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Development of a radio-frequency, superconducting, electromechanical transducer.

机译:射频超导机电换能器的开发。

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This project concerns the theory, design, fabrication, and experimental testing of an ultrasensitive, electromechanical transducer for use on gravitational wave antennae. The transducer converts small, audio-frequency vibrations to a radio-frequency, electrical signal.; The system employs a resonant bridge circuit, driven at a "pump" frequency between 100 and 300 MHz. The circuit is capacitively coupled to a mechanical, test mass, which vibrates at approximately 1 kHz. The motion of the test mass, by changing the bridge capacitors, modulates the pump voltage to produce an excitation at the output terminals of the bridge. The output signal contains a signal at the pump frequency, with 1 kHz sidebands caused by the mechanically induced modulation. It is by observing these sidebands that a mechanical signal can be detected.; Techniques have been employed to minimize several important sources of noise. To reduce the Johnson noise in the electrical circuit, the bridge is constructed entirely of superconducting niobium and low-loss dielectrics. To allow the circuit to be superconducting and to decrease the Brownian motion of the mechanical system, the detector is cooled to liquid helium temperature. The bridge is balanced with piezoelectric tuners so that the size of the pump frequency signal, with its added phase noise, is minimized with respect to the mechanically induced sidebands.; The transducer, which has a 0.080 kg test mass, is affixed to the end of a resonant bar, gravity wave antenna with a mass of approximately 100 kg. The primary purpose of this small antenna is to evaluate the transducer, which is designed ultimately to be mounted on a full-size, 2000 kg antenna. Theory and testing of the detector indicate a noise temperature of 1.812 K using the 100 kg bar. This corresponds to a gravity wave burst sensitivity of 1.14 {dollar}times{dollar} 10{dollar}sp{lcub}-16{rcub}{dollar}, in terms of relative strain amplitude. If tuned and installed on a 2000 kg antenna, the transducer is predicted to obtain a noise temperature of 1.27 mK, which is equivalent to a burst sensitivity of 5.67 {dollar}times{dollar} 10{dollar}sp{lcub}-19{rcub}{dollar}.
机译:该项目涉及用于重力波天线的超灵敏机电换能器的理论,设计,制造和实验测试。换能器将小的音频振动转换为射频电信号。该系统采用谐振电桥电路,该电桥电路以100至300 MHz之间的“泵”频率驱动。电路与机械测试块电容耦合,该测试块以大约1 kHz的频率振动。通过改变电桥电容器,测试质量的运动会调制泵浦电压,以在电桥的输出端产生激励。输出信号包含泵浦频率的信号,该信号具有由机械感应调制引起的1 kHz边带。通过观察这些边带可以检测到机械信号。已经采用了使一些重要噪声源最小化的技术。为了减少电路中的约翰逊噪声,该桥完全由超导铌和低损耗电介质构成。为了使电路超导并降低机械系统的布朗运动,将检测器冷却至液氦温度。该电桥由压电调谐器平衡,因此泵浦频率信号的大小以及其附加的相位噪声相对于机械感应边带最小。具有0.080千克测试质量的换能器固定在质量约为100千克的共振棒重力波天线的末端。这种小天线的主要目的是评估传感器,该传感器最终设计为安装在2000 kg的全尺寸天线上。探测器的理论和测试表明,使用100 kg bar时,噪声温度为1.812K。就相对应变幅度而言,这对应于1.14倍(美元)10 {美元} sp {lcub} -16 {rcub} {美元}的重力波猝发敏感性。如果将其调谐并安装在2000 kg的天线上,则预计该换能器将获得1.27 mK的噪声温度,这相当于5.67 {dolal} times {dollar} 10 {dollar} sp {lcub} -19 { rcub} {dollar}。

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