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The direct measurements of the cosmic electron-positron spectrum around 1 TeV made by DAMPE have induced many theoretical speculations about possible excesses in the data above the standard astrophysical predictions that might have the dark…

高能天体物理现象 · 物理学 2019-07-01 Konstantin Belotsky , Airat Kamaletdinov , Maxim Laletin , Maxim Solovyov

The precise measurements of energy spectra of cosmic ray positrons and/or electrons by recent experiments show clear excesses above 10 GeV. Moreover, a potential sharp spectral feature was suggested by the Dark Matter Particle Explorer…

高能物理 - 唯象学 · 物理学 2020-04-29 Lei Feng , Zhaofeng Kang , Qiang Yuan , Peng-Fei Yin , Yi-Zhong Fan

The tentative 1.4 TeV excess in the $e^+e^-$ spectrum measured by The DArk Matter Particle Explorer (DAMPE) motivates the possible existence of one or more local dark matter concentrated regions. In particular, Ultra-compact Micro Halos…

高能天体物理现象 · 物理学 2017-12-13 Fengwei Yang , Meng Su , Yue Zhao

The DArk Matter Particle Explorer (DAMPE) mission revealed a break in the spectrum of cosmic-ray electons and positrons. This is associated with an excess above the expected backgrounds at energies around 1 TeV. Several authors have argued…

宇宙学与河外天体物理 · 物理学 2019-02-21 Geoff Beck , Sergio Colafrancesco

The Dark Matter Particle Explorer (DAMPE) satellite detector announced its first result for measuring the cosmic-ray electron/positron (CRE) energy spectrum up to 4.6TeV, including a tentative peak-like event excess at (1.3-1.5)TeV. In this…

高能天体物理现象 · 物理学 2018-04-10 Shao-Feng Ge , Hong-Jian He , Yu-Chen Wang

Recent accurate measurements of cosmic ray electron flux by the Dark Matter Particle Explorer (DAMPE) reveal a sharp peak structure near 1.4 TeV, which is difficult to explain by standard astrophysical processes. In this letter, we propose…

高能天体物理现象 · 物理学 2020-01-20 Man Ho Chan , Chak Man Lee

The recent high energy electron and positron flux observed by the DAMPE experiment indicates possible excess events near 1.4 TeV. Such an excess may be evidence of dark matter annihilations or decays in a dark matter subhalo that is located…

高能物理 - 唯象学 · 物理学 2018-08-22 Xuewen Liu , Zuowei Liu

The cosmic electron energy spectrum recently observed by the DAMPE experiment exhibits two interesting features, including a break around 0.9 TeV and a sharp resonance near 1.4 TeV. In this analysis, we propose a dark matter explanation to…

高能物理 - 唯象学 · 物理学 2022-10-12 Xuewen Liu , Zuowei Liu , Yushan Su

Many studies have shown that either the nearby astrophysical source or dark matter (DM) annihilation/decay is required to explain the origin of high energy cosmic ray (CR) $e^\pm$, which are measured by many experiments, such as PAMELA and…

高能天体物理现象 · 物理学 2017-12-12 Bing-Bing Wang , Xiao-Jun Bi , Su-Jie Lin , Peng-fei Yin

The DArk Matter Particle Explorer (DAMPE) has reported a measurement of the flux of high energy cosmic ray electrons plus positrons (CREs) in the energy range between $25$ GeV and $4.6$ TeV. With unprecedented high energy resolution, the…

高能物理 - 唯象学 · 物理学 2018-02-07 Tong Li , Nobuchika Okada , Qaisar Shafi

PAMELA and ATIC recently reported excesses in e+ e- cosmic rays. Since the interpretation in terms of DM annihilations was found to be not easily compatible with constraints from photon observations, we consider the DM decay hypothesis and…

高能物理 - 唯象学 · 物理学 2009-05-26 Enrico Nardi , Francesco Sannino , Alessandro Strumia

Nearby sources may contribute to cosmic-ray electron (CRE) structures at high energies. Recently, the first DAMPE results on the CRE flux hinted at a narrow excess at energy ~1.4 TeV. We show that in general a spectral structure with a…

高能天体物理现象 · 物理学 2018-05-09 Xian-Jun Huang , Yue-Liang Wu , Wei-Hong Zhang , Yu-Feng Zhou

Recently, DAMPE has released its first results on the high-energy cosmic-ray electrons and positrons (CREs) from about $25$ GeV to $4.6$ TeV, which directly detect a break at $\sim 1$ TeV. This result gives us an excellent opportunity to…

高能天体物理现象 · 物理学 2018-05-02 Jia-Shu Niu , Tianjun Li , Ran Ding , Bing Zhu , Hui-Fang Xue , Yang Wang

Recently data from PAMELA, ATIC, FERMI-LAT and HESS show that there are $e^{\pm}$ excesses in the cosmic ray energy spectrum. PAMELA observed excesses only in $e^+$, but not in anti-proton spectrum. ATIC, FERMI-LAT and HESS observed…

高能物理 - 唯象学 · 物理学 2010-11-15 Xiao-Gang He

The flux of high-energy cosmic-ray electrons plus positrons recently measured by the DArk Matter Particle Explorer (DAMPE) exhibits a tentative peak excess at an energy of around $1.4$ TeV. In this paper, we consider the minimal gauged…

高能物理 - 唯象学 · 物理学 2018-09-03 Nobuchika Okada , Osamu Seto

The DArk Matter Particle Explorer (DAMPE), a high energy cosmic ray and $\gamma$-ray detector in space, has recently reported the new measurement of the total electron plus positron flux between 25 GeV and 4.6 TeV. A spectral softening at…

The DAMPE experiment has recently reported strong indications for the existence of an excess of high-energy electrons and positrons. If interpreted in terms of the annihilation of dark matter, the DAMPE result restricts the dark matter mass…

高能物理 - 唯象学 · 物理学 2017-12-05 Wei Chao , Qiang Yuan

The DArk Matter Particle Explorer (DAMPE) recently reported an excess of electrons/positrons above expected background fluxes even when a double power-law background spectrum is assumed. Several dark matter models that involve TeV-scale…

高能天体物理现象 · 物理学 2019-05-03 Geoff Beck , Sergio Colafrancesco

The Dark Matter Particle Explorer (DAMPE) recently released measurements of the electron spectrum with a hint of a narrow peak at about 1.4 TeV. We investigate dark matter (DM) models that could produce such a signal by annihilation in a…

高能物理 - 唯象学 · 物理学 2018-02-22 Peter Athron , Csaba Balazs , Andrew Fowlie , Yang Zhang

Several experiments have reported regions in the TeV sky with an excess of cosmic rays. Here we consider the possibility that the excess cosmic rays are coming from dark matter annihilation in nearby subhalos. We provide motivation for dark…

高能天体物理现象 · 物理学 2013-07-25 J. Patrick Harding
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