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Featured researches published by F. Ricci.


Classical and Quantum Gravity | 1997

The Virgo interferometer

B. Caron; A. Dominjon; C. Drezen; R. Flaminio; X. Grave; F. Marion; L. Massonnet; C. Mehmel; R. Morand; B. Mours; V. Sannibale; M. Yvert; D. Babusci; S. Bellucci; S. Candusso; G. Giordano; G. Matone; J.-M. Mackowski; L. Pinard; F. Barone; E. Calloni; L. Di Fiore; M. Flagiello; F. Garufi; A. Grado; Maurizio Longo; M. Lops; S. Marano; L. Milano; S. Solimeno

The Virgo gravitational wave detector is an interferometer with 3 km long arms in construction near Pisa to be commissioned in the year 2000. Virgo has been designed to achieve a strain sensitivity of a few times at 200 Hz. A large effort has gone into the conception of the mirror suspension system, which is expected to reduce noise to the level of at 10 Hz. The expected signals and main sources of noise are briefly discussed; the choices made are illustrated together with the present status of the experiment.


Measurement Science and Technology | 2000

The maraging-steel blades of the Virgo super attenuator

S. Braccini; C Casciano; F. Cordero; F. Corvace; M. De Sanctis; R. Franco; F. Frasconi; E. Majorana; G. Paparo; R. Passaquieti; P. Rapagnani; F. Ricci; D. Righetti; A. Solina; Renzo Valentini

The blades are crucial components of the Virgo super attenuators. The material used for their construction is maraging steel, a low-carbon-content alloy with high ultimate tensile strength and low creep under stress. Youngs modulus, the shear modulus, the Poisson ratio and the corresponding elastic energy-loss coefficients have been measured. The measurements have been performed on specimens subjected to the same thermal treatments as those of elements for the Virgo interferometer realized with maraging steel. In addition, anelastic properties of the material subjected to different thermal treatments have been measured. It has been found that, for a maraging-steel structure (one free of plastic deformation), which undergoes an excitation with flexural vibrations, the elastic energy-loss coefficient can vary over a wide range as a function of the thermal treatment of the material and it is dominated by the thermo-elastic effect. The main reason for such a great alteration is supposed to be the dependence of the thermal conductivity on the average sizes of the precipitate particles and their relative separations.


Measurement Science and Technology | 1992

Test facility for resonance transducers of cryogenic gravitational wave antennas

E. Majorana; P. Rapagnani; F. Ricci

In order to reach the maximum sensitivity of the new ultra-low temperature gravitational wave antennas, a further improvement in transducer technology is necessary. The authors present the test system developed for the laboratory study of the resonant capacitive transducer and discuss some of the experimental results obtained at low and room temperatures.


arXiv: General Relativity and Quantum Cosmology | 2001

Gravitational Waves, Sources and Detectors

Bernard F. Schutz; F. Ricci


CASPUR Annual Report | 2009

Un sistema RFID in banda UHF per l'autoprestito in Biblioteca

F. Ricci; Andrea Crisanti


Archive | 2001

Astrophysics of gravitational-wave sources

Bernard F. Schutz; F. Ricci


SCIRES-IT : SCIentific RESearch and Information Technology | 2011

xFID: un sistema innovativo per l’autoprestito e la ricognizione inventariale in biblioteca

Ugo Contino; F. Ricci


CASPUR Annual Report | 2010

XFID: un sistema di autoprestito per le biblioteche

F. Ricci


Physical Review Letters | 2003

Gravitational lensing and gravitomagnetic time delay

Ignazio Ciufolini; F. Ricci


Archive | 2001

Elements of gravitational waves

Bernard F. Schutz; F. Ricci

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E. Majorana

Istituto Nazionale di Fisica Nucleare

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P. Rapagnani

Sapienza University of Rome

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Andrea Crisanti

Sapienza University of Rome

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E. Calloni

Istituto Nazionale di Fisica Nucleare

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F. Barone

University of Salerno

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F. Garufi

Istituto Nazionale di Fisica Nucleare

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