Finsler Geometry vs. Dark Matter and Dark Energy HypothesisCHANG ZheInstitute of High Energy PhysicsChinese Academy of Sciences17112009 at ITPI. Experimental observations1. Galactic rotation curves
Fare clic per modificare stileFare clic per modificare gli stili del testo dello schemaSecondo livelloTerzo livelloQuarto livelloQuinto livelloWIMP dark matter starsFabio IoccoInstitut de Physique Th
单击此处编辑母版标题样式单击此处编辑母版文本样式第二级第三级第四级第五级Propertiesdark matternon-baryonew bsm particles must existnon-relativisticstableCDMleading candidates:WIMPs 1 GeV.Axions .ALPsDark Photons.....The U(1)
マスタ タイトルの書式設定マスタ テキストの書式設定第 2 レベル第 3 レベル第 4 レベル第 5 レベル Enhancement of Line Gamma Ray Signature from Bino-like Dark Matter Annihilation due to CP ViolationYoshio Sato (Saitama UniversityTechnical Univ
Direct Search and LHC Detection of the Simplest Dark MatterXiao-Gang He NTUSJTUThe Simplest Dark Matter ModelDirect SearchImplications for Higgs search at LHCDiscussions and ConclusionsRotation v