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MICROSCOPE Mission: Final Results of the Test of the Equivalence Principle.
Touboul, Pierre; Métris, Gilles; Rodrigues, Manuel; Bergé, Joel; Robert, Alain; Baghi, Quentin; André, Yves; Bedouet, Judicaël; Boulanger, Damien; Bremer, Stefanie; Carle, Patrice; Chhun, Ratana; Christophe, Bruno; Cipolla, Valerio; Damour, Thibault; Danto, Pascale; Demange, Louis; Dittus, Hansjoerg; Dhuicque, Océane; Fayet, Pierre; Foulon, Bernard; Guidotti, Pierre-Yves; Hagedorn, Daniel; Hardy, Emilie; Huynh, Phuong-Anh; Kayser, Patrick; Lala, Stéphanie; Lämmerzahl, Claus; Lebat, Vincent; Liorzou, Françoise; List, Meike; Löffler, Frank; Panet, Isabelle; Pernot-Borràs, Martin; Perraud, Laurent; Pires, Sandrine; Pouilloux, Benjamin; Prieur, Pascal; Rebray, Alexandre; Reynaud, Serge; Rievers, Benny; Selig, Hanns; Serron, Laura; Sumner, Timothy; Tanguy, Nicolas; Torresi, Patrizia; Visser, Pieter.
Afiliación
  • Touboul P; ONERA, Université Paris Saclay, F-91123 Palaiseau, France.
  • Métris G; Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, IRD, Géoazur, 250 avenue Albert Einstein, F-06560 Valbonne, France.
  • Rodrigues M; DPHY, ONERA, Université Paris Saclay, F-92322 Châtillon, France.
  • Bergé J; DPHY, ONERA, Université Paris Saclay, F-92322 Châtillon, France.
  • Robert A; CNES Toulouse, 18 avenue Edouard Belin-31401 Toulouse Cedex 9, France.
  • Baghi Q; Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, IRD, Géoazur, 250 avenue Albert Einstein, F-06560 Valbonne, France.
  • André Y; DPHY, ONERA, Université Paris Saclay, F-92322 Châtillon, France.
  • Bedouet J; CNES Toulouse, 18 avenue Edouard Belin-31401 Toulouse Cedex 9, France.
  • Boulanger D; ONERA, Université de Toulouse, F-31055 Toulouse, France.
  • Bremer S; DPHY, ONERA, Université Paris Saclay, F-92322 Châtillon, France.
  • Carle P; ZARM, Center of Applied Space Technology and Microgravity, University of Bremen, Am Fallturm, D-28359 Bremen, Germany.
  • Chhun R; ONERA, Université Paris Saclay, F-91123 Palaiseau, France.
  • Christophe B; DPHY, ONERA, Université Paris Saclay, F-92322 Châtillon, France.
  • Cipolla V; DPHY, ONERA, Université Paris Saclay, F-92322 Châtillon, France.
  • Damour T; CNES Toulouse, 18 avenue Edouard Belin-31401 Toulouse Cedex 9, France.
  • Danto P; IHES, Institut des Hautes Etudes Scientifiques, 35 Route de Chartres, 91440 Bures-sur-Yvette, France.
  • Demange L; CNES Toulouse, 18 avenue Edouard Belin-31401 Toulouse Cedex 9, France.
  • Dittus H; Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, IRD, Géoazur, 250 avenue Albert Einstein, F-06560 Valbonne, France.
  • Dhuicque O; DLR, Köln headquarters, Linder Höhe, 51147 Köln, Germany.
  • Fayet P; DPHY, ONERA, Université Paris Saclay, F-92322 Châtillon, France.
  • Foulon B; Laboratoire de physique de l'Ecole normale supérieure, ENS, Université PSL, CNRS, Sorbonne Université, Université de Paris, F-75005 Paris, France, and CPhT, Ecole polytechnique, IPP, F-91128 Palaiseau, France.
  • Guidotti PY; DPHY, ONERA, Université Paris Saclay, F-92322 Châtillon, France.
  • Hagedorn D; CNES Toulouse, 18 avenue Edouard Belin-31401 Toulouse Cedex 9, France.
  • Hardy E; PTB, Physikalisch-Technische Bundesanstalt, Bundesallee 100, 38116 Braunschweig, Germany.
  • Huynh PA; DPHY, ONERA, Université Paris Saclay, F-92322 Châtillon, France.
  • Kayser P; DPHY, ONERA, Université Paris Saclay, F-92322 Châtillon, France.
  • Lala S; DPHY, ONERA, Université Paris Saclay, F-92322 Châtillon, France.
  • Lämmerzahl C; ONERA, Université Paris Saclay, F-91123 Palaiseau, France.
  • Lebat V; ZARM, Center of Applied Space Technology and Microgravity, University of Bremen, Am Fallturm, D-28359 Bremen, Germany.
  • Liorzou F; DPHY, ONERA, Université Paris Saclay, F-92322 Châtillon, France.
  • List M; DPHY, ONERA, Université Paris Saclay, F-92322 Châtillon, France.
  • Löffler F; ZARM, Center of Applied Space Technology and Microgravity, University of Bremen, Am Fallturm, D-28359 Bremen, Germany.
  • Panet I; PTB, Physikalisch-Technische Bundesanstalt, Bundesallee 100, 38116 Braunschweig, Germany.
  • Pernot-Borràs M; IPGP, 35 rue Hélène Brion, 75013 Paris, France.
  • Perraud L; DPHY, ONERA, Université Paris Saclay, F-92322 Châtillon, France.
  • Pires S; CNES Toulouse, 18 avenue Edouard Belin-31401 Toulouse Cedex 9, France.
  • Pouilloux B; Université Paris Saclay et Université de Paris, CEA, CNRS, AIM, F-91190 Gif-sur-Yvette, France.
  • Prieur P; CNES Toulouse, 18 avenue Edouard Belin-31401 Toulouse Cedex 9, France.
  • Rebray A; CNES Toulouse, 18 avenue Edouard Belin-31401 Toulouse Cedex 9, France.
  • Reynaud S; DPHY, ONERA, Université Paris Saclay, F-92322 Châtillon, France.
  • Rievers B; Laboratoire Kastler Brossel, Sorbonne Université, CNRS, ENS-PSL Université, Collège de France, 75252 Paris, France.
  • Selig H; ZARM, Center of Applied Space Technology and Microgravity, University of Bremen, Am Fallturm, D-28359 Bremen, Germany.
  • Serron L; ZARM, Center of Applied Space Technology and Microgravity, University of Bremen, Am Fallturm, D-28359 Bremen, Germany.
  • Sumner T; Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, IRD, Géoazur, 250 avenue Albert Einstein, F-06560 Valbonne, France.
  • Tanguy N; Blackett Laboratory, Imperial College London, Prince Consort Road, London SW7 2AZ, United Kingdom.
  • Torresi P; DPHY, ONERA, Université Paris Saclay, F-92322 Châtillon, France.
  • Visser P; CNES Toulouse, 18 avenue Edouard Belin-31401 Toulouse Cedex 9, France.
Phys Rev Lett ; 129(12): 121102, 2022 Sep 16.
Article en En | MEDLINE | ID: mdl-36179190
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.

Texto completo: 1 Colección: 01-internacional Base de datos: MEDLINE Idioma: En Revista: Phys Rev Lett Año: 2022 Tipo del documento: Article País de afiliación: Francia

Texto completo: 1 Colección: 01-internacional Base de datos: MEDLINE Idioma: En Revista: Phys Rev Lett Año: 2022 Tipo del documento: Article País de afiliación: Francia
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