Troy A. Porter, Robert P. Johnson, Peter W. Graham
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Solicited review article to appear in Annual Reviews of Astronomy and Astrophysics. 52 pages, 10 figures (higher resolution figures will appear in the journal article)
The existence of dark matter (DM) was first noticed by Zwicky in the 1930s, but its nature remains one of the great unsolved problems of physics. A variety of observations indicate that it is non-baryonic and non-relativistic. One of the preferred candidates for non-baryonic DM is a weakly interacting massive particle (WIMP) that in most models is stable. WIMP self-annihilation can produce cosmic rays, gamma rays, and other particles with signatures that may be detectable. Hints of anomalous cosmic-ray spectra found by recent experiments, such as PAMELA, have motivated interesting interpretations in terms of DM annihilation and/or decay. However, these signatures also have standard astrophysical interpretations, so additional evidence is needed in order to make a case for detection of DM annihilation or decay. Searches by the Fermi Large Area Telescope for gamma-ray signals from clumps, nearby dwarf spheroidal galaxies, and galaxy clusters have also been performed, along with measurements of the diffuse Galactic and extragalactic gamma-ray emission. In addition, imaging atmospheric Cherenkov telescopes like HESS, MAGIC, and VERITAS have reported on searches for gamma-ray emission from dwarf galaxies. In this review, we examine the status of searches for particle DM by these instruments and discuss the interpretations and resulting DM limits.
Astroparticle and particle physics at ultra-high energy: results from the Pierre Auger Observatory
Pierre Auger合作组织的科学成果涵盖了各种互补的研究领域。对超高能宇宙射线(UHECR)起源的研究是基于对原初射线的能谱和质量组成的测量、对多信使的研究以及广泛的各向异性研究。利用收集到的数据,还可以探索在人造加速器无法达到的能量下强子相互作用的特征,并评估非标准物理效应的存在。一个选择的最新成果,并讨论了新兴的图片。
Superheavy dark matter from the natural inflation in light of the highest-energy astroparticle events
The Pennsylvania State University(宾夕法尼亚州立大学);Yukawa Institute for Theoretical Physics, Kyoto University(京都大学汤川理论物理研究所);Tokyo Metropolitan University(东京都立大学);Tohoku University(东北大学)