mode Mismatch and Misalignment

Mode mismatch or misalignemt can be described as light scatteringin higher-order spatial modes. Coupling coefficiants for the interferometer matrix are derived by projecting beam 1 on beam 2:

Page 11: FINESSE Frequency Domain Interferometer Simulation

5. September 2003 Andreas Freise

FINESSE: Fast and (fairly) well tested

TEM order O matrix elements (effective)computation time (100 data points)

0 ~25000 340 <1 sec

5 ~11000000 83000 400 sec

Example: Optical layout of GEO 600 (80 nodes)

The Hermite-Gauss analysis has been validated by:

computing mode-cleaner autoalignment error signals (G. Heinzel) comparing it to OptoCad (program for tracing Gaussian beams by

R. Schilling) comparing it to FFT propagation simulations (R. Schilling)

Page 12: FINESSE Frequency Domain Interferometer Simulation

5. September 2003 Andreas Freise

Power Recycling Signals

Page 13: FINESSE Frequency Domain Interferometer Simulation

5. September 2003 Andreas Freise

FINESSEFINESSE

http://www.rzg.mpg.de/~adf/

/virgo/VCS/1.0/VIRGOSW/Finesse/v0r93/...

Windows, Linux

Linux, AIX

Page 14: FINESSE Frequency Domain Interferometer Simulation

5. September 2003 Andreas Freise

Page 15: FINESSE Frequency Domain Interferometer Simulation

5. September 2003 Andreas Freise

Using Par-Axial Modes

Hermite-Gauss modes allow to analyse the optical system with respect to alignment and beam shape.

Both misalignment and mismatch of beam shapes (mode mismatch) can be described as scattering of light into higher-order spatial modes.

This means that the spatial modes are coupled where an opticalcomponent is misaligned and where the beam sizes are notmatched.

Page 16: FINESSE Frequency Domain Interferometer Simulation

5. September 2003 Andreas Freise

From Plane Waves to Par-Axial Modes

The electric field is described as a sum of the frequency components and Hermite-Gauss modes:

Example: lowest-order Hermite-Gauss:

Gaussian beam parameter q

Page 17: FINESSE Frequency Domain Interferometer Simulation

5. September 2003 Andreas Freise

Gaussian Beam Parameters

Example: normal incidence transmission through a curved surface:

Transforming Gaussian beam parameters by optical elements with ABCD matrices:

Page 18: FINESSE Frequency Domain Interferometer Simulation

5. September 2003 Andreas Freise

Frequency Noise Coupling

Coupling of a frequency calibration peak into the dark fringe output:

Difference between results forTEM00 only and those withhigher-order TEM modes: factor 100 phase 90°

Page 19: FINESSE Frequency Domain Interferometer Simulation

5. September 2003 Andreas Freise

Mode Healing

1.0 0.1 0.01

TMSR

Page 20: FINESSE Frequency Domain Interferometer Simulation

5. September 2003 Andreas Freise

Mode Healing

power recycling only:

Each recycling cavity minimises the loss due to mode mismatch of the respective other

with signal recycling:

Page 21: FINESSE Frequency Domain Interferometer Simulation

5. September 2003 Andreas Freise

Error signals, control signals

photo detectors, multiple

mixers

Transfer functions

amplitude-, phase- and

frequency modulations

Shot-noise-limited

sensitivities

Typical Tasks For FINESSE

Page 22: FINESSE Frequency Domain Interferometer Simulation

5. September 2003 Andreas Freise

FINESSE:

Versatile simulation software for user-defined interferometer topologies. Fast, easy to use.

Higher-order spatial modes:

Commissioning of interferometers with high- finesse cavities requires to understand the influences of mode-matching and alignment on control signals and noise couplings.