Picture of a black hole

Strathclyde Open Access research that creates ripples...

The Strathprints institutional repository is a digital archive of University of Strathclyde's Open Access research outputs. Strathprints provides access to thousands of research papers by University of Strathclyde researchers, including by Strathclyde physicists involved in observing gravitational waves and black hole mergers as part of the Laser Interferometer Gravitational-Wave Observatory (LIGO) - but also other internationally significant research from the Department of Physics. Discover why Strathclyde's physics research is making ripples...

Strathprints also exposes world leading research from the Faculties of Science, Engineering, Humanities & Social Sciences, and from the Strathclyde Business School.

Discover more...

Gravitational modelling of the test masses for STEP and LISA

Lockerbie, N.A. and Xu, X. and Veryaskin, A.V. (1996) Gravitational modelling of the test masses for STEP and LISA. Classical and Quantum Gravity, 13 (11A). A91-A95. ISSN 0264-9381

Full text not available in this repository. (Request a copy from the Strathclyde author)

Abstract

The test masses for the proposed STEP (satellite test of the equivalence principle) experiment can be influenced, adversely, by time-varying gravitational coupling to other masses within the spacecraft. The liquid helium in the spacecraft's Dewar is a severe potential source of this effect, since its influence is at the same frequency as any actual equivalence principal violation. The pairs of STEP test masses must be made differentially immune to this effect, and a measure of this immunity can be quantified in terms of a 'differential acceleration susceptibility', defined as .R; ; '/ D 1az=a. Here 1az and a are the differential-axial and commonmode accelerations, respectively, of the two masses, for a perturbing source at relative position .R; ; '/. This work presents the results of analyses for STEP's test masses having either four or six flats, included to prevent them from rolling in azimuth .'/. Different schemes for minimizing .R; ; '/ are discussed in detail, and it is shown that the gravitational effect of the flats may be balanced between the inner and outer masses, leading to a 'fully-balanced' pair. However, it is concluded that such a scheme is not practical, and the 'susceptibility' may be minimized, alternatively, by choosing six flats rather than four. It is noted that the gravitational theory used here may be applied to six- or four-sided bodies, including cubic test masses-as proposed for LISA.