A ring lasers array for fundamental physics

被引：51

作者：

Di Virgilio, Angela ^{[1
]}

Allegrini, Maria ^{[2
]}

Beghi, Alessandro ^{[3
]}

Belfi, Jacopo ^{[1
]}

Beverini, Nicolo ^{[2
]}

Bosi, Filippo ^{[1
]}

Bouhadef, Bachir ^{[1
]}

Calamai, Massimo ^{[2
]}

Carelli, Giorgio ^{[2
]}

Cuccato, Davide ^{[3
,4
]}

Maccioni, Enrico ^{[2
]}

Ortolan, Antonello ^{[4
]}

Passeggio, Giuseppe ^{[5
]}

Porzio, Alberto ^{[5
,6
]}

Ruggiero, Matteo Luca ^{[7
]}

Santagata, Rosa ^{[8
]}

Tartaglia, Angelo ^{[7
]}

机构：

[1] INFN Sez Pisa, Pisa, Italy

[2] Univ Pisa, Dept Phys, I-56100 Pisa, Italy

[3] Univ Padua, DEI, Padua, Italy

[4] INFN Legnaro Natl Lab, Padua, Italy

[5] INFN Sez Napoli, Naples, Italy

[6] CNR SPIN, Naples, Italy

[7] Politecn Torino, Turin, Italy

[8] Univ Siena, Dept Phys, I-53100 Siena, Italy

来源：

COMPTES RENDUS PHYSIQUE | 2014年 / 15卷 / 10期

关键词：

Sagnac effect; Ring-laser; Inertial sensor; Gravito-magnetism; Lense-Thirring effect; Length of the day; CONSTANT;

D O I：

10.1016/j.crhy.2014.10.005

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

After reviewing the importance of light as a probe for testing the structure of space-time, we describe the GINGER project. GINGER will be a three-dimensional array of large-size ring-lasers able to measure the de Sitter and Lense-Thirring effects. The instrument will be located at the underground laboratory of Gran Sasso, in Italy. We describe the preliminary actions and measurements already under way and present the full road map to GINGER. The intermediate apparatuses GP2 and GINGERino are described. GINGER is expected to be fully operating in few years. (C) 2014 Academie des sciences. Published by Elsevier Masson SAS. All rights reserved.

引用

页码：866 / 874

页数：9

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