Angular and frequency response of LISA

摘要: The sensitivity of LISA at frequencies above about 10 mHz is determined by the shot noise light together with decreasing antenna transfer function, finally being limited mechanical resonances 1 Hz. In this paper we will investigate function laser-interferometric gravitational-wave antennas in upper frequency range, where physical arm length becomes comparable to or even greater than wavelength gravitational waves. This analysis reveals results which are also interesting for ground-based detectors. Furthermore, calculate dependence on orbit azimuth, source declination and polarization, form average over these angles order arrive a mean curve. It turns out that resulting response better estimated previously.