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Development of superconducting Klystron cavity for the Mario Schenberg gravitational wave detector

机译:mario schenberg超导速调管腔的研制   引力波探测器

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摘要

Superconducting reentrant cavities can be used in parametric transducers forGravitational Wave antennas. The Mario Schenberg detector, which is being builtby the GRAVITON group at Instituto Nacional de Pesquisas Espaciais (INPE),basically consists of a resonant mass (ball) and a set of parametrictransducers in order to monitor the fundamental modes of vibration. Whencoupled to the antenna, the transducer-sphere system will work as a mass-springsystem. In this work the main task is the development of parametric transducersconsisting of reentrant superconducting cavity with high performance to beimplemented in the Mario Schenberg detector. Many geometries, materials anddesigns have been tested and compared to optimize parameters such as electricand mechanical Q-factor. The aim is the construction of a complete set of nineparametric transducers that, attached to the spherical antenna, will possiblyreach the sensitivity $h$ $\sim$ 10$^{-22}$ $Hz$$^{-1/2}$ in the near future.
机译:超导凹腔可用于重力波天线的参数换能器中。 Mario Schenberg探测器是由西班牙国家石油研究所(INPE)的GRAVITON集团建造的,主要由一个共振质量(球)和一组参量换能器组成,以监测振动的基本模式。当耦合到天线时,换能器球系统将充当质量弹簧系统。在这项工作中,主要任务是开发由可重入的超导腔构成的参数换能器,并在Mario Schenberg检测器中实现,该腔具有高性能。已测试并比较了许多几何形状,材料和设计,以优化诸如电和机械Q因子之类的参数。目的是构建一套完整的九参数传感器,该传感器连接到球形天线,将可能达到灵敏度$ h $ $ \ sim $ 10 $ ^ {-22} $ $ Hz $$ ^ {-1/2} $在不久的将来。

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