找回密碼
 To register

QQ登錄

只需一步,快速開始

掃一掃,訪問微社區(qū)

打印 上一主題 下一主題

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

[復(fù)制鏈接]
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.
 關(guān)于派博傳思  派博傳思旗下網(wǎng)站  友情鏈接
派博傳思介紹 公司地理位置 論文服務(wù)流程 影響因子官網(wǎng) 吾愛論文網(wǎng) 大講堂 北京大學(xué) Oxford Uni. Harvard Uni.
發(fā)展歷史沿革 期刊點(diǎn)評(píng) 投稿經(jīng)驗(yàn)總結(jié) SCIENCEGARD IMPACTFACTOR 派博系數(shù) 清華大學(xué) Yale Uni. Stanford Uni.
QQ|Archiver|手機(jī)版|小黑屋| 派博傳思國(guó)際 ( 京公網(wǎng)安備110108008328) GMT+8, 2025-10-10 20:35
Copyright © 2001-2015 派博傳思   京公網(wǎng)安備110108008328 版權(quán)所有 All rights reserved
快速回復(fù) 返回頂部 返回列表
大邑县| 仁化县| 寻甸| 台东县| 荔波县| 望都县| 武宣县| 昌平区| 文安县| 蓝田县| 英德市| 东乡县| 汕尾市| 通山县| 满洲里市| 收藏| 郁南县| 石渠县| 高碑店市| 苏尼特左旗| 施秉县| 金寨县| 平安县| 武夷山市| 海淀区| 乳源| 建昌县| 恩平市| 台江县| 泸定县| 威远县| 漠河县| 新建县| 廉江市| 东山县| 雷山县| 渑池县| 吴旗县| 肃南| 兴和县| 上蔡县|