Constraints on fifth forces and ultralight dark matter from OSIRIS-REx target asteroid Bennu

被引:0
|
作者
Tsai, Yu-Dai [1 ,2 ,3 ,4 ]
Farnocchia, Davide [5 ]
Micheli, Marco [6 ]
Vagnozzi, Sunny [7 ,8 ]
Visinelli, Luca [9 ,10 ]
机构
[1] Los Almos Natl Lab LANL, Los Alamos, NM 87545 USA
[2] Univ Calif Irvine, Dept Phys & Astron, Irvine, CA 92697 USA
[3] Fermi Natl Accelerator Lab Fermilab, Batavia, IL 60510 USA
[4] Univ Chicago, Kavli Inst Cosmol Phys KICP, Chicago, IL 60637 USA
[5] CALTECH, Jet Prop Lab JPL, Pasadena, CA USA
[6] European Space Agcy ESA, NEO Coordinat Ctr, Frascati, RM, Italy
[7] Univ Trento, Dept Phys, Povo, TN, Italy
[8] INFN, Trento Inst Fundamental Phys & Applicat TIFPA, Povo, TN, Italy
[9] Tsung Dao Lee Inst TDLI, Shanghai, Peoples R China
[10] Shanghai Jiao Tong Univ, Sch Phys & Astron, Shanghai, Peoples R China
来源
COMMUNICATIONS PHYSICS | 2024年 / 7卷 / 01期
基金
美国国家航空航天局; 美国国家科学基金会; 中国国家自然科学基金;
关键词
PHYSICS;
D O I
10.1038/s42005-024-01779-3
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
It is important to test the possible existence of fifth forces, as ultralight bosons that would mediate these are predicted to exist in several well-motivated extensions of the Standard Model. Recent work indicated asteroids as promising probes, but applications to real data are lacking so far. Here we use the OSIRIS-REx mission and ground-based tracking data for the asteroid Bennu to derive constraints on fifth forces. Our limits are strongest for mediator masses m similar to (10(-18)-10(-17)) eV, where we currently achieve the tightest bounds. These can be translated to a wide class of models leading to Yukawa-type fifth forces, and we demonstrate how they apply to U(1)(B) dark photons and baryon-coupled scalars. Our results demonstrate the potential of asteroid tracking in probing well-motivated extensions of the Standard Model and ultralight bosons near the fuzzy dark matter range.
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收藏
页数:7
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