Novel constraints on fifth forces and ultralight dark sector with asteroidal data
Abstract
Here, we study for the first time the possibility of probing long-range fifth forces utilizing asteroid astrometric data, via the fifth force-induced orbital precession. We examine nine Near-Earth Object (NEO) asteroids whose orbital trajectories are accurately determined via optical and radar astrometry. Focusing on a Yukawa-type potential mediated by a new gauge field (dark photon) or a baryon-coupled scalar, we estimate the sensitivity reach for the fifth force coupling strength and mediator mass in the mass range m ≃ (10-21-10-15) eV, near the "fuzzy" dark matter region. Our estimated sensitivity is comparable to leading limits from equivalence principle tests, potentially exceeding these in a specific mass range. The fifth force-induced precession increases with the orbital semi-major axis in the small m limit, motivating the study of objects further away from the Sun. We also demonstrate that precession tests are particularly strong in probing long-range forces which approximately conserve the equivalence principle. We discuss future prospects for extending our study to more than a million asteroids, including NEOs, main-belt asteroids, Hildas, and Jupiter Trojans, as well as trans-Neptunian objects and exoplanets.
- Authors:
-
- Univ. of California, Irvine, CA (United States); Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States); Univ. of Chicago, IL (United States). Kavli Inst. for Cosmological Physics (KICP)
- Univ. of Michigan, Ann Arbor, MI (United States)
- Univ. of Trento (Italy); Istituto Nazionale di Fisica Nucleare, Trento (Italy). Trento Institute for Fundamental Physics and Applications (INFN-TIFPA); Univ. of Cambridge (United Kingdom). Kavli Institute for Cosmology Cambridge
- Tsung-Dao Lee Institute, Shanghai (China); Shanghai Jiao Tong Univ. (China)
- Publication Date:
- Research Org.:
- Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States); Univ. of Michigan, Ann Arbor, MI (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC), High Energy Physics (HEP)
- OSTI Identifier:
- 1824313
- Report Number(s):
- FERMILAB-PUB-21-298-AE-T; LCTP-21-17; arXiv:2107.04038
Journal ID: ISSN 1475-7516; oai:inspirehep.net:1880918
- Grant/Contract Number:
- AC02-07CH11359; SC007859
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Journal of Cosmology and Astroparticle Physics
- Additional Journal Information:
- Journal Volume: 2023; Journal Issue: 04; Journal ID: ISSN 1475-7516
- Publisher:
- Institute of Physics (IOP)
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; 72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS
Citation Formats
Tsai, Yu-Dai, Wu, Youjia, Vagnozzi, Sunny, and Visinelli, Luca. Novel constraints on fifth forces and ultralight dark sector with asteroidal data. United States: N. p., 2023.
Web. doi:10.1088/1475-7516/2023/04/031.
Tsai, Yu-Dai, Wu, Youjia, Vagnozzi, Sunny, & Visinelli, Luca. Novel constraints on fifth forces and ultralight dark sector with asteroidal data. United States. https://doi.org/10.1088/1475-7516/2023/04/031
Tsai, Yu-Dai, Wu, Youjia, Vagnozzi, Sunny, and Visinelli, Luca. Wed .
"Novel constraints on fifth forces and ultralight dark sector with asteroidal data". United States. https://doi.org/10.1088/1475-7516/2023/04/031. https://www.osti.gov/servlets/purl/1824313.
@article{osti_1824313,
title = {Novel constraints on fifth forces and ultralight dark sector with asteroidal data},
author = {Tsai, Yu-Dai and Wu, Youjia and Vagnozzi, Sunny and Visinelli, Luca},
abstractNote = {Here, we study for the first time the possibility of probing long-range fifth forces utilizing asteroid astrometric data, via the fifth force-induced orbital precession. We examine nine Near-Earth Object (NEO) asteroids whose orbital trajectories are accurately determined via optical and radar astrometry. Focusing on a Yukawa-type potential mediated by a new gauge field (dark photon) or a baryon-coupled scalar, we estimate the sensitivity reach for the fifth force coupling strength and mediator mass in the mass range m ≃ (10-21-10-15) eV, near the "fuzzy" dark matter region. Our estimated sensitivity is comparable to leading limits from equivalence principle tests, potentially exceeding these in a specific mass range. The fifth force-induced precession increases with the orbital semi-major axis in the small m limit, motivating the study of objects further away from the Sun. We also demonstrate that precession tests are particularly strong in probing long-range forces which approximately conserve the equivalence principle. We discuss future prospects for extending our study to more than a million asteroids, including NEOs, main-belt asteroids, Hildas, and Jupiter Trojans, as well as trans-Neptunian objects and exoplanets.},
doi = {10.1088/1475-7516/2023/04/031},
journal = {Journal of Cosmology and Astroparticle Physics},
number = 04,
volume = 2023,
place = {United States},
year = {Wed Apr 12 00:00:00 EDT 2023},
month = {Wed Apr 12 00:00:00 EDT 2023}
}
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