Detection of Scalar Particles in Gravitational Waves from Resonant-Mass Detectors of Spherical Shape
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چکیده
Table 1: Possible sources of GW with their typical frequency. The last column lists the way to detect such signals. Frequency (Hz) Source Detection Method 10 Primordial Anisotropy of CBR 10 Primordial, Cosmic String Timing of ms pulsars Binary Starts 10 ÷ 10 Supermassive BH Laser interferometers in space Binaries of NS or BH 10 ÷ 10 Supernovae, Pulsars Laser interferometers on earth Coalescence of NS or BH binaries 10 Supernovae, ms Pulsars Resonant-mass detectors
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تاریخ انتشار 1998