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Titlebook: Aspects of WIMP Dark Matter Searches at Colliders and Other Probes; Enrico Morgante Book 2017 Springer International Publishing AG 2017 Da

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樓主: 游牧
21#
發(fā)表于 2025-3-25 03:41:02 | 只看該作者
22#
發(fā)表于 2025-3-25 09:57:07 | 只看該作者
23#
發(fā)表于 2025-3-25 14:41:48 | 只看該作者
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.
24#
發(fā)表于 2025-3-25 19:07:15 | 只看該作者
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.
25#
發(fā)表于 2025-3-25 21:17:18 | 只看該作者
26#
發(fā)表于 2025-3-26 01:36:45 | 只看該作者
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.
27#
發(fā)表于 2025-3-26 05:59:20 | 只看該作者
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.
28#
發(fā)表于 2025-3-26 10:53:43 | 只看該作者
The Relic Density ConstraintThe calculation of the relic abundance of DM particles in the standard freeze-out mechanism was discussed in Sect.?..
29#
發(fā)表于 2025-3-26 15:25:20 | 只看該作者
30#
發(fā)表于 2025-3-26 20:30:49 | 只看該作者
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.
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