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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Presentation transcript:

G 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 G Z

G 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

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

G 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

G Z 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 12 34

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

G Z FFT Code FFT Configuration » 256 x 256 grids » Advanced LIGO parameters

G Z Matlab Code Dynamical 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

G Z Verification “Australian” Case » Acoustic mode at 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 = 3.63R = 3.71

G Z Results

G Z Questions?

G Z

φ HTM ± ω m T = 2πn (resonance)

G Z