g060385-00-z mentor: bill kells investigating a parametric instability in the ligo test masses hans...

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G060385-00-Z Mentor: Bill Kells Investigating a Parametric Instability in the LIGO Test Masses Hans Bantilan (Carleton College) for the LIGO Scientific Collaboration LIGO SURF, 2006 G060385-00-Z

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G Z Non-Linear Optical Interaction Mandelstam-Brillouin Scattering »Non-linear coupling of acoustic and optical waves Stokes/anti-Stokes Process »Incident ω 0 optical wave excites phonons, releasing a ω 0 - ω m optical sideband (destabilizing) »Incident ω 0 optical wave absorbs phonons, releasing a ω 0 + ω m optical sideband (damping) Parametric Instability »Ponderomotive force on test-mass »Acoustic displacements in test-mass »Under certain conditions, instability

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Page 1: G060385-00-Z Mentor: Bill Kells Investigating a Parametric Instability in the LIGO Test Masses Hans Bantilan (Carleton College) for the LIGO Scientific

G060385-00-Z Mentor: Bill Kells

Investigating a Parametric Instability in the LIGO Test Masses

Hans Bantilan (Carleton College) for the LIGO Scientific Collaboration

LIGO SURF, 2006

G060385-00-Z

Page 2: G060385-00-Z Mentor: Bill Kells Investigating a Parametric Instability in the LIGO Test Masses Hans Bantilan (Carleton College) for the LIGO Scientific

G060385-00-Z

Instabilities in Mirror Test-Masses

Problem» Acoustic modes excited by radiation pressure» Coupling of acoustic modes and optical modes

Solution» Map instability behavior of interferometer, R values » Use new FFT method for more complete R calculation

Outline» Non-Linear Optical Interaction» R values» R Pipeline» Results

Page 3: G060385-00-Z Mentor: Bill Kells Investigating a Parametric Instability in the LIGO Test Masses Hans Bantilan (Carleton College) for the LIGO Scientific

G060385-00-Z

Non-Linear Optical Interaction

Mandelstam-Brillouin Scattering» Non-linear coupling of acoustic and optical waves

Stokes/anti-Stokes Process » Incident ω0 optical wave excites phonons, releasing

a ω0 - ωm optical sideband (destabilizing)» Incident ω0 optical wave absorbs phonons, releasing

a ω0 + ωm optical sideband (damping)

Parametric Instability» Ponderomotive force on test-mass» Acoustic displacements in test-mass» Under certain conditions, instability

Page 4: G060385-00-Z Mentor: Bill Kells Investigating a Parametric Instability in the LIGO Test Masses Hans Bantilan (Carleton College) for the LIGO Scientific

G060385-00-Z

R Value

R Eigenvalue» Real part of eigenvalue of system of equations

describing » Instability for R > 1» Old “mode-pair” formulation» New “total E field” formulation

Configuration» Advanced LIGO parameters» Modelling one interferometer arm» Considering acoustic mode deformation at one

mirror

Page 5: G060385-00-Z Mentor: Bill Kells Investigating a Parametric Instability in the LIGO Test Masses Hans Bantilan (Carleton College) for the LIGO Scientific

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R Pipeline

Systematic calculation of R values» FEM package to calculate acoustic modes» FFT code to calculate optical modes» Matlab code to process acoustic and optical data» Calculate R values

1 2 3 4

Page 6: G060385-00-Z Mentor: Bill Kells Investigating a Parametric Instability in the LIGO Test Masses Hans Bantilan (Carleton College) for the LIGO Scientific

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FEM Package

FEM Configuration» 21797 nodes, 4752 elements» 17 cm radius, 20 cm thickness, 95 mm flats

Page 7: G060385-00-Z Mentor: Bill Kells Investigating a Parametric Instability in the LIGO Test Masses Hans Bantilan (Carleton College) for the LIGO Scientific

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FFT Code

FFT Configuration» 256 x 256 grids» Advanced LIGO parameters

Page 8: G060385-00-Z Mentor: Bill Kells Investigating a Parametric Instability in the LIGO Test Masses Hans Bantilan (Carleton College) for the LIGO Scientific

G060385-00-Z

Matlab CodeDynamical System, Static Model

» Dynamical system; scattering into different frequencies» Static model; no concept of time or frequency

Phase “Trick”» Only concerned with round-trip phase» Difference in frequency can be simulated by an appropriate change in

cavity length» Stokes field calculation: cavity length made shorter» Anti-Stokes field calculation: cavity length made longer

Page 9: G060385-00-Z Mentor: Bill Kells Investigating a Parametric Instability in the LIGO Test Masses Hans Bantilan (Carleton College) for the LIGO Scientific

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Verification

“Australian” Case» Acoustic mode at 28.34 kHz » R values closely correspond

Synthetic LG10 Case» Generalized Laguerre polynomial “acoustic mode”» Scattering into only LG10 optical mode; exact R expression» R value correctly predicted

R = 3.63 R = 3.71

Page 10: G060385-00-Z Mentor: Bill Kells Investigating a Parametric Instability in the LIGO Test Masses Hans Bantilan (Carleton College) for the LIGO Scientific

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Results

Page 11: G060385-00-Z Mentor: Bill Kells Investigating a Parametric Instability in the LIGO Test Masses Hans Bantilan (Carleton College) for the LIGO Scientific

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Questions?

Page 12: G060385-00-Z Mentor: Bill Kells Investigating a Parametric Instability in the LIGO Test Masses Hans Bantilan (Carleton College) for the LIGO Scientific

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Page 13: G060385-00-Z Mentor: Bill Kells Investigating a Parametric Instability in the LIGO Test Masses Hans Bantilan (Carleton College) for the LIGO Scientific

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Page 14: G060385-00-Z Mentor: Bill Kells Investigating a Parametric Instability in the LIGO Test Masses Hans Bantilan (Carleton College) for the LIGO Scientific

G060385-00-Z

φHTM ± ωmT = 2πn (resonance)

Page 15: G060385-00-Z Mentor: Bill Kells Investigating a Parametric Instability in the LIGO Test Masses Hans Bantilan (Carleton College) for the LIGO Scientific

G060385-00-Z