Observation of a Spectral Hardening in Cosmic Ray Boron Spectrum with the DAMPE Space Mission

Alemanno, F.; Altomare, C.; An, Q.; Azzarello, P.; Barbato, F.  c.  t.; Bernardini, P.; X.  j., Bi; Boutin, H.; Cagnoli, I.; Cai, M.  s.; Casilli, E.; Catanzani, E.; Chang, J.; Chen, D.  y.; Chen, J.  l.; Chen, Z.  f.; Chen, Z.  x.; Coppin, P.; Cui, M.  y.; Cui, T.  s.; Cui, Y.  x.; De Mitri, I.; De Palma, F.; Di Giovanni, A.; Dong, T.  k.; Dong, Z.  x.; Donvito, G.; Droz, D.; Duan, J.  l.; Duan, K.  k.; Fan, R.  r.; Fan, Y.  z.; Fang, F.; Fang, K.; Feng, C.  q.; Feng, L.; Frieden, J.  m.; Fusco, P.; Gao, M.; Gargano, F.; Ghose, E.; Gong, K.; Gong, Y.  z.; Guo, D.  y.; Guo, J.  h.; Han, S.  x.; Y.  m., Hu; Huang, G.  s.; Huang, X.  y.; Huang, Y.  y.; Ionica, M.; Jiang, L.  y.; Jiang, Y.  z.; Jiang, W.; Kong, J.; Kotenko, A.; Kyratzis, D.; Lei, S.  j.; W.  h., Li; W.  l., Li; Li, X.; X.  q., Li; Liang, Y.  m.; Liu, C.  m.; Liu, H.; Liu, J.; Liu, S.  b.; Liu, Y.; Loparco, F.; Ma, M.; P.  x., Ma; Ma, T.; X.  y., Ma; Marsella, G.; Mazziotta, M.  n.; Mo, D.; Niu, X.  y.; Parenti, A.; Peng, W.  x.; Peng, X.  y.; Perrina, C.; Putti-Garcia, E.; Qiao, R.; Rao, J.  n.; Sarkar, R.; Savina, P.; Serpolla, A.; Shangguan, Z.; Shen, W.  h.; Shen, Z.  q.; Shen, Z.  t.; Silveri, L.; Song, J.  x.; Stolpovskiy, M.; Su, H.; Su, M.; Sun, H.  r.; Sun, Z.  y.; Surdo, A.; Teng, X.  j.; Tykhonov, A.; Wang, J.  z.; Wang, L.  g.; Wang, S.; Wang, X.  l.; Wang, Y.  f.; Wang, Y.; Wei, D.  m.; Wei, J.  j.; Wei, Y.  f.; Wu, D.; Wu, J.; S.  s., Wu; Wu, X.; Xia, Z.  q.; E.  h., Xu; H.  t., Xu; Xu, J.; Z.  h., Xu; Z.  l., Xu; Z.  z., Xu; Xue, G.  f.; Yang, H.  b.; Yang, P.; Yang, Y.  q.; Yao, H.  j.; Y.  h., Yu; Yuan, Q.; Yue, C.; Zang, J.  j.; Zhang, S.  x.; Zhang, W.  z.; Zhang, Yan; Zhang, Yi; Zhang, Y.  j.; Zhang, Y.  l.; Zhang, Y.  p.; Zhang, Y.  q.; Zhang, Z.; Zhang, Z.  y.; Zhao, C.; Zhao, H.  y.; Zhao, X.  f.; Zhou, C.  y.; Zhu, Y.; Null, Null

doi:10.1103/physrevlett.134.191001

: Secondary cosmic ray fluxes are important probes of the propagation and interaction of high-energy particles in the Galaxy. Recent measurements of primary and secondary cosmic ray nuclei have revealed unexpected spectral features that demand a deeper understanding. In this work we report the direct measurement of the cosmic ray boron spectrum from 10 GeV/n to 8 TeV/n with eight years of data collected by the Dark Matter Particle Explorer (DAMPE) mission. The measured spectrum shows a hardening at 182±24 GeV/n with a spectral index of γ_{1}=3.02±0.01 before the break and an index change of Δγ=0.31±0.05 after the break. A simple power law model is disfavored at a confidence level of 8σ. Compared with the hardenings measured in the DAMPE proton and helium spectra, the secondary boron spectrum hardens roughly twice as much as these primaries, which is consistent with a propagation related mechanism to interpret the spectral hardenings of cosmic rays observed at hundreds of GeV/n.