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相关论文: Dark matter gets DAMPE at high energies

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Progress in observational cosmology over the past five years has established that the Universe is dominated dynamically by dark matter and dark energy. Both these new and apparently independent forms of matter-energy have properties that…

天体物理学 · 物理学 2009-11-10 J. M. Overduin , P. S. Wesson

In this review we discuss constraints on minimal supersymmetric models of particle physics implied by the recent astrophysical observations of WMAP. Although the prospects of detecting supersymmetry increase and 90 percent of the available…

高能物理 - 唯象学 · 物理学 2011-05-05 A. B. Lahanas , N. E. Mavromatos , D. V. Nanopoulos

We provide conservative bounds on the dark matter cross-section and lifetime from final state radiation produced by annihilation or decay into charged leptons, either directly or via an intermediate particle $\phi$. Our analysis utilizes…

高能物理 - 唯象学 · 物理学 2009-09-04 Rouven Essig , Neelima Sehgal , Louis E. Strigari

Light dark matter is a compelling experimental target in light of stringent constraints on heavier WIMPs. However, for a sub-MeV WIMP, the universe is sufficiently well understood at temperatures below 10 MeV that there is no room for it to…

高能物理 - 唯象学 · 物理学 2018-03-02 Daniel Green , Surjeet Rajendran

Taking into account spins, we classify all two-body non-relativistic Dark Matter annihilation channels to the allowed polarization states of Standard Model particles, computing the energy spectra of the stable final-state particles relevant…

高能物理 - 唯象学 · 物理学 2013-10-07 Marco Cirelli , Mario Kadastik , Martti Raidal , Alessandro Strumia

The DArk Matter Particle Explorer (DAMPE) is well suitable for searching for monochromatic and sharp $\gamma$-ray structures in the GeV$-$TeV range thanks to its unprecedented high energy resolution. In this work, we search for $\gamma$-ray…

高能天体物理现象 · 物理学 2022-12-07 Francesca Alemanno , Qi An , Philipp Azzarello , Felicia Carla Tiziana Barbato , Paolo Bernardini , Xiao-Jun Bi , Ming-Sheng Cai , Elisabetta Casilli , Enrico Catanzani , Jin Chang , Deng-Yi Chen , Jun-Ling Chen , Zhan-Fang Chen , Ming-Yang Cui , Tian-Shu Cui , Yu-Xing Cui , Hao-Ting Dai , Antonio De Benedittis , Ivan De Mitri , Francesco de Palma , Maksym Deliyergiyev , Margherita Di Santo , Qi Ding , Tie-Kuang Dong , Zhen-Xing Dong , Giacinto Donvito , David Droz , Jing-Lai Duan , Kai-Kai Duan , Domenico D'Urso , Rui-Rui Fan , Yi-Zhong Fan , Fang Fang , Kun Fang , Chang-Qing Feng , Lei Feng , Piergiorgio Fusco , Min Gao , Fabio Gargano , Ke Gong , Yi-Zhong Gong , Dong-Ya Guo , Jian-Hua Guo , Shuang-Xue Han , Yi-Ming Hu , Guang-Shun Huang , Xiao-Yuan Huang , Yong-Yi Huang , Maria Ionica , Wei Jiang , Jie Kong , Andrii Kotenko , Dimitrios Kyratzis , Shi-Jun Lei , Shang Li , Wen-Hao Li , Wei-Liang Li , Xiang Li , Xian-Qiang Li , Yao-Ming Liang , Cheng-Ming Liu , Hao Liu , Jie Liu , Shu-Bin Liu , Yang Liu , Francesco Loparco , Chuan-Ning Luo , Miao Ma , Peng-Xiong Ma , Tao Ma , Xiao-Yong Ma , Giovanni Marsella , Mario Nicola Mazziotta , Dan Mo , Maria Mu , Xiao-Yang Niu , Xu Pan , Andrea Parenti , Wen-Xi Peng , Xiao-Yan Peng , Chiara Perrina , Rui Qiao , Jia-Ning Rao , Arshia Ruina , Zhi Shangguan , Wei-Hua Shen , Zhao-Qiang Shen , Zhong-Tao Shen , Leandro Silveri , Jing-Xing Song , Mikhail Stolpovskiy , Hong Su , Meng Su , Hao-Ran Sun , Zhi-Yu Sun , Antonio Surdo , Xue-Jian Teng , Andrii Tykhonov , Jin-Zhou Wang , Lian-Guo Wang , Shen Wang , Shu-Xin Wang , Xiao-Lian Wang , Ying Wang , Yan-Fang Wang , Yuan-Zhu Wang , Da-Ming Wei , Jia-Ju Wei , Yi-Feng Wei , Di Wu , Jian Wu , Li-Bo Wu , Sha-Sha Wu , Xin Wu , Zi-Qing Xia , En-Heng Xu , Hai-Tao Xu , Zhi-Hui Xu , Zun-Lei Xu , Zi-Zong Xu , Guo-Feng Xue , Hai-Bo Yang , Peng Yang , Ya-Qing Yang , Hui-Jun Yao , Yu-Hong Yu , Guan-Wen Yuan , Qiang Yuan , Chuan Yue , Jing-Jing Zang , Sheng-Xia Zhang , Wen-Zhang Zhang , Yan Zhang , Yi Zhang , Yong-Jie Zhang , Yun-Long Zhang , Ya-Peng Zhang , Yong-Qiang Zhang , Zhe Zhang , Zhi-Yong Zhang , Cong Zhao , Hong-Yun Zhao , Xun-Feng Zhao , Chang-Yi Zhou , Yan Zhu , Yun-Feng Liang

