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Beyond the Required LISA Free-Fall Performance: New LISA Pathfinder Results down to 20 µHz.
Armano, M; Audley, H; Baird, J; Binetruy, P; Born, M; Bortoluzzi, D; Castelli, E; Cavalleri, A; Cesarini, A; Cruise, A M; Danzmann, K; de Deus Silva, M; Diepholz, I; Dixon, G; Dolesi, R; Ferraioli, L; Ferroni, V; Fitzsimons, E D; Freschi, M; Gesa, L; Gibert, F; Giardini, D; Giusteri, R; Grimani, C; Grzymisch, J; Harrison, I; Heinzel, G; Hewitson, M; Hollington, D; Hoyland, D; Hueller, M; Inchauspé, H; Jennrich, O; Jetzer, P; Karnesis, N; Kaune, B; Korsakova, N; Killow, C J; Lobo, J A; Lloro, I; Liu, L; López-Zaragoza, J P; Maarschalkerweerd, R; Mance, D; Meshksar, N; Martín, V; Martin-Polo, L; Martino, J; Martin-Porqueras, F; Mateos, I.
Affiliation
  • Armano M; European Space Astronomy Centre, European Space Agency, Villanueva de la Cañada, 28692 Madrid, Spain.
  • Audley H; Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany.
  • Baird J; High Energy Physics Group, Physics Department, Imperial College London, Blackett Laboratory, Prince Consort Road, London, SW7 2BW, United Kingdom.
  • Binetruy P; APC, Université Paris Diderot, CNRS/IN2P3, CEA/lrfu, Observatoire de Paris, Sorbonne Paris Cité, France.
  • Born M; Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany.
  • Bortoluzzi D; Department of Industrial Engineering, University of Trento, via Sommarive 9, 38123 Trento, and Trento Institute for Fundamental Physics and Application/INFN, Italy.
  • Castelli E; Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Application/INFN, 38123 Povo, Trento, Italy.
  • Cavalleri A; Istituto di Fotonica e Nanotecnologie, CNR-Fondazione Bruno Kessler, I-38123 Povo, Trento, Italy.
  • Cesarini A; DISPEA, Università di Urbino "Carlo Bo," Via S. Chiara, 27 61029 Urbino/INFN, Italy.
  • Cruise AM; The School of Physics and Astronomy, University of Birmingham, Birmingham, United Kingdom.
  • Danzmann K; Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany.
  • de Deus Silva M; European Space Astronomy Centre, European Space Agency, Villanueva de la Cañada, 28692 Madrid, Spain.
  • Diepholz I; Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany.
  • Dixon G; The School of Physics and Astronomy, University of Birmingham, Birmingham, United Kingdom.
  • Dolesi R; Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Application/INFN, 38123 Povo, Trento, Italy.
  • Ferraioli L; Institut für Geophysik, ETH Zürich, Sonneggstrasse 5, CH-8092, Zürich, Switzerland.
  • Ferroni V; Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Application/INFN, 38123 Povo, Trento, Italy.
  • Fitzsimons ED; The UK Astronomy Technology Centre, Royal Observatory, Edinburgh, Blackford Hill, Edinburgh, EH9 3HJ, United Kingdom.
  • Freschi M; European Space Astronomy Centre, European Space Agency, Villanueva de la Cañada, 28692 Madrid, Spain.
  • Gesa L; Institut de Ciències de l'Espai (ICE, CSIC), Campus UAB, Carrer de Can Magrans s/n, 08193 Cerdanyola del Vallès, and Institut d'Estudis Espacials de Catalunya (IEEC), Gran Capità, 2-4, 08034 Barcelona, Spain.
  • Gibert F; Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Application/INFN, 38123 Povo, Trento, Italy.
  • Giardini D; Institut für Geophysik, ETH Zürich, Sonneggstrasse 5, CH-8092, Zürich, Switzerland.
  • Giusteri R; Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Application/INFN, 38123 Povo, Trento, Italy.
  • Grimani C; DISPEA, Università di Urbino "Carlo Bo," Via S. Chiara, 27 61029 Urbino/INFN, Italy.
  • Grzymisch J; European Space Technology Centre, European Space Agency, Keplerlaan 1, 2200 AG Noordwijk, Netherlands.
  • Harrison I; European Space Operations Centre, European Space Agency, 64293 Darmstadt, Germany.
  • Heinzel G; Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany.
  • Hewitson M; Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany.
  • Hollington D; High Energy Physics Group, Physics Department, Imperial College London, Blackett Laboratory, Prince Consort Road, London, SW7 2BW, United Kingdom.
  • Hoyland D; The School of Physics and Astronomy, University of Birmingham, Birmingham, United Kingdom.
  • Hueller M; Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Application/INFN, 38123 Povo, Trento, Italy.
