[1] |
PLANCK collaboration. Planck 2015 results. XⅢ. Cosmological parameters[J]. Astron. Astrophys., 2016, 594(A):13
|
[2] |
JUNGMAN G, KAMIONKOWSKI M, GRIEST K. Supersymmetric dark matter[J]. Phys. Rept., 1996, 267:195-373
|
[3] |
BERTONE G, HOOPER D, SILK J. Particle dark matter:evidence, candidates and constraints[J]. Phys. Rept., 2005, 405:279-390
|
[4] |
BI X J, YIN P F, YUAN Q. Status of dark matter detection[J]. Front. Phys., 2013, 8:794-827
|
[5] |
PAMELA collaboration. An anomalous positron abundance in cosmic rays with energies 1.5~100 GeV[J]. Nature, 2009, 458:607-609
|
[6] |
Fermi-LAT collaboration. Measurement of separate cosmic-ray electron and positron spectra with the Fermi Large Area Telescope[J]. Phys. Rev. Lett., 2012, 108:011103
|
[7] |
AMS collaboration. First result from the Alpha Magnetic Spectrometer on the International Space Station:precision measurement of the positron fraction in primary cosmic rays of 0.5~350 GeV[J]. Phys. Rev. Lett., 2013, 110:141102
|
[8] |
ATIC collaboration. An excess of cosmic ray electrons at energies of 300~800 GeV[J]. Nature, 2008, 456:362-365
|
[9] |
Fermi-LAT collaboration. Measurement of the cosmic ray e++ e- spectrum from 20 GeV to 1 TeV with the Fermi Large Area Telescope[J]. Phys. Rev. Lett., 2009, 102:181101
|
[10] |
AMS collaboration. High statistics measurement of the positron fraction in primary cosmic rays of 0.5~500 GeV with the Alpha Magnetic Spectrometer on the International Space Station[J]. Phys. Rev. Lett., 2014, 113:121101
|
[11] |
SHEN C S. Pulsars and very high-energy cosmic-ray electrons[J]. Astrophys. J. Lett., 1970, 162(L):181-186
|
[12] |
HOOPER D, BLASI P, DARIO SERPICO P. Pulsars as the sources of high energy cosmic ray positrons[J]. J. Cosmol. Astropart. Phys., 2009, 1:25
|
[13] |
YUKSEL H, KISTLER M D, STANEV T. TeV gamma rays from Geminga and the origin of the GeV positron excess[J]. Phys. Rev. Lett., 2009, 103:051101
|
[14] |
BERGSTROM L, BRINGMANN T, EDSJO J. New positron spectral features from supersymmetric dark matter-a way to explain the PAMELA data[J]. Phys. Rev.:D, 2008, 78:103520
|
[15] |
CIRELLI M, KADASTIK M, RAIDAL M, et al. Modelindependent implications of the e+, e-, anti-proton cosmic ray spectra on properties of dark matter[J]. Nucl. Phys. B, 2009, 813:1
|
[16] |
YIN P F, YUAN Q, LIU J, et al. PAMELA data and leptonically decaying dark matter[J]. Phys. Rev. D, 2009, 79:023512
|
[17] |
HAWC collaboration. Extended gamma-ray sources around pulsars constrain the origin of the positron flux at Earth[J]. Science, 2017, 358:911
|
[18] |
HOOPER D,GOODENOUGH L. Dark matter annihilation in the galactic centeras seen by the Fermi Gamma Ray Space Telescope[J]. Phys. Lett. B, 2011, 697:412-428
|
[19] |
CUI M Y, YUAN Q, SMING TSAI Y L, et al. Possible dark matter annihilation signal in the AMS-02 antiproton data[J]. Phys. Rev. Lett., 2017, 118:191101
|
[20] |
CUOCO A, KRAMER M, KORSMEIER M. Novel dark matter constraints from antiprotons in light of AMS-02[J]. Phys. Rev. Lett., 2017, 118:191102
|
[21] |
CHANG J. Dark matter particle explorer:the first Chinese cosmic ray and hard γ-ray detector in space[J]. Chin. J. Space Sci., 2014, 34:550-557
|
[22] |
DAMPE collaboration. Cosmic-ray electron + positron spectrum from 7 GeV to 2 TeV with the Fermi Large Area Telescope[J]. Astropart. Phys., 2017, 95:6
|
[23] |
YU Yuhong, SUN Zhiyu, SU Hong, et al. The plastic scintillator detector for DAMPE[J]. Astropart. Phys., 2017, 94:1-10
|
[24] |
AZZARELLO P, AMBROSI G, ASFANDIYAROV R, et al. The DAMPE silicon-tungsten tracker[J]. Nucl. Instrum. Meth. Phys. Res.:A, 2016, 831:378-384
|
[25] |
ZHANG Zhiyong, ZHANG Yunlong, DONG Jianing,et al. Design of a high dynamic range photomultiplier base board for the BGO ECAL of DAMPE[J]. Nucl. Instrum. Meth. Phys. Res.:A, 2015, 780:21-26
|
[26] |
HE M, MAO T, CHANG J, et al. GEANT4 Simulation of Neutron Detector DAMPE[J]. Acta Astron. Sin., 2016, 57:1-8
|
[27] |
CHANG J. On the detection and identification of cosmic gamma-rays in a cosmic ray detector[J]. BMJ, 1999, 1(2):136-137
|
[28] |
CHANG J, ADAMS J H, AHN H S, et al. Resolving electrons from protons in ATIC[J]. Adv. Space Res., 2008, 42:431-436
|
[29] |
DAMPE collaboration. Direct detection of a break in the teraelectronvolt cosmic-ray spectrum of electrons and positrons[J]. Nature, 2017, 552:63-66
|
[30] |
YUE Chuan, ZANG Jingjing, DONG Tiekuang, et al. A parameterized energy correction method for electromagnetic showers in BGO-ECAL of DAMPE[J]. Nucl. Instrum. Meth. Phys. Res.:A, 2017, 856:11
|
[31] |
Fermi LAT Collaboration. Cosmic-ray electron+ positron spectrum from 7 GeV to 2 TeV with the Fermi Large Area Telescope[J]. Phys. Rev.:D, 2017, 95:082007
|
[32] |
HESS Collaboration. The energy spectrum of cosmic-ray electrons at TeV energies[J]. Phys. Rev. Lett., 2008, 101:261104
|
[33] |
HESS Collaboration. Probing the ATIC peak in the cosmic-ray electron spectrum with HESS[J]. Astron. Astrophys., 2009, 508:561-564
|