用于引力微波的超导微镜
Laboratory-Scale Superconducting Mirrors for Gravitational Microwaves
摘要：
当一个微波频率的引力波撞击到一个薄的I型超导薄膜上时，由于不确定原理，薄膜中带负电的库珀对的自由基离域，使它们经历相对于退相干的测地线运动的非测地线运动，薄膜晶格中带正电的离子的测地线运动是由于等效原理。随后的电荷分离导致虚拟等离子体激发。这种“海森堡-库仑”效应极大地增强了引力波与超导体之间的相互作用，使得即使是非常薄的超导薄膜也会反射引力波。这一结果是用BCS理论和超导等离子体模型给出的。
英文摘要：
When a gravitational wave at microwave frequencies impinges on a thin, type I superconducting film, the radical delocalization of the film's negatively charged Cooper pairs, which is due to the Uncertainty Principle, causes them to undergo non-geodesic motion relative to the geodesic motion of the decohered, positively charged ions in the film's lattice, which is due to the Equivalence Principle. The ensuing charge separation leads to a virtual plasma excitation. This "Heisenberg-Coulomb" effect enormously enhances the interaction of a gravitational wave with a superconductor relative to that of normal matter, so that the wave will be reflected even from a very thin superconducting film. This result is presented using the BCS theory and a superconducting plasma model.
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