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- W1515053378 abstract "Perfect porcupines are specially-configured networks of gravitational wave detectors, in the limit that the individual detectors and the distances between them are short relative to the gravitational wavelengths of interest. They have beautiful properties which make them ideal gravitational wave telescopes. I present the most important cases explicitly. For a network of one-arm detectors (like AGIS cite{Dimopoulos_et_al}), the minimal perfect porcupine has 6 detectors, oriented along the 6 diameters of a regular icosahedron. For a network of two-arm detectors (like the equal-arm Michelson interferometers LIGO/VIRGO) the minimal perfect porcupine is a certain 5 detector configuration." @default.
- W1515053378 created "2016-06-24" @default.
- W1515053378 creator A5047296137 @default.
- W1515053378 date "2010-03-25" @default.
- W1515053378 modified "2023-09-27" @default.
- W1515053378 title "Perfect porcupines: ideal networks for low frequency gravitational wave astronomy" @default.
- W1515053378 hasPublicationYear "2010" @default.
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