Bruno Christophe

Mr. Bruno Christophe

orcid

Research Focus & Metrics

Academic Career Length

32Years (1995-Present)

(Calculated once Scilit publication data is synced: current year − year of first publication + 1)

Representative Publications

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4 December 2017 in Physical Review Letters
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Journal Article
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PTPierre Touboul
Pierre Touboul
GMGilles Métris
Gilles Métris
MRManuel Rodrigues
Manuel Rodrigues
YAYves André
Yves André
QBQuentin Baghi
Quentin Baghi
PVPieter Visser
Pieter Visser
According to the weak equivalence principle, all bodies should fall at the same rate in a gravitational field. The MICROSCOPE satellite, launched in April 2016, aims to test its validity at the 10−15 precision level, by measuring the force required to maintain two test masses (of titanium and platinum alloys) exactly in the same orbit. A nonvanishing result would correspond to a violation of the equivalence principle, or to the discovery of a new long-range force. Analysis of the first data gives δ(Ti,Pt)=[−1±9(stat)±9(syst)]×10−15 (1σ statistical uncertainty) for the titanium-platinum Eötvös parameter characterizing the relative difference in their free-fall accelerations.

24 March 2016 in EPJ Quantum Technology
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Journal Article
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RKRainer Kaltenbaek
Rainer Kaltenbaek
MAMarkus Aspelmeyer
Markus Aspelmeyer
PBPeter F Barker
Peter F Barker
ABAngelo Bassi
Angelo Bassi
JBJames Bateman
James Bateman
VVVlatko Vedral
Vlatko Vedral
Do the laws of quantum physics still hold for macroscopic objects - this is at the heart of Schrödinger’s cat paradox - or do gravitation or yet unknown effects set a limit for massive particles? What is the fundamental relation between quantum physics and gravity? Ground-based experiments addressing these questions may soon face limitations due to limited free-fall times and the quality of vacuum and microgravity. The proposed mission Macroscopic Quantum Resonators (MAQRO) may overcome these limitations and allow addressing such fundamental questions. MAQRO harnesses recent developments in quantum optomechanics, high-mass matter-wave interferometry as well as state-of-the-art space technology to push macroscopic quantum experiments towards their ultimate performance limits and to open new horizons for applying quantum technology in space. The main scientific goal is to probe the vastly unexplored ‘quantum-classical’ transition for increasingly massive objects, testing the predictions of quantum theory for objects in a size and mass regime unachievable in ground-based experiments. The hardware will largely be based on available space technology. Here, we present the MAQRO proposal submitted in response to the 4th Cosmic Vision call for a medium-sized mission (M4) in 2014 of the European Space Agency (ESA) with a possible launch in 2025, and we review the progress with respect to the original MAQRO proposal for the 3rd Cosmic Vision call for a medium-sized mission (M3) in 2010. In particular, the updated proposal overcomes several critical issues of the original proposal by relying on established experimental techniques from high-mass matter-wave interferometry and by introducing novel ideas for particle loading and manipulation. Moreover, the mission design was improved to better fulfill the stringent environmental requirements for macroscopic quantum experiments.

4 September 2008 in Experimental Astronomy
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Journal Article
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PWP. Wolf
P. Wolf
CBCh. J. Bordé
Ch. J. Bordé
ACA. Clairon
A. Clairon
LDL. Duchayne
L. Duchayne
ALA. Landragin
A. Landragin
KSK. Sengstock
K. Sengstock

1 December 2015 in Acta Astronautica
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Journal Article
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BCBruno Christophe
Bruno Christophe
DBD. Boulanger
D. Boulanger
BFB. Foulon
B. Foulon
PHP.-A. Huynh
P.-A. Huynh
VLV. Lebat
V. Lebat
EPE. Perrot
E. Perrot

1 August 2019 in Advances In Space Research
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Journal Article
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TBTamara Bandikova
Tamara Bandikova
CMChristopher McCullough
Christopher McCullough
GKGerhard L. Kruizinga
Gerhard L. Kruizinga
HSHimanshu Save
Himanshu Save
BCBruno Christophe
Bruno Christophe

27 March 2008 in Experimental Astronomy
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Journal Article
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BCBruno Christophe
Bruno Christophe
PAP. H. Andersen
P. H. Andersen
JAJ. D. Anderson
J. D. Anderson
SAS. Asmar
S. Asmar
PBPh. Bério
Ph. Bério
NYN. Yu
N. Yu
The Solar System Odyssey mission uses modern-day high-precision experimental techniques to test the laws of fundamental physics which determine dynamics in the solar system. It could lead to major discoveries by using demonstrated technologies and could be flown within the Cosmic Vision time frame. The mission proposes to perform a set of precision gravitation experiments from the vicinity of Earth to the outer Solar System. Its scientific objectives can be summarized as follows: (1) test of the gravity force law in the Solar System up to and beyond the orbit of Saturn; (2) precise investigation of navigation anomalies at the fly-bys; (3) measurement of Eddington’s parameter at occultations; (4) mapping of gravity field in the outer solar system and study of the Kuiper belt. To this aim, the Odyssey mission is built up on a main spacecraft, designed to fly up to 13 AU, with the following components: (a) a high-precision accelerometer, with bias-rejection system, measuring the deviation of the trajectory from the geodesics, that is also giving gravitational forces; (b) Ka-band transponders, as for Cassini, for a precise range and Doppler measurement up to 13 AU, with additional VLBI equipment; (c) optional laser equipment, which would allow one to improve the range and Doppler measurement, resulting in particular in an improved measurement (with respect to Cassini) of the Eddington’s parameter. In this baseline concept, the main spacecraft is designed to operate beyond the Saturn orbit, up to 13 AU. It experiences multiple planetary fly-bys at Earth, Mars or Venus, and Jupiter. The cruise and fly-by phases allow the mission to achieve its baseline scientific objectives [(1) to (3) in the above list]. In addition to this baseline concept, the Odyssey mission proposes the release of the Enigma radio-beacon at Saturn, allowing one to extend the deep space gravity test up to at least 50 AU, while achieving the scientific objective of a mapping of gravity field in the outer Solar System [(4) in the above list].