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Where do we stand in testing general relativity?

Schäfer, G. | Elsevier | 2003

gravity. Completed towards the end of 1915, until now the theory has passed all tests, including the prediction of gravitational waves. The paper ...

VLBI for better gravimetry in SELENE

Hanada, H. / Iwata, T. / Namiki, N. et al. | Elsevier | 2007

improve the accuracy to which the low degree gravitational harmonics and the gravity field near the limb can be measured, and when combined with ...

Ultra-sensitive electrostatic planar acceleration gradiometer for airborne geophysical surveys

Douch, Karim / Christophe, Bruno / Foulon, Bernard et al. | Tema Archive | 2014

We propose a new concept of gravity gradiometer, GREMLIT, for the determination of the spatial derivatives of gravitational acceleration ...

Ultralow-temperature resonant gravitational wave detectors, present state and future prospects

Frossati, G. | Elsevier | 2003

AbstractResonant gravitational wave detectors have evolved from the room ...

The midlatitude ionosphere D-region response to some events on the sun

Gokov, Alexander M. / Tyrnov, Oleg F. | Elsevier | 2002

D-region. Such processes in this height range are accompanied by the generation and enhancement of acoustic-gravitational waves with periods ...

The Laser Interferometer Gravitational-wave Observatory (LIGO)

Spero, R. E. / Whitcomb, S. E. | British Library Online Contents | 1995

The gravitational wave signature of young and dense star clusters

Portegies Zwart, Simon F. | Elsevier | 2006

gravitational wave radiation in the LISA band. If the star captured by the intermediate mass black hole is relatively low mass (≲2M ...

Keywords: Gravitational waves

The final phase of inspiral of neutron stars: Realistic equations of state

Gondek-Rosińska, D. / Bejger, M. / Bulik, T. et al. | Elsevier | 2006

-shedding limit for neutron star binaries. The gravitational wave frequency at the ISCO, which marks the end of the inspiral phase, is found to be ...

Keywords: Gravitational waves

The double-pulsar binary J0737–3039

Lyne, A.G. | Elsevier | 2005

detection of such events by the new ground-based gravitational wave detectors. ...

The CHAMP-only earth gravity field model EIGEN-2

Reigber, Ch / Schwintzer, P / Neumayer, K.-H et al. | Elsevier | 2003

since July 2000 in a highly inclined orbit with an altitude of initially 450 km and meanwhile at about 400 km. From the gravitational orbit ...