Abstract
We propose a new method of gravitational wave detection in the 10−1÷ 10−2Hz band for a space laboratory based on the use of the Kozorez effect in the magnetic interaction of superconducting solenoids.
Similar content being viewed by others
References
Thorne, K. S. (1980).Rev. Mod. Phys. 52, 285.
Braginsky, V. B., Thorne, K. S. (1985).Nature 316, 610.
Chan, H. A., and Paik, H. J. (1987).Phys. Rev. D 35, 3551.
Kozorez, V. V. (1981).Dynamics of the magnetic interacting bodies systems (Naukova dumka, Kiev, in Russian).
Blaquier, A. (1966).Nonlinear systems analysis (Academic, New York and London).
Chadrasekhar, S. (1943).Rev. Mod. Phys. 15, 1.
Van Duser, T., and Terner, C. W. (1981).Principles of superconductive devices and circuits (Elsevier, North Holland).
Schwartz, B. B., and Foner, S., eds. (1977)Superconductor Application: SQUIDs and Machines (Plenum Press, New York).
Blaser, J. P., at al. (1993).STEP (Satellite Test of the Equivalence Principle). Report on the Phase A study. ESA and NASA, SCI(93)4 March 1993.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Verozub, L.V. Earth-orbiting low-frequency gravitational wave detector. Gen Relat Gravit 28, 77–86 (1996). https://doi.org/10.1007/BF02106855
Received:
Issue Date:
DOI: https://doi.org/10.1007/BF02106855