费解
发表于 2025-3-25 03:41:02
http://reply.papertrans.cn/17/1632/163116/163116_21.png
克制
发表于 2025-3-25 09:57:07
http://reply.papertrans.cn/17/1632/163116/163116_22.png
袋鼠
发表于 2025-3-25 14:41:48
Introduction to Dark Matter,The history of our understanding of dark matter is long and fascinating. It is not easy to indicate a precise starting point for these studies, since the question about the amount of low-luminosity material in the Milky Way was asked numerous times already in the 19th century.
INERT
发表于 2025-3-25 19:07:15
Direct Detection of WIMPsIn the next chapters we are going to give an overview of the main WIMP search strategies, which fall in three big categories.
Occlusion
发表于 2025-3-25 21:17:18
http://reply.papertrans.cn/17/1632/163116/163116_25.png
摄取
发表于 2025-3-26 01:36:45
Dark Matter Searches at the LHCThe Large Hadron Collider (LHC) is the world’s largest and most powerful particle accelerator, located at CERN. It consists of a 27-km ring of superconducting magnets with a number of accelerating structures to boost the energy of the particles.
增减字母法
发表于 2025-3-26 05:59:20
The EFT Approach and Its ValidityGiven the plethora of particle physics model beyond the SM providing a WIMP candidate, it is highly desirable to study the signatures of this DM candidate in a model-independent way. In this and the following chapters, we are going to analyse the two main tools for such a model independent study, namely effective operators and simplified models.
painkillers
发表于 2025-3-26 10:53:43
The Relic Density ConstraintThe calculation of the relic abundance of DM particles in the standard freeze-out mechanism was discussed in Sect. ..
intention
发表于 2025-3-26 15:25:20
http://reply.papertrans.cn/17/1632/163116/163116_29.png
BUOY
发表于 2025-3-26 20:30:49
Focus on AMS-02 Anti-protons Resultson fraction .. Indeed, DM annihilation could lead to a similar signal in antiprotons, where the degeneracy with a pulsar explanation is not present, since antiprotons are too heavy to be produced by pulsars’ magnetic fields.