Detecting cosmological scalar fields using orbital networks of quantum sensors
In this paper, we propose a method to detect the interaction of a hypothetical coherently evolving cosmological scalar field with an orbital network of quantum sensors, focusing on the Global Positioning System (GPS) satellite network as a test example. Cosmological scenarios, such as a scalar-tensor theory for dark energy or the axi-Higgs model, suggest that such a field may exist. As this field would be (approximately) at rest in the cosmic microwave background (CMB) frame, it would exhibit a dipole as a result of the movement of our terrestrial observers relative to the CMB. While the current sensitivity of the GPS network is insufficient to detect a cosmological dipole, future networks of quantum sensors on heliocentric orbits, using state-of-the-art atomic clocks, can reach and exceed this requirement.
Authors
- Conner Dailey (ORCID: https://orcid.org/0000-0003-2488-3461)
- Ruolin Liu (ORCID: https://orcid.org/0009-0003-7385-3071)
- Niayesh Afshordi (ORCID: https://orcid.org/0000-0002-9940-7040)
- Yu Li (ORCID: https://orcid.org/0009-0009-1565-6356)
Institutions
- University of Waterloo (CA)
- Perimeter Institute (CA)
Publication Details
- Journal
- Physical review. D/Physical review. D.
- Published
- 2024-08-21
- DOI
- https://doi.org/10.1103/physrevd.110.043028
- Citations
- 1
- Primary Topic
- Cosmology and Gravitation Theories
- Type
- article
- Field-Weighted Citation Impact
- 0.33
Funders
- Innovation, Science and Economic Development Canada
- Government of Canada
- Canada First Research Excellence Fund
- Institut Périmètre de physique théorique
- Ministry of Colleges and Universities
- Natural Sciences and Engineering Research Council of Canada