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Deep Chatterjee IISER Kolkata Mentors: Koji Arai; Matthew Abernathy
Design of a Coating-less Optical Cavity based on Total Internal Reflection Deep Chatterjee IISER Kolkata Mentors: Koji Arai; Matthew Abernathy
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Why TIR Optical Cavity? Optical cavity
Typically consists of a pair of mirrors, flat or curved, facing each other to create standing wave patterns in light waves. Since only certain modes can exist in the cavity depending on the geometry, they are used for Frequency stabilization. LIGO Laboratory
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Why TIR Optical Cavity? Total Internal Reflection (TIR) cavity
It uses the phenomenon of Total Internal Reflection. Injection of light into the cavity is carried out by the means of Evanescent coupling.(see Optics Lett. 17, 5, pp ) Top view Actual Shape LIGO Laboratory
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Why TIR Optical Cavity? No mirrors used and hence no reflection coatings Brownian Thermal Noise from coatings is a big issue Coating removal is better for frequency stabilization High reflectivity without coatings can be achieved with TIR Cancelling other Thermal Noise sources is a possibility. TIR cavity is expected to be more “quiet” and is suitable for frequency stabilization LIGO Laboratory
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Thermal Noise It is the unwanted, random signal caused by Thermal Fluctuations. Thermal fluctuations affect the refractive index and the dimensions of the body due to thermal expansion. These changes adds an extra random phase to the beam which manifests as noise. Temperature change causes expansion(contraction) Beam reflecting off the surface Temperature change causes change in refractive index Optical path φ = nL changes with changing n (TR Noise) Change in position of reflection causes change in phase (TE Noise) Beam going through LIGO Laboratory
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Noise in TIR cavity TE Noise TR Noise Change in position of faces
Optical path length The optical path φ = nL is affected which results in TE and TR Noise LIGO Laboratory
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Calculating the Noise – The Fluctuation Dissipation Theorem
General case of Einstein’s theory of Brownian Motion Relation between them Fluctuations in position of Brownian particle Viscosity of the medium More general case by Callen and Welton (see Phys. Rev. 83, 34–40 (1951)) Fluctuations in a thermodynamic variable Dissipation mechanism associated Fluctuations can be calculated from the dissipation LIGO Laboratory
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Applying the FDT – The Levin’s Approach
Y. Levin applied the FDT to compute the Noise in GW test masses (see Phys. Rev. D 57, 2 (1998)) Levin’s algorithm to calculate the Noise Apply an oscillatory “force” to the system that will cause perturbation in the quantity of interest. Calculate the dissipation caused due to the applied “force”. Relate the Dissipation to the Fluctuation using the FDT. We calculate the Dissipation and relate it to the Fluctuation LIGO Laboratory
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Calculating the Thermo-Elastic Noise
The procedure of TE noise calculation following Levin’s approach, for cylindrical geometry, goes as Heat dissipation takes place Oscillatory pressure (scaled by beam intensity) is applied to reflecting surface Stresses develop Heat is generated The total power dissipation which is lost as heat is related to the temperature fluctuation by the FDT LIGO Laboratory
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Calculating the Thermo-Refractive Noise
The procedure of TR noise calculation following Levin’s approach, for cylindrical geometry, goes as Oscillatory heat source (scaled by beam intensity) is applied along beam path Heat dissipation takes place Thermal gradients develop The power dissipation as heat is related to the spectral density of TR noise by the FDT LIGO Laboratory
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Finite Element Calculation of TE and TR Noise
Finite Element Analysis (FEA) was performed using COMSOL and MATLAB. Simpler case of cylindrical cavity was tested out first. Results were compared to the analytic cases. Aim to find suitable material properties that minimizes the total TE and TR noise. Expect to look towards cancellation of TE and TR Noise. LIGO Laboratory
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Finite Element Calculation of TE and TR Noise
Cylindrical test mass cavity Radius = 0.25 [m] Height = 0.46 [m] Beam Radius = 0.09 [m] TR analytic: Phys. Rev. D 84, (2011) TE(infinite) analytic: Phys. Rev. D 62, (2000) LIGO Laboratory
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Finite Element Calculation of TE and TR Noise
Cylindrical test mass cavity Radius = 0.25 [m] Height = 0.46 [m] Beam Radius = 0.09 [m] TR analytic: Phys. Rev. D 84, (2011) TE(infinite) analytic: Phys. Rev. D 63, (2001) LIGO Laboratory
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Putting TE and TR together
With the models working fine, the effects are put together to check for any cancellation. Heat source used along laser beam path Pressure applied on the two faces Heat source and pressure is applied simultaneously to see the combined effect LIGO Laboratory
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Putting TE and TR together
Cylindrical test mass cavity Radius = 0.25 [m] Height = 0.46 [m] Beam Radius = 0.09 [m] TR analytic: Phys. Rev. D 84, (2011) TE(infinite) analytic: Phys. Rev. D 62, (2000) LIGO Laboratory
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Putting TE and TR together
Cylindrical test mass cavity Radius = 0.25 [m] Height = 0.1 [m] Beam Radius = 0.09 [m] TR analytic: Phys. Rev. D 84, (2011) TE(infinite) analytic: Phys. Rev. D 63, (2001) LIGO Laboratory
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Future Work Parametric study to bring TE and TR noise close.
Cancellation occurs when TE and TR are of same order Building the correct model for TIR cavity Calculate Noise using FEA for the same Noise Cancellation – Can it be achieved? If not cancelled, can the noise be minimized? LIGO Laboratory
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Summary and Conclusion
Simpler model has been built successfully. Special Analytic cases have been tested. Model is expected to work well for the TIR cavity Noise cancellation has to be thought about. LIGO Laboratory
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Thank you
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