Measurement of the cosmic ray helium energy spectrum from 70 GeV to 80 TeV with the DAMPE space mission
Creators: name: Alemanno, F.
name: An, Q.
name: Azzarello, P.
name: Barbato, F. C. T.
name: Bernardini, P.
name: Bi, X. J.
name: Cai, M. S.
name: Catanzani, E.
name: Chang, J.
name: Chen, D. Y.
name: Chen, J. L.
name: Chen, Z. F.
name: Cui, M. Y.
name: Cui, T. S.
name: Cui, Y. X.
name: Dai, H. T.
name: D'Amone, A.
name: De Benedittis, A.
name: De Mitri, I.
name: de Palma, F.
name: Deliyergiyev, M.
name: Di Santo, M.
name: Dong, T. K.
name: Dong, Z. X.
name: Donvito, G.
name: Droz, D.
name: Duan, J. L.
name: Duan, K. K.
name: D'Urso, D.
name: Fan, R. R.
name: Fan, Y. Z.
name: Fang, K.
name: Fang, F.
name: Feng, C. Q.
name: Feng, L.
name: Fusco, P.
name: Gao, M.
name: Gargano, F.
name: Gong, K.
name: Gong, Y. Z.
name: Guo, D. Y.
name: Guo, J. H.
name: Guo, X. L.
name: Han, S. X.
name: Hu, Y. M.
name: Huang, G. S.
name: Huang, X. Y.
name: Huang, Y. Y.
name: Ionica, M.
name: Jiang, W.
name: Kong, J.
name: Kotenko, A.
name: Kyratzis, D.
name: Lei, S. J.
name: Li, S.
name: Li, W. L.
name: Li, X.
name: Li, X. Q.
name: Liang, Y. M.
name: Liu, C. M.
name: Liu, H.
name: Liu, J.
name: Liu, S. B.
name: Liu, W. Q.
name: Liu, Y.
name: Loparco, F.
name: Luo, C. N.
name: Ma, M.
name: Ma, P. X.
name: Ma, T.
name: Ma, X. Y.
name: Marsella, G.
name: Mazziotta, M. N.
name: Mo, D.
name: Niu, X. Y.
name: Pan, X.
name: Parenti, A.
name: Peng, W. X.
name: Peng, X. Y.
name: Perrina, C.
name: Qiao, R.
name: Rao, J. N.
name: Ruina, A.
name: Salinas, M. M.
name: Shang, G. Z.
name: Shen, W. H.
name: Shen, Z. Q.
name: Shen, Z. T.
name: Silveri, L.
name: Song, J. X.
name: Stolpovskiy, M.
name: Su, H.
name: Su, M.
name: Sun, Z. Y.
name: Surdo, A.
name: Teng, X. J.
name: Tykhonov, A.
name: Wang, H.
name: Wang, J. Z.
name: Wang, L. G.
name: Wang, S.
name: Wang, X. L.
name: Wang, Y.
name: Wang, Y. F.
name: Wang, Y. Z.
name: Wang, Z. M.
name: Wei, D. M.
name: Wei, J. J.
name: Wei, Y. F.
name: Wen, S. C.
name: Wu, D.
name: Wu, J.
name: Wu, L. B.
name: Wu, S. S.
name: Wu, X.
name: Xia, Z. Q.
name: Xu, H. T.
name: Xu, Z. H.
name: Xu, Z. L.
name: Xu, Z. Z.
name: Xue, G. F.
name: Yang, H. B.
name: Yang, P.
name: Yang, Y. Q.
name: Yao, H. J.
name: Yu, Y. H.
name: Yuan, G. W.
name: Yuan, Q.
name: Yue, C.
name: Zang, J. J.
name: Zhang, F.
name: Zhang, S. X.
name: Zhang, W. Z.
name: Zhang, Y.
name: Zhang, Y. J.
name: Zhang, Y. L.
name: Zhang, Y. P.
name: Zhang, Y. Q.
name: Zhang, Z.
name: Zhang, Z. Y.
name: Zhao, C.
name: Zhao, H. Y.
name: Zhao, X. F.
name: Zhou, C. Y.
name: Zhu, Y.
Publisher: name: arXiv
Year: 2021
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences
subject: FOS: Physical sciences

description: The measurement of the energy spectrum of cosmic ray helium nuclei from 70 GeV to 80 TeV using 4.5 years of data recorded by the DArk Matter Particle Explorer (DAMPE) is reported in this work. A hardening of the spectrum is observed at an energy of about 1.3 TeV, similar to previous observations. In addition, a spectral softening at about 34 TeV is revealed for the first time with large statistics and well controlled systematic uncertainties, with an overall significance of $4.3σ$. The DAMPE spectral measurements of both cosmic protons and helium nuclei suggest a particle charge dependent softening energy, although with current uncertainties a dependence on the number of nucleons cannot be ruled out.
description: 11 pages, 13 figures, published in Phys. Rev. Lett. Add one more digit for first three columns in Table S2