<i>L_α</i>Line of Dark Positronium as a Nongravitational Detection of DM  

作　　者：V. Burdyuzha V. Charugin 

机构地区：[1]Astro-Space Center, Lebedev Physical Institute, Russian Academy of Sciences, Moscow, Russia [2]Moscow Pedagogical State University, Moscow, Russia

出　　处：《Journal of Modern Physics》2015年第13期1833-1839,共7页现代物理（英文）

摘　　要：An attempt to predict the new atomic dark matter lines is done on the example of a dark lepton atom-positronium. Its Layman-alpha line with the energy near 3 GeV may be observable if the appropriate conditions are realized. For this we have studied a γ-ray excess in the center of our galaxy. In principle, this excess may be produced by the Lα line of a dark positronium in the medium with Compton scattering. The possibility of observations of an annihilation line (E^300 TeV) of dark positronium is also predicted. Other proposals to observe the atomic dark matter are shortly described. Besides, Hα line (1.3μ) of usual positronum must be observable in the direction on the center of our galaxy.An attempt to predict the new atomic dark matter lines is done on the example of a dark lepton atom-positronium. Its Layman-alpha line with the energy near 3 GeV may be observable if the appropriate conditions are realized. For this we have studied a γ-ray excess in the center of our galaxy. In principle, this excess may be produced by the Lα line of a dark positronium in the medium with Compton scattering. The possibility of observations of an annihilation line (E^300 TeV) of dark positronium is also predicted. Other proposals to observe the atomic dark matter are shortly described. Besides, Hα line (1.3μ) of usual positronum must be observable in the direction on the center of our galaxy.

关 键 词：Atomic DARK Matter POSITRONIUM COMPTON Scattering 

分 类 号：R73[医药卫生—肿瘤]