Measurement of the cosmic ray proton spectrum from 40 GeV to 100 TeV with the DAMPE satellite-Reference-Cited by-同舟云学术

Measurement of the cosmic ray proton spectrum from 40 GeV to 100 TeV with the DAMPE satellite

Published:2019-09-06 Issue:9 Volume:5 Page:
ISSN:2375-2548
Container-title:Science Advances
language:en
Short-container-title:Sci. Adv.

Author:

,An Q.¹²,Asfandiyarov R.³^ORCID,Azzarello P.³^ORCID,Bernardini P.⁴⁵,Bi X. J.⁶⁷^ORCID,Cai M. S.⁸⁹,Chang J.⁸⁹,Chen D. Y.⁷⁸,Chen H. F.¹²,Chen J. L.¹⁰,Chen W.⁷⁸,Cui M. Y.⁸^ORCID,Cui T. S.¹¹,Dai H. T.¹²,D’Amone A.⁴⁵^ORCID,De Benedittis A.⁴⁵^ORCID,De Mitri I.¹²¹³^ORCID,Di Santo M.⁴⁵,Ding M.⁷¹⁰^ORCID,Dong T. K.⁸^ORCID,Dong Y. F.⁶^ORCID,Dong Z. X.¹¹,Donvito G.¹⁴,Droz D.³,Duan J. L.¹⁰^ORCID,Duan K. K.⁷⁸,D’Urso D.¹⁵^ORCID,Fan R. R.⁶^ORCID,Fan Y. Z.⁸⁹,Fang F.¹⁰,Feng C. Q.¹²,Feng L.⁸,Fusco P.¹⁴¹⁶^ORCID,Gallo V.³,Gan F. J.¹²,Gao M.⁶,Gargano F.¹⁴^ORCID,Gong K.⁶,Gong Y. Z.⁸,Guo D. Y.⁶,Guo J. H.⁸⁹^ORCID,Guo X. L.⁸⁹,Han S. X.¹¹,Hu Y. M.⁸,Huang G. S.¹²,Huang X. Y.⁸,Huang Y. Y.⁸,Ionica M.¹⁵,Jiang W.⁸⁹,Jin X.¹²,Kong J.¹⁰,Lei S. J.⁸,Li S.⁷⁸,Li W. L.¹¹,Li X.⁸^ORCID,Li X. Q.¹¹,Li Y.¹⁰,Liang Y. F.⁸^ORCID,Liang Y. M.¹¹,Liao N. H.⁸,Liu C. M.¹²,Liu H.⁸,Liu J.¹⁰,Liu S. B.¹²,Liu W. Q.¹⁰,Liu Y.⁸,Loparco F.¹⁴¹⁶^ORCID,Luo C. N.⁸⁹,Ma M.¹¹,Ma P. X.⁸⁹^ORCID,Ma S. Y.¹²^ORCID,Ma T.⁸,Ma X. Y.¹¹,Marsella G.⁴⁵,Mazziotta M. N.¹⁴^ORCID,Mo D.¹⁰,Niu X. Y.¹⁰,Pan X.⁸⁹,Peng W. X.⁶,Peng X. Y.⁸,Qiao R.⁶^ORCID,Rao J. N.¹¹,Salinas M. M.³,Shang G. Z.¹¹,Shen W. H.¹¹,Shen Z. Q.⁷⁸,Shen Z. T.¹²^ORCID,Song J. X.¹¹,Su H.¹⁰,Su M.⁸¹⁷^ORCID,Sun Z. Y.¹⁰^ORCID,Surdo A.⁵^ORCID,Teng X. J.¹¹,Tykhonov A.³^ORCID,Vitillo S.³,Wang C.¹²^ORCID,Wang H.¹¹,Wang H. Y.⁶,Wang J. Z.⁶,Wang L. G.¹¹,Wang Q.¹²,Wang S.⁷⁸,Wang X. H.¹⁰,Wang X. L.¹²,Wang Y. F.¹²,Wang Y. P.⁷⁸^ORCID,Wang Y. Z.⁷⁸^ORCID,Wang Z. M.¹²¹³,Wei D. M.⁸⁹^ORCID,Wei J. J.⁸,Wei Y. F.¹²,Wen S. C.¹²,Wu D.⁶,Wu J.⁸⁹,Wu L. B.¹²,Wu S. S.¹¹,Wu X.³^ORCID,Xi K.¹⁰,Xia Z. Q.⁸⁹^ORCID,Xu H. T.¹¹,Xu Z. H.⁸⁹,Xu Z. L.⁸,Xu Z. Z.¹²,Xue G. F.¹¹,Yang H. B.¹⁰,Yang P.¹⁰,Yang Y. Q.¹⁰,Yang Z. L.¹⁰,Yao H. J.¹⁰,Yu Y. H.¹⁰,Yuan Q.⁸⁹^ORCID,Yue C.⁷⁸^ORCID,Zang J. J.⁸,Zhang F.⁶,Zhang J. Y.⁶,Zhang J. Z.¹⁰,Zhang P. F.⁸,Zhang S. X.¹⁰^ORCID,Zhang W. Z.¹¹,Zhang Y.⁷⁸^ORCID,Zhang Y. J.¹⁰,Zhang Y. L.¹²,Zhang Y. P.¹⁰,Zhang Y. Q.⁷⁸,Zhang Z.⁸,Zhang Z. Y.¹²,Zhao H.⁶,Zhao H. Y.¹⁰,Zhao X. F.¹¹,Zhou C. Y.¹¹,Zhou Y.¹⁰^ORCID,Zhu X.¹²,Zhu Y.¹¹,Zimmer S.³^ORCID

