Hauptseite > Publikationsdatenbank > Properties of Cosmic Deuterons Measured by the Alpha Magnetic Spectrometer > print

001     1037650
005     20250203124510.0
024 7 _ |a 10.1103/PhysRevLett.132.261001
|2 doi
024 7 _ |a 0031-9007
|2 ISSN
024 7 _ |a 1092-0145
|2 ISSN
024 7 _ |a 1079-7114
|2 ISSN
024 7 _ |a 10.34734/FZJ-2025-00815
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024 7 _ |a 38996294
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024 7 _ |a WOS:001290702900001
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037 _ _ |a FZJ-2025-00815
082 _ _ |a 530
100 1 _ |a Aguilar, M.
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245 _ _ |a Properties of Cosmic Deuterons Measured by the Alpha Magnetic Spectrometer
260 _ _ |a College Park, Md.
|c 2024
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336 7 _ |a article
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336 7 _ |a Output Types/Journal article
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336 7 _ |a Journal Article
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336 7 _ |a ARTICLE
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336 7 _ |a JOURNAL_ARTICLE
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336 7 _ |a Journal Article
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520 _ _ |a Precision measurements by the Alpha Magnetic Spectrometer (AMS) on the International Space Station of the deuteron (𝐷) flux are presented. The measurements are based on 21×106 𝐷 nuclei in the rigidity range from 1.9 to 21 GV collected from May 2011 to April 2021. We observe that over the entire rigidity range the 𝐷 flux exhibits nearly identical time variations with the 𝑝, 3He, and 4He fluxes. Above 4.5 GV, the 𝐷/4He flux ratio is time independent and its rigidity dependence is well described by a single power law ∝𝑅Δ with Δ𝐷/4He=−0.108±0.005. This is in contrast with the 3He/4He flux ratio for which we find Δ3He/4He=−0.289±0.003. Above ∼13  GV we find a nearly identical rigidity dependence of the 𝐷 and 𝑝 fluxes with a 𝐷/𝑝 flux ratio of 0.027 ±0.001. These unexpected observations indicate that cosmic deuterons have a sizable primarylike component. With a method independent of cosmic ray propagation, we obtain the primary component of the 𝐷 flux equal to 9.4 ±0.5% of the 4He flux and the secondary component of the 𝐷 flux equal to 58 ±5% of the 3He flux.
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