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Evaluation of heat extraction through sapphire fibers for the GW observatory KAGRA

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arxiv 1401.2346 v3 pith:Q365XRTI submitted 2014-01-09 astro-ph.IM physics.ins-det

classification astro-ph.IMphysics.ins-det
keywords fibersheatwillkagramirrorssapphirestageconductivity
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abstract

Currently, the Japanese gravitational wave laser interferometer KAGRA is under construction in the Kamioka mine. As one main feature, it will employ sapphire mirrors operated at a temperature of 20K to reduce the impact from thermal noise. To reduce seismic noise, the mirrors will also be suspended from multi-stage pendulums. Thus the heat load deposited in the mirrors by absorption of the circulating laser light as well as heat load from thermal radiation will need to be extracted through the last suspension stage. This stage will consist of four thin sapphire fibers with larger heads necessary to connect the fibers to both the mirror and the upper stage. In this paper, we discuss heat conductivity measurements on different fiber candidates. While all fibers had a diameter of 1.6mm, different surface treatments and approaches to attach the heads were analyzed. Our measurements show that fibers fulfilling the basic KAGRA heat conductivity requirement of $\kappa\geq $5000W/m/K at 20K are technologically feasible.

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