Affiliation:

1. State Key Laboratory of Particle Detection and Electronics, University of Science and Technology of China, Hefei 230026, China.

2. Department of Modern Physics, University of Science and Technology of China, Hefei 230026, China.

3. Department of Nuclear and Particle Physics, University of Geneva, Geneva CH-1211, Switzerland.

4. Dipartimento di Matematica e Fisica E. De Giorgi, Università del Salento, I-73100 Lecce, Italy.

5. Istituto Nazionale di Fisica Nucleare (INFN)–Sezione di Lecce, I-73100 Lecce, Italy.

6. Institute of High Energy Physics, Chinese Academy of Sciences, Yuquan Road 19B, Beijing 100049, China.

7. University of Chinese Academy of Sciences, Yuquan Road 19A, Beijing 100049, China.

8. Key Laboratory of Dark Matter and Space Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210033, China.

9. School of Astronomy and Space Science, University of Science and Technology of China, Hefei 230026, China.

10. Institute of Modern Physics, Chinese Academy of Sciences, Nanchang Road 509, Lanzhou 730000, China.

11. National Space Science Center, Chinese Academy of Sciences, Nanertiao 1, Zhongguancun, Haidian District, Beijing 100190, China.

12. Gran Sasso Science Institute (GSSI), Via Iacobucci 2, I-67100 L’Aquila, Italy.

13. Istituto Nazionale di Fisica Nucleare (INFN)–Laboratori Nazionali del Gran Sasso, Assergi, I-67100 L’Aquila, Italy.

14. Istituto Nazionale di Fisica Nucleare (INFN)–Sezione di Bari, I-70125, Bari, Italy.

15. Istituto Nazionale di Fisica Nucleare (INFN)–Sezione di Perugia, I-06123 Perugia, Italy.

16. Dipartimento di Fisica “M. Merlin” dell’Università e del Politecnico di Bari, I-70126 Bari, Italy.

17. Department of Physics and Laboratory for Space Research, The University of Hong Kong, Pok Fu Lam, Hong Kong, China.

Abstract

DAMPE satellite has directly measured the cosmic ray proton spectrum from 40 GeV to 100 TeV and revealed a new feature at about 13.6 TeV.

Funder

National Natural Science Foundation of China

National key R&D program of China

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

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