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Bassi A, Cacciapuoti L, Capozziello S, Dell'Agnello S, Diamanti E, Giulini D, Iess L, Jetzer P, Joshi SK, Landragin A, Poncin-Lafitte CL, Rasel E, Roura A, Salomon C, Ulbricht H. A way forward for fundamental physics in space. NPJ Microgravity 2022; 8:49. [PMID: 36336703 PMCID: PMC9637703 DOI: 10.1038/s41526-022-00229-0] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Key Words] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 04/26/2022] [Accepted: 10/03/2022] [Indexed: 11/08/2022] Open
Abstract
Space-based research can provide a major leap forward in the study of key open questions in the fundamental physics domain. They include the validity of Einstein's Equivalence principle, the origin and the nature of dark matter and dark energy, decoherence and collapse models in quantum mechanics, and the physics of quantum many-body systems. Cold-atom sensors and quantum technologies have drastically changed the approach to precision measurements. Atomic clocks and atom interferometers as well as classical and quantum links can be used to measure tiny variations of the space-time metric, elusive accelerations, and faint forces to test our knowledge of the physical laws ruling the Universe. In space, such instruments can benefit from unique conditions that allow improving both their precision and the signal to be measured. In this paper, we discuss the scientific priorities of a space-based research program in fundamental physics.
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Affiliation(s)
- A Bassi
- Department of Physics, University of Trieste, Strada Costiera 11, 34151, Trieste, Italy
- Istituto Nazionale di Fisica Nucleare, Trieste Section, Via Valerio 2, 34127, Trieste, Italy
| | - L Cacciapuoti
- European Space Agency, Keplerlaan 1 - P.O. Box 299, 2200 AG, Noordwijk, ZH, The Netherlands.
| | - S Capozziello
- Dipartimento di Fisica 'E. Pancini', Università di Napoli 'Federico II', INFN, Sezione di Napoli, via Cinthia 9, I-80126, Napoli, Italy
- Scuola Superiore Meridionale, Largo S. Marcellino 10, I-80138, Napoli, Italy
| | - S Dell'Agnello
- Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali di Frascati (INFN-LNF), via E. Fermi 54, 00044, Frascati (Rome), Italy
| | - E Diamanti
- LIP6, CNRS, Sorbonne Université, Paris, France
| | - D Giulini
- Institute for Theoretical Physics, Leibniz University Hannover, Appelstrasse 2, 30167, Hannover, Germany
| | - L Iess
- Sapienza Università di Roma, 00184, Rome, Italy
| | - P Jetzer
- Department of Physics, University of Zürich, Winterthurerstrasse 190, 8057, Zürich, Switzerland
| | - S K Joshi
- Quantum Engineering Technology Labs, H. H. Wills Physics Laboratory & Department of Electrical and Electronic Engineering, University of Bristol, Bristol, UK
| | - A Landragin
- SYRTE, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, LNE, Paris, France
| | - C Le Poncin-Lafitte
- SYRTE, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, LNE, Paris, France
| | - E Rasel
- Leibniz Universität Hannover, Institut für Quantenoptik, Welfengarten 1, 30167, Hannover, Germany
| | - A Roura
- Institute of Quantum Technologies, German Aerospace Center (DLR), Wilhelm-Runge-Straße 10, 89081, Ulm, Germany
| | - C Salomon
- Laboratoire Kastler Brossel, ENS-Université PSL, CNRS, Sorbonne Université, Collège de France, Paris, France
| | - H Ulbricht
- School of Physics and Astronomy, University of Southampton, SO17 1BJ, Southampton, United Kingdom
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Savalle E, Hees A, Frank F, Cantin E, Pottie PE, Roberts BM, Cros L, McAllister BT, Wolf P. Searching for Dark Matter with an Optical Cavity and an Unequal-Delay Interferometer. PHYSICAL REVIEW LETTERS 2021; 126:051301. [PMID: 33605767 DOI: 10.1103/physrevlett.126.051301] [Citation(s) in RCA: 2] [Impact Index Per Article: 0.7] [Reference Citation Analysis] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 06/11/2020] [Revised: 12/09/2020] [Accepted: 01/14/2021] [Indexed: 06/12/2023]
Abstract
We propose a new type of experiment that compares the frequency of a clock (an ultrastable optical cavity in this case) at time t to its own frequency some time t-T earlier, by "storing" the output signal (photons) in a fiber delay line. In ultralight oscillating dark matter (DM) models, such an experiment is sensitive to coupling of DM to the standard model fields, through oscillations of the cavity and fiber lengths and of the fiber refractive index. Additionally, the sensitivity is significantly enhanced around the mechanical resonances of the cavity. We present experimental results of such an experiment and report no evidence of DM for masses in the [4.1×10^{-11}, 8.3×10^{-10}] eV region. In addition, we improve constraints on the involved coupling constants by one order of magnitude in a standard galactic DM model, at the mass corresponding to the resonant frequency of our cavity. Furthermore, in the model of relaxion DM, we improve on existing constraints over the whole DM mass range by about one order of magnitude, and up to 6 orders of magnitude at resonance.
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Affiliation(s)
- Etienne Savalle
- SYRTE, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, LNE, 75014 Paris, France
| | - Aurélien Hees
- SYRTE, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, LNE, 75014 Paris, France
| | - Florian Frank
- SYRTE, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, LNE, 75014 Paris, France
| | - Etienne Cantin
- SYRTE, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, LNE, 75014 Paris, France
| | - Paul-Eric Pottie
- SYRTE, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, LNE, 75014 Paris, France
| | - Benjamin M Roberts
- School of Mathematics and Physics, The University of Queensland, Brisbane QLD 4072, Australia
| | - Lucie Cros
- SYRTE, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, LNE, 75014 Paris, France
- MINES ParisTech, Université PSL, 75006 Paris, France
| | - Ben T McAllister
- ARC Centre of Excellence for Engineered Quantum Systems, School of Physics, University of Western Australia, Crawley, Western Australia 6009, Australia
| | - Peter Wolf
- SYRTE, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, LNE, 75014 Paris, France
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