Academic literature on the topic 'Galactic deuteron'

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Journal articles on the topic "Galactic deuteron"

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Koldobskiy, S. A., O. Adriani, G. C. Barbarino, et al. "Galactic deuteron spectrum measured in PAMELA experiment." Journal of Physics: Conference Series 409 (February 1, 2013): 012040. http://dx.doi.org/10.1088/1742-6596/409/1/012040.

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Koldobskiy, S. A., V. Formato, O. Adriani, et al. "Measurement of galactic cosmic-ray deuteron spectrum in the PAMELA experiment." Bulletin of the Russian Academy of Sciences: Physics 77, no. 5 (2013): 606–8. http://dx.doi.org/10.3103/s1062873813050274.

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Tomassetti, Nicola, and Jie Feng. "The Curious Case of High-energy Deuterons in Galactic Cosmic Rays." Astrophysical Journal 835, no. 2 (2017): L26. http://dx.doi.org/10.3847/2041-8213/835/2/l26.

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Koldobskiy, S. A., O. Adriani, G. C. Barbarino, et al. "Galactic deuteron spectrum measured in PAMELA experiment." February 1, 2013. https://doi.org/10.1088/1742-6596/409/1/012040.

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5

Chen, Jun-Liang, Su-Jun Yun, Tie-Kuang Dong, Zhong-Zhou Ren, and Xiao-Ping Zhang. "Studies of the radiation environment on the Mars surface using the Geant4 toolkit." Nuclear Science and Techniques 33, no. 1 (2022). http://dx.doi.org/10.1007/s41365-022-00987-2.

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AbstractThe radiation environment on the surface of Mars is a potential threat for future manned exploration missions to this planet. In this study, a simple geometrical model was built for simulating the radiation environment on the Mars surface caused by galactic cosmic rays; the model was built and studied using the Geant4 toolkit. The simulation results were compared with the data reported by a radiation assessment detector (RAD). The simulated spectra of neutrons, photons, protons, $$\alpha$$ α particles, and particle groups $$Z=3$$ Z = 3 –5, $$Z=6$$ Z = 6 –8, $$Z=9$$ Z = 9 –13, and $$Z=1
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Dissertations / Theses on the topic "Galactic deuteron"

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LENNI, ALEX. "Study of cosmic-ray proton and deuteron solar modulation and its relevence for indirect dark-matter searches with the PAMELA and GAPS experiments." Doctoral thesis, Università degli Studi di Trieste, 2022. http://hdl.handle.net/11368/3014975.

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Cosmic rays (CRs) are electrically charged particles accelerated by astrophysical powerful sources. CRs consists mainly of protons and helium nuclei and in minimal part of other nuclei and electrons. Among these, there are the deuterons, i.e. the deuterium nuclei, which are produced as a secondary component from interactions of CRs with the interstellar medium. During their voyage in the Galaxy, CRs experience energy losses, fragmentations in secondary products, trajectory deflections by galactic magnetic fields and generally a change of the spectral features. Before reaching the Earth, CRs p
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