Your browser doesn't support javascript.
loading
Exploring gravity with the MIGA large scale atom interferometer.
Canuel, B; Bertoldi, A; Amand, L; Pozzo di Borgo, E; Chantrait, T; Danquigny, C; Dovale Álvarez, M; Fang, B; Freise, A; Geiger, R; Gillot, J; Henry, S; Hinderer, J; Holleville, D; Junca, J; Lefèvre, G; Merzougui, M; Mielec, N; Monfret, T; Pelisson, S; Prevedelli, M; Reynaud, S; Riou, I; Rogister, Y; Rosat, S; Cormier, E; Landragin, A; Chaibi, W; Gaffet, S; Bouyer, P.
Afiliação
  • Canuel B; MIGA Consortium, Talence, France. benjamin.canuel@institutoptique.fr.
  • Bertoldi A; LP2N, Laboratoire Photonique, Numérique et Nanosciences, Université Bordeaux-IOGS-CNRS:UMR 5298, rue F. Mitterrand, F-33400, Talence, France. benjamin.canuel@institutoptique.fr.
  • Amand L; MIGA Consortium, Talence, France.
  • Pozzo di Borgo E; LP2N, Laboratoire Photonique, Numérique et Nanosciences, Université Bordeaux-IOGS-CNRS:UMR 5298, rue F. Mitterrand, F-33400, Talence, France.
  • Chantrait T; MIGA Consortium, Talence, France.
  • Danquigny C; LNE-SYRTE, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, 61, avenue de l'Observatoire, F-75014, Paris, France.
  • Dovale Álvarez M; MIGA Consortium, Talence, France.
  • Fang B; UMR 1114 EMMAH, Université d'Avignon et des Pays de Vaucluse, INRA, BP 21239, F-84916, Avignon Cedex 9, France.
  • Freise A; MIGA Consortium, Talence, France.
  • Geiger R; LNE-SYRTE, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, 61, avenue de l'Observatoire, F-75014, Paris, France.
  • Gillot J; MIGA Consortium, Talence, France.
  • Henry S; UMR 1114 EMMAH, Université d'Avignon et des Pays de Vaucluse, INRA, BP 21239, F-84916, Avignon Cedex 9, France.
  • Hinderer J; School of Physics and Astronomy and Institute of Gravitational Wave Astronomy, University of Birmingham, Edgbaston, Birmingham, B15 2TT, UK.
  • Holleville D; MIGA Consortium, Talence, France.
  • Junca J; LNE-SYRTE, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, 61, avenue de l'Observatoire, F-75014, Paris, France.
  • Lefèvre G; School of Physics and Astronomy and Institute of Gravitational Wave Astronomy, University of Birmingham, Edgbaston, Birmingham, B15 2TT, UK.
  • Merzougui M; MIGA Consortium, Talence, France.
  • Mielec N; LNE-SYRTE, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, 61, avenue de l'Observatoire, F-75014, Paris, France.
  • Monfret T; MIGA Consortium, Talence, France.
  • Pelisson S; LP2N, Laboratoire Photonique, Numérique et Nanosciences, Université Bordeaux-IOGS-CNRS:UMR 5298, rue F. Mitterrand, F-33400, Talence, France.
  • Prevedelli M; Oxford University, Department of Physics, Denys Wilkinson Building, Keble Road, Oxford, OX1 3RH, UK.
  • Reynaud S; MIGA Consortium, Talence, France.
  • Riou I; Institut de Physique du Globe de Strasbourg, UMR 7516, Université de Strasbourg/EOST, CNRS, 5 rue Descartes, 67084, Strasbourg, France.
  • Rogister Y; MIGA Consortium, Talence, France.
  • Rosat S; LNE-SYRTE, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, 61, avenue de l'Observatoire, F-75014, Paris, France.
  • Cormier E; MIGA Consortium, Talence, France.
  • Landragin A; LP2N, Laboratoire Photonique, Numérique et Nanosciences, Université Bordeaux-IOGS-CNRS:UMR 5298, rue F. Mitterrand, F-33400, Talence, France.
  • Chaibi W; MIGA Consortium, Talence, France.
  • Gaffet S; LP2N, Laboratoire Photonique, Numérique et Nanosciences, Université Bordeaux-IOGS-CNRS:UMR 5298, rue F. Mitterrand, F-33400, Talence, France.
  • Bouyer P; MIGA Consortium, Talence, France.
Sci Rep ; 8(1): 14064, 2018 Sep 14.
Article em En | MEDLINE | ID: mdl-30218107
ABSTRACT
We present the MIGA experiment, an underground long baseline atom interferometer to study gravity at large scale. The hybrid atom-laser antenna will use several atom interferometers simultaneously interrogated by the resonant mode of an optical cavity. The instrument will be a demonstrator for gravitational wave detection in a frequency band (100 mHz-1 Hz) not explored by classical ground and space-based observatories, and interesting for potential astrophysical sources. In the initial instrument configuration, standard atom interferometry techniques will be adopted, which will bring to a peak strain sensitivity of [Formula see text] at 2 Hz. This demonstrator will enable to study the techniques to push further the sensitivity for the future development of gravitational wave detectors based on large scale atom interferometers. The experiment will be realized at the underground facility of the Laboratoire Souterrain à Bas Bruit (LSBB) in Rustrel-France, an exceptional site located away from major anthropogenic disturbances and showing very low background noise. In the following, we present the measurement principle of an in-cavity atom interferometer, derive the method for Gravitational Wave signal extraction from the antenna and determine the expected strain sensitivity. We then detail the functioning of the different systems of the antenna and describe the properties of the installation site.

Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Idioma: En Revista: Sci Rep Ano de publicação: 2018 Tipo de documento: Article País de afiliação: França

Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Idioma: En Revista: Sci Rep Ano de publicação: 2018 Tipo de documento: Article País de afiliação: França