We consider a charged leptophilic extension of the Standard Model of particle physics as a minimal dark sector. It accomodates a WIMP paradigm at the TeV-scale that is sufficient to solve all small-scale problems of $\Lambda$CDM and explain…

高能物理 - 唯象学 · 物理学 2018-12-07 Ottavia Balducci , Stefan Hofmann , Alexis Kassiteridis

The era of precision cosmology has revealed that about 85% of the matter in the universe is dark matter. Two well-motivated candidates are weakly interacting massive particles (WIMPs) and weakly interacting sub-eV particles (WISPs) (e.g.…

This is the mini-review on Dark Matter in the 2012 edition of the Particle Data Group's Review of Particle Properties. After briefly summarizing the arguments in favor of the existence of Dark Matter, we list possible candidates, ranging in…

高能物理 - 唯象学 · 物理学 2012-04-12 Manuel Drees , Gilles Gerbier

The diffuse galactic EGRET gamma ray data show a clear excess for energies above 1 GeV in comparison with the expectations from conventional galactic models. This excess shows all the features expected from Dark Matter WIMP Annihilation:…

天体物理学 · 物理学 2009-09-29 W. de Boer , I. Gebauer , C. Sander , M. Weber , V. Zhukov

Observations by the WMAP experiment have identified an excess of microwave emission from the center of the Milky Way. It has previously been shown that this "WMAP Haze" could be synchrotron emission from relativistic electrons and positrons…

天体物理学 · 物理学 2008-11-26 Dan Hooper , Gabrijela Zaharijas , Douglas P. Finkbeiner , Gregory Dobler

We present a model of weak scale Dark Matter (DM) where the thermal DM density is set by the lepton asymmetry due to the presence of higher dimension lepton violating operators. In these models there is generically a separation between the…

高能物理 - 唯象学 · 物理学 2010-04-06 Timothy Cohen , Kathryn M. Zurek

Dark matter might be in the form of a dark plasma in the Milky Way halo. Specifically, we consider here a hidden sector consisting of a light `dark electron' and a much heavier `dark proton', each charged under an unbroken $U(1)'$ gauge…

高能物理 - 唯象学 · 物理学 2021-02-03 Lei Zu , R. Foot , Yi-Zhong Fan , Lei Feng

We propose a novel mechanism to explain the positron excesses, which are observed by satellite-based telescopes including PAMELA and AMS-02, in dark matter (DM) scenarios. The novelty behind the proposal is that it makes direct use of DM…

高能物理 - 唯象学 · 物理学 2018-05-09 Doojin Kim , Jong-Chul Park , Seodong Shin

The DArk Matter Particle Explorer (DAMPE), also known as Wukong in China, launched on December 17, 2015, is a new high energy cosmic ray and {\gamma}-ray satellite-borne observatory in space. One of the main scientific goals of DAMPE is to…

We develop a comprehensive study of the gamma-ray flux observed by H.E.S.S. in 5 regions of the Galactic Center (GC). Motivated by previous works on a possible Dark Matter (DM) explanation for the TeV cut-off observed in the innermost $\sim…

高能天体物理现象 · 物理学 2023-11-22 Jaume Zuriaga-Puig , Viviana Gammaldi , Daniele Gaggero , Thomas Lacroix , Miguel Ángel Sánchez-Conde

It has been long discussed that cosmic rays may contain signals of dark matter. In the last couple of years an anomaly of cosmic-ray positrons has drawn a lot of attentions, and recently an excess in cosmic-ray anti-proton has been reported…

高能物理 - 唯象学 · 物理学 2016-06-29 Shin'ichiro Ando , Koji Ishiwata

In this paper we investigate the phenomenology of the electron flavored Dirac dark matter with two types of portal interactions. We analyze constraints from the electron magnetic moment anomaly, LHC searches of singly charged scalar, dark…

高能物理 - 唯象学 · 物理学 2018-06-06 Wei Chao , Huai-Ke Guo , Hao-Lin Li , Jing Shu

We present exoplanets as new targets to discover Dark Matter (DM). Throughout the Milky Way, DM can scatter, become captured, deposit annihilation energy, and increase the heat flow within exoplanets. We estimate upcoming infrared telescope…

高能物理 - 唯象学 · 物理学 2023-04-26 Rebecca K. Leane , Juri Smirnov

Direct detection experiments are poised to detect dark matter in the form of weakly interacting massive particles (WIMPs). The signals expected in these experiments depend on the ultra-local WIMP density and velocity distribution. Firstly…

宇宙学与河外天体物理 · 物理学 2012-02-14 Anne M. Green