Mechanical loss associated with silicate bonding of fused silica

We report on mechanical loss associated with hydroxy-catalysis (or 'silicate') bonding between fused silica substrates in the presence of potassium hydroxide or sodium silicate. We measured the mechanical quality factor of three fused silica samples, each composed of two half-rods bonded together on their flat surfaces and compared them to that of an unbonded half-rod. The measurements show a significant reduction of quality factor due to mechanical loss associated with the silicate bonds. We calculate the loss factor of the bonded region bond and estimate that the effect of silicate bonding on thermal noise in the Advanced LIGO interferometers will be small.

[1]  M. Fejer,et al.  The intrinsic mechanical loss factor of hydroxy-catalysis bonds for use in the mirror suspensions of gravitational wave detectors , 2003 .

[2]  K. Kawabe,et al.  Study of the thermal noise caused by inhomogeneously distributed loss , 2002 .

[3]  M. Fejer,et al.  Thermal noise in interferometric gravitational wave detectors due to dielectric optical coatings , 2001, gr-qc/0109073.

[4]  M. Fejer,et al.  Excess mechanical loss associated with dielectric mirror coatings on test masses in interferometric gravitational wave detectors , 2001, gr-qc/0109074.

[5]  Joshua R. Smith,et al.  High quality factor measured in fused silica , 2000, gr-qc/0009035.

[6]  Thermoelastic noise and homogeneous thermal noise in finite sized gravitational-wave test masses , 2000, gr-qc/0002055.

[7]  M. Fejer,et al.  Investigation of mechanical loss factors of some candidate materials for the test masses of gravitational wave detectors , 2000 .

[8]  G. Harry,et al.  Dissipation of mechanical energy in fused silica fibers , 1999, physics/9904015.

[9]  Peter R. Saulson,et al.  Dissipation mechanisms in pendulums and their implications for gravitational wave interferometers , 1998 .

[10]  Sheila Rowan,et al.  Mechanical losses associated with the technique of hydroxide-catalysis bonding of fused silica , 1998 .

[11]  Y. Levin Internal thermal noise in the LIGO test masses: A direct approach , 1997, gr-qc/9707013.

[12]  S. Rowan,et al.  The quality factor of natural fused quartz ribbons over a frequency range from 6 to 160 Hz , 1997 .

[13]  Joshua R. Smith,et al.  LIGO: the Laser Interferometer Gravitational-Wave Observatory , 1992, Science.

[14]  A. Abramovici,et al.  Measuring high mechanical quality factors of bodies made of bare insulating materials , 1988 .

[15]  J. Weber Gravitational Wave Experiments , 1985 .