  • Inchauspé H; APC, Université Paris Diderot, CNRS/IN2P3, CEA/lrfu, Observatoire de Paris, Sorbonne Paris Cité, France.
  • Jennrich O; European Space Technology Centre, European Space Agency, Keplerlaan 1, 2200 AG Noordwijk, Netherlands.
  • Jetzer P; Physik Institut, Universität Zürich, Winterthurerstrasse 190, CH-8057 Zürich, Switzerland.
  • Karnesis N; Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany.
  • Kaune B; Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik und Leibniz Universität Hannover, Callinstraße 38, 30167 Hannover, Germany.
  • Korsakova N; SUPA, Institute for Gravitational Research, School of Physics and Astronomy, University of Glasgow, Glasgow, G12 8QQ, United Kingdom.
  • Killow CJ; SUPA, Institute for Gravitational Research, School of Physics and Astronomy, University of Glasgow, Glasgow, G12 8QQ, United Kingdom.
  • Lobo JA; Institut de Ciències de l'Espai (ICE, CSIC), Campus UAB, Carrer de Can Magrans s/n, 08193 Cerdanyola del Vallès, and Institut d'Estudis Espacials de Catalunya (IEEC), Gran Capità, 2-4, 08034 Barcelona, Spain.
  • Lloro I; Institut de Ciències de l'Espai (ICE, CSIC), Campus UAB, Carrer de Can Magrans s/n, 08193 Cerdanyola del Vallès, and Institut d'Estudis Espacials de Catalunya (IEEC), Gran Capità, 2-4, 08034 Barcelona, Spain.
  • Liu L; Dipartimento di Fisica, Università di Trento and Trento Institute for Fundamental Physics and Application/INFN, 38123 Povo, Trento, Italy.
  • López-Zaragoza JP; Institut de Ciències de l'Espai (ICE, CSIC), Campus UAB, Carrer de Can Magrans s/n, 08193 Cerdanyola del Vallès, and Institut d'Estudis Espacials de Catalunya (IEEC), Gran Capità, 2-4, 08034 Barcelona, Spain.
  • Maarschalkerweerd R; European Space Operations Centre, European Space Agency, 64293 Darmstadt, Germany.
  • Mance D; Institut für Geophysik, ETH Zürich, Sonneggstrasse 5, CH-8092, Zürich, Switzerland.
  • Meshksar N; Institut für Geophysik, ETH Zürich, Sonneggstrasse 5, CH-8092, Zürich, Switzerland.
  • Martín V; Institut de Ciències de l'Espai (ICE, CSIC), Campus UAB, Carrer de Can Magrans s/n, 08193 Cerdanyola del Vallès, and Institut d'Estudis Espacials de Catalunya (IEEC), Gran Capità, 2-4, 08034 Barcelona, Spain.
  • Martin-Polo L; European Space Astronomy Centre, European Space Agency, Villanueva de la Cañada, 28692 Madrid, Spain.
  • Martino J; APC, Université Paris Diderot, CNRS/IN2P3, CEA/lrfu, Observatoire de Paris, Sorbonne Paris Cité, France.
  • Martin-Porqueras F; European Space Astronomy Centre, European Space Agency, Villanueva de la Cañada, 28692 Madrid, Spain.
  • Mateos I; Institut de Ciències de l'Espai (ICE, CSIC), Campus UAB, Carrer de Can Magrans s/n, 08193 Cerdanyola del Vallès, and Institut d'Estudis Espacials de Catalunya (IEEC), Gran Capità, 2-4, 08034 Barcelona, Spain.
Phys Rev Lett ; 120(6): 061101, 2018 Feb 09.
Article in En | MEDLINE | ID: mdl-29481269
ABSTRACT
In the months since the publication of the first results, the noise performance of LISA Pathfinder has improved because of reduced Brownian noise due to the continued decrease in pressure around the test masses, from a better correction of noninertial effects, and from a better calibration of the electrostatic force actuation. In addition, the availability of numerous long noise measurement runs, during which no perturbation is purposely applied to the test masses, has allowed the measurement of noise with good statistics down to 20 µHz. The Letter presents the measured differential acceleration noise figure, which is at (1.74±0.05) fm s^{-2}/sqrt[Hz] above 2 mHz and (6±1)×10 fm s^{-2}/sqrt[Hz] at 20 µHz, and discusses the physical sources for the measured noise. This performance provides an experimental benchmark demonstrating the ability to realize the low-frequency science potential of the LISA mission, recently selected by the European Space Agency.

Full text: 1 Collection: 01-internacional Database: MEDLINE Language: En Journal: Phys Rev Lett Year: 2018 Document type: Article Affiliation country: Spain

Full text: 1 Collection: 01-internacional Database: MEDLINE Language: En Journal: Phys Rev Lett Year: 2018 Document type: Article Affiliation country: Spain
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