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: Dynamical Stabilization of the Fermi Scale; Towards a Composite Francesco Sannino Book 2013 The Author(s) 2013 Composite Higgs.Dynamical S

[復(fù)制鏈接]
查看: 43559|回復(fù): 35
樓主
發(fā)表于 2025-3-21 16:25:54 | 只看該作者 |倒序瀏覽 |閱讀模式
書目名稱Dynamical Stabilization of the Fermi Scale
副標(biāo)題Towards a Composite
編輯Francesco Sannino
視頻videohttp://file.papertrans.cn/284/283847/283847.mp4
概述Includes supplementary material:
叢書名稱SpringerBriefs in Physics
圖書封面Titlebook: Dynamical Stabilization of the Fermi Scale; Towards a Composite  Francesco Sannino Book 2013 The Author(s) 2013 Composite Higgs.Dynamical S
描述.Strong dynamics constitutes one of the pillars of the standard model of particle interactions, and it accounts for the bulk of the visible matter in the universe made by ordinary protons and neutrons. It is therefore a well posed question to ask if the rest of the universe can be described in terms of new highly natural four-dimensional strongly coupled theories. The main goal of this lecture-based primer is to provide a coherent overview of how new strong dynamics can be employed to address the relevant challenges in particle physics and cosmology from composite Higgs dynamics to dark matter and inflation. We will first introduce the topic of dynamical breaking of the electroweak symmetry also known as technicolor. The knowledge of the phase diagram of strongly coupled theories plays a fundamental role when trying to construct viable extensions of the standard model. Therefore we present the state-of-the-art of the phase diagram for gauge theories as function of the number of colors, flavors, matter representation and gauge group. Recent extensions of the standard model featuring minimal technicolor theories are then introduced as relevant examples. We finally show how technicolo
出版日期Book 2013
關(guān)鍵詞Composite Higgs; Dynamical Symmetry Breaking; Electroweak Interactions; Fermi Scale; Minimal Walking Tec
版次1
doihttps://doi.org/10.1007/978-3-642-33341-5
isbn_softcover978-3-642-33340-8
isbn_ebook978-3-642-33341-5Series ISSN 2191-5423 Series E-ISSN 2191-5431
issn_series 2191-5423
copyrightThe Author(s) 2013
The information of publication is updating

書目名稱Dynamical Stabilization of the Fermi Scale影響因子(影響力)




書目名稱Dynamical Stabilization of the Fermi Scale影響因子(影響力)學(xué)科排名




書目名稱Dynamical Stabilization of the Fermi Scale網(wǎng)絡(luò)公開度




書目名稱Dynamical Stabilization of the Fermi Scale網(wǎng)絡(luò)公開度學(xué)科排名




書目名稱Dynamical Stabilization of the Fermi Scale被引頻次




書目名稱Dynamical Stabilization of the Fermi Scale被引頻次學(xué)科排名




書目名稱Dynamical Stabilization of the Fermi Scale年度引用




書目名稱Dynamical Stabilization of the Fermi Scale年度引用學(xué)科排名




書目名稱Dynamical Stabilization of the Fermi Scale讀者反饋




書目名稱Dynamical Stabilization of the Fermi Scale讀者反饋學(xué)科排名




單選投票, 共有 0 人參與投票
 

0票 0%

Perfect with Aesthetics

 

0票 0%

Better Implies Difficulty

 

0票 0%

Good and Satisfactory

 

0票 0%

Adverse Performance

 

0票 0%

Disdainful Garbage

您所在的用戶組沒有投票權(quán)限
沙發(fā)
發(fā)表于 2025-3-21 22:06:51 | 只看該作者
板凳
發(fā)表于 2025-3-22 04:16:28 | 只看該作者
,Aquae aromaticae — aromatische W?sser,The dark side holds the 96?% share of the Universe. Given that to describe the remaining 4?% we need at least three forces it is very likely that the dark side of the Universe hides many new forces. We will suggest few possibilities yielding candidates for composite dark matter and inflation making use of new strong dynamics.
地板
發(fā)表于 2025-3-22 05:59:23 | 只看該作者
Minimal Technicolor Models: Toccata and Fugue,In the prelude we introduced the basic concepts about technicolor and argued for the need of new strongly coupled dynamics. In the previous interlude section we argued for the existence of such a new type of dynamics. Here we construct a few explicit model examples. The associated LHC phenomenology is reported in the . report [.].
5#
發(fā)表于 2025-3-22 12:37:10 | 只看該作者
Composite Dark Matters: Coda,The dark side holds the 96?% share of the Universe. Given that to describe the remaining 4?% we need at least three forces it is very likely that the dark side of the Universe hides many new forces. We will suggest few possibilities yielding candidates for composite dark matter and inflation making use of new strong dynamics.
6#
發(fā)表于 2025-3-22 14:34:21 | 只看該作者
https://doi.org/10.1007/978-3-642-33341-5Composite Higgs; Dynamical Symmetry Breaking; Electroweak Interactions; Fermi Scale; Minimal Walking Tec
7#
發(fā)表于 2025-3-22 20:54:12 | 只看該作者
Francesco SanninoIncludes supplementary material:
8#
發(fā)表于 2025-3-22 21:15:48 | 只看該作者
SpringerBriefs in Physicshttp://image.papertrans.cn/e/image/283847.jpg
9#
發(fā)表于 2025-3-23 02:29:04 | 只看該作者
10#
發(fā)表于 2025-3-23 06:32:03 | 只看該作者
,Aquae aromaticae — aromatische W?sser,l extensions of the standard model. These are also among the most challenging models to work with since they require deep knowledge of gauge dynamics in a regime where perturbation theory fails. In particular, it is of utmost importance to gain information on the nonperturbative dynamics of non-abel
 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 期刊點評 投稿經(jīng)驗總結(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| 派博傳思國際 ( 京公網(wǎng)安備110108008328) GMT+8, 2026-1-21 04:39
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
绥化市| 麦盖提县| 隆尧县| 宿迁市| 商城县| 通河县| 绍兴市| 且末县| 河曲县| 绥德县| 思南县| 门源| 梨树县| 紫金县| 龙海市| 玉树县| 贵阳市| 苗栗市| 巴彦淖尔市| 南京市| 卫辉市| 新津县| 库车县| 涞水县| 乾安县| 南陵县| 湘乡市| 华容县| 吉首市| 迁西县| 鹿泉市| 潜山县| 茂名市| 丹巴县| 高邑县| 贵州省| 石首市| 龙山县| 珲春市| 龙岩市| 深州市|