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19982009
most citedFirst joint Gravitational Waves search by the Auriga-Explorer-Nautilus-Virgo collaboration

16 citations · 16 across the 2 of their papers we have counts for

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gr-qc20112 cited

Fourth order indirect integration method for black hole perturbations: even modes

Patxi Ritter, Alessandro D. A. M. Spallicci, Sofiane Aoudia +1

On the basis of a recently proposed strategy of finite element integration in time domain for partial differential equations with a singular source term, we present a fourth order…

gr-qc2009

Self-force and motion of stars around black holes

A. Spallicci, S. Aoudia

Through detection by low gravitational wave space interferometers, the capture of stars by supermassive black holes will constitute a giant step forward in the understanding of gra…

gr-qc200716 cited

First joint Gravitational Waves search by the Auriga-Explorer-Nautilus-Virgo collaboration

Virgo collaboration

We present results of the search for coincident burst excitations over a 24 hours long data set collected by AURIGA, EXPLORER, NAUTILUS and Virgo detectors during September 2005. T…

gr-qc2005

Expected Coalescence Rate of Double Neutron Stars for Ground Based Interferometers

T. Regimbau, J. A. de Freitas Pacheco, A. Spallicci +1

In this paper we present new estimates of the coalescence rate of neutron star binaries in the local universe and we discuss its consequences for the first generations of ground ba…

gr-qc2004

Brans-Dicke gravity and the capture of stars by black holes: some asymptotic results

Bertrand Chauvineau, Alessandro D. A. M. Spallicci, Jean-Daniel Fournier

In the context of star capture by a black hole, a new noticeable difference between Brans-Dicke theory and general relativity gravitational radiation is pointed out. This feature s…

gr-qc2004

Advanced VIRGO: detector optimization for gravitational waves by inspiralling binaries

Alessandro D. A. M. Spallicci, Sofiane Aoudia, Jose De Freitas Pacheco +2

For future configurations, we study the relation between the abatement of the noise sources and the Signal to Noise Ratio (SNR) for coalescing binaries. Our aim is not the proposit…