Details
| Original language | English |
|---|---|
| Article number | 064010 |
| Number of pages | 19 |
| Journal | Physical Review D |
| Volume | 109 |
| Issue number | 6 |
| Publication status | Published - 5 Mar 2024 |
Abstract
The space-time explorer and quantum equivalence principle space test (STE-QUEST) recently proposed, aims at performing a precision test of the weak equivalence principle (WEP), a fundamental cornerstone of general relativity. Taking advantage of the ideal operation conditions for high-precision quantum sensing on board of a satellite, it aims to detect possible violations of WEP down to the 10-17 level. This level of performance leads to stringent environmental requirements on the control of the spacecraft. We assume an operation of a dual-species atom interferometer of rubidium and potassium isotopes in a double-diffraction configuration and derive the constraints to achieve an Eötvös parameter η=10-17 in statistical and systematic uncertainties. We show that technical heritage of previous satellite missions, such as MICROSCOPE, satisfies the platform requirements to achieve the proposed objectives underlying the technical readiness of the STE-QUEST mission proposal.
ASJC Scopus subject areas
- Physics and Astronomy(all)
- Nuclear and High Energy Physics
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In: Physical Review D, Vol. 109, No. 6, 064010, 05.03.2024.
Research output: Contribution to journal › Article › Research › peer review
}
TY - JOUR
T1 - Platform and environment requirements of a satellite quantum test of the weak equivalence principle at the 10-17 level
AU - Struckmann, Christian
AU - Corgier, Robin
AU - Loriani, Sina
AU - Kleinsteinberg, Gina
AU - Gox, Nina
AU - Giese, Enno
AU - Métris, Gilles
AU - Gaaloul, Naceur
AU - Wolf, Peter
N1 - Funding Information: The authors thank all contributors to STE-QUEST proposals (see Ref. for a full list). R. C. thanks the Paris Observatory Scientific Council and was funded by “PSL fellowship at Paris Observatory” program. This work was funded by the Deutsche Forschungsgemeinschaft (German Research Foundation) under Germany’s Excellence Strategy (EXC-2123 QuantumFrontiers Grant No. 390837967) and through Collaborative Research Centre (CRC) 1227 (DQ-mat) within Project No. A05, and the German Space Agency at the German Aerospace Center (Deutsche Raumfahrtagentur im Deutschen Zentrum für Luft- und Raumfahrt, DLR) with funds provided by the German Federal Ministry of Economic Affairs and Climate Action due to an enactment of the German Bundestag under Grants No. 50WM2250A and No. 50WM2250E (QUANTUS+), No. 50WP1700 (BECCAL), No. 50WM2245A (CAL-II), No. 50WM2263A (CARIOQA-GE), No. 50WM2253A (AI-Quadrat), No. 50RK1957 (QGYRO), No. 50WM2177 (INTENTAS), as well as No. 50NA2106 (QGYRO+).
PY - 2024/3/5
Y1 - 2024/3/5
N2 - The space-time explorer and quantum equivalence principle space test (STE-QUEST) recently proposed, aims at performing a precision test of the weak equivalence principle (WEP), a fundamental cornerstone of general relativity. Taking advantage of the ideal operation conditions for high-precision quantum sensing on board of a satellite, it aims to detect possible violations of WEP down to the 10-17 level. This level of performance leads to stringent environmental requirements on the control of the spacecraft. We assume an operation of a dual-species atom interferometer of rubidium and potassium isotopes in a double-diffraction configuration and derive the constraints to achieve an Eötvös parameter η=10-17 in statistical and systematic uncertainties. We show that technical heritage of previous satellite missions, such as MICROSCOPE, satisfies the platform requirements to achieve the proposed objectives underlying the technical readiness of the STE-QUEST mission proposal.
AB - The space-time explorer and quantum equivalence principle space test (STE-QUEST) recently proposed, aims at performing a precision test of the weak equivalence principle (WEP), a fundamental cornerstone of general relativity. Taking advantage of the ideal operation conditions for high-precision quantum sensing on board of a satellite, it aims to detect possible violations of WEP down to the 10-17 level. This level of performance leads to stringent environmental requirements on the control of the spacecraft. We assume an operation of a dual-species atom interferometer of rubidium and potassium isotopes in a double-diffraction configuration and derive the constraints to achieve an Eötvös parameter η=10-17 in statistical and systematic uncertainties. We show that technical heritage of previous satellite missions, such as MICROSCOPE, satisfies the platform requirements to achieve the proposed objectives underlying the technical readiness of the STE-QUEST mission proposal.
UR - http://www.scopus.com/inward/record.url?scp=85186887204&partnerID=8YFLogxK
U2 - 10.1103/PhysRevD.109.064010
DO - 10.1103/PhysRevD.109.064010
M3 - Article
AN - SCOPUS:85186887204
VL - 109
JO - Physical Review D
JF - Physical Review D
SN - 2470-0010
IS - 6
M1 - 064010
ER -