MICROSCOPE Mission

Final Results of the Test of the Equivalence Principle

verfasst von
Pierre Touboul, Gilles Métris, Manuel Rodrigues, Joel Bergé, Alain Robert, Quentin Baghi, Yves André, Judicaël Bedouet, Damien Boulanger, Stefanie Bremer, Patrice Carle, Ratana Chhun, Bruno Christophe, Valerio Cipolla, Thibault Damour, Pascale Danto, Louis Demange, Hansjoerg Dittus, Océane Dhuicque, Pierre Fayet, Bernard Foulon, Pierre Yves Guidotti, Daniel Hagedorn, Emilie Hardy, Phuong Anh Huynh, Patrick Kayser, Stéphanie Lala, Claus Lämmerzahl, Vincent Lebat, Françoise Liorzou, Meike List, Frank Löffler, Isabelle Panet, Martin Pernot-Borràs, Laurent Perraud, Sandrine Pires, Benjamin Pouilloux, Pascal Prieur, Alexandre Rebray, Serge Reynaud, Benny Rievers, Hanns Selig, Laura Serron, Timothy Sumner, Nicolas Tanguy, Patrizia Torresi, Pieter Visser
Abstract

The MICROSCOPE mission was designed to test the weak equivalence principle (WEP), stating the equality between the inertial and the gravitational masses, with a precision of 10-15 in terms of the Eötvös ratio η. Its experimental test consisted of comparing the accelerations undergone by two collocated test masses of different compositions as they orbited the Earth, by measuring the electrostatic forces required to keep them in equilibrium. This was done with ultrasensitive differential electrostatic accelerometers onboard a drag-free satellite. The mission lasted two and a half years, cumulating five months worth of science free-fall data, two-thirds with a pair of test masses of different compositions - titanium and platinum alloys - and the last third with a reference pair of test masses of the same composition - platinum. We summarize the data analysis, with an emphasis on the characterization of the systematic uncertainties due to thermal instabilities and on the correction of short-lived events which could mimic a WEP violation signal. We found no violation of the WEP, with the Eötvös parameter of the titanium and platinum pair constrained to η(Ti,Pt)=[-1.5±2.3(stat)±1.5(syst)]×10-15 at 1σ in statistical errors.

Externe Organisation(en)
Universität Paris-Saclay
Observatoire de la Côte d’Azur (OCA)
Centre national d’études spatiales (CNES)
Université de Toulouse
Institut des Hautes Etudes Scientifiques
Deutsches Zentrum für Luft- und Raumfahrt e.V. (DLR)
Université Paris Sciences et Lettres
Centre national de la recherche scientifique (CNRS)
Physikalisch-Technische Bundesanstalt (PTB)
Institut de Physique du Globe de Paris (IPGP)
Universite Paris 6
Imperial College London
Delft University of Technology
Zentrum für angewandte Raumfahrt­technologie und Mikro­gravitation (ZARM)
Universität Bremen
Typ
Artikel
Journal
Physical review letters
Band
129
ISSN
0031-9007
Publikationsdatum
16.09.2022
Publikationsstatus
Veröffentlicht
Peer-reviewed
Ja
ASJC Scopus Sachgebiete
Physik und Astronomie (insg.)
Elektronische Version(en)
https://doi.org/10.1103/PhysRevLett.129.121102 (Zugang: Offen)