LIGO-G020276-00-D Fused Silica Suspensions Phil Willems LIGO/Caltech Elba GWADW Meeting May 19-26, 2002.

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LIGO-G D Fused Silica Suspensions Phil Willems LIGO/Caltech Elba GWADW Meeting May 19-26, 2002

LIGO-G D 2

3 Justification for Silica Metal wire suspension thermal noise dominates in the low audio frequency range Best metal wires get about Q= for violin modes (Niobium flexures approach 10 7 ) Very high intrinsic Q of fused silica, plus other nice mechanical properties, allow far lower thermal noise Estimates are that suspension noise will drop below radiation pressure noise in AdLIGO

LIGO-G D 4 Thermal noise, metal vs. silica Red: metal Black: silica

LIGO-G D 5 What’s so nice about silica Intrinsic Q is very high (8x10 7 and climbing) Surface losses limit this, but still to very high values Thermal expansion low, giving small thermoelastic damping Young’s modulus increases with temperature, allowing cancellation of nonlinear thermoelastic damping Silica is strong (same yield load as same diameter steel) But has lower elastic modulus, so less bending stiffness, higher dilution

LIGO-G D 6 Size Dependence of Fiber Loss Loss inversely proportional to volume/surface ratio Data from Syracuse group

LIGO-G D 7 Q of Typical Silica Fiber intrinsic loss, thermoelastic loss,

LIGO-G D 8 Nonlinear Thermoelastic Damping Loss function  : Note: true only for u large compared to oscillation strain

LIGO-G D 9 Typical silica fiber strengths

LIGO-G D 10 Some Notable Results Intrinsic Q=8x10^7 for thick annealed rod (Syracuse) Pendulum Q=2.5x10^8 for bifilar torsional pendulum (Moscow/Glasgow) Violin Q=5.2x10^8 (Caltech) Vertical Bounce Q=1.2x10^7 (Caltech)

LIGO-G D 11 Alternative Suspension Geometries Fiber- easy to make, low thermal noise, diameter fixed by NTE Ribbon- somewhat harder to make, but aspect ratio can be chosen to push increased NTE damping to higher frequency, allowing cross section choice to set vertical bounce frequency Dumbbell fiber- somewhat harder to make, optimizes end diameters for NTE and middle diameter for lower vertical bounce frequency

LIGO-G D 12 Thermal noise of fibers and ribbons Note: assumes AdLIGO suspension parameters Red: fiber Blue: ribbon Black: dumbbell fiber

LIGO-G D 13 Difficulties, Peculiarities, and Work To Be Done Quartz suspensions are very brittle, need tender loving care. Silica fibers are welded, not clamped, into suspension. Effects of welding attachments and tapered ends must be considered. Demonstration of expected high Q’s still elusive. Stress dependence of loss not yet known. Excess noise in fused silica not yet known. Violin modes have such high Q that they interfere with interferometer control and must be damped.

LIGO-G D 14 Influence of Welded Pins on Suspension Q The program that models dumbbell fibers can easily model the welded pins on the ends of suspension fibers (good approximation if pins are relatively long and thin) Used this analysis to confirm Mitrofanov and Tokmakov’s estimate of Q limit due to lossy pins Our result: this is substantially correct, although for thicker fibers the torque also plays a significant role. Basic result: A reasonably good, reasonably short pin will not unduly influence Q or thermal noise.

LIGO-G D 15 Influence of Taper Ends on Suspension Loss Suspension fibers drawn from rod stock often retain thick rod ends for ease in welding. The tapered transition from fiber to end increases the effective thickness of the fiber and reduces the dissipation dilution. Assuming diameter-independent loss (not strictly true), finite-element models show factor of two reduction of violin mode Q for typical suspension experimental parameters due to tapers.

LIGO-G D Silica Suspension Research at Caltech P. Willems, V. Sannibale, V. Mitrofanov, J. Weel, M. Thattai, A. Heptonstall, J. Johnson, D. Berns

LIGO-G D 17 Suspensions Research 2,600 Years Ago

LIGO-G D 18 Suspensions Research Today Automated fiber pulling lathe Q-measurement rig

LIGO-G D 19

LIGO-G D 20 Welded Fiber End

LIGO-G D 21 Measurement of (dE/dT)/E from Temperature Shift of Unloaded Fiber Mode Frequencies

LIGO-G D 22 Mode Frequencies: theory vs. experiment

LIGO-G D 23 Temperature Shift of the Violin Modes Yields the Dilution Factor For this suspension, In general,

LIGO-G D 24 Good Agreement with Theory data otheory

LIGO-G D 25 Q of Typical Silica Fiber intrinsic loss, thermoelastic loss,

LIGO-G D 26 Q’s of the Violin Modes theory, with NTE theory, w/o NTE and  x10 -7 /K data

LIGO-G D 27 Vertical Bounce Apparatus isolation mass test mass tensioner

LIGO-G D 28 Vertical Bounce Ringdown (first result) Q=1.25e7 Note: this fiber under the same stress planned for AdLIGO

LIGO-G D 29 Q of Typical Silica Fiber