找回密碼
 To register

QQ登錄

只需一步，快速開(kāi)始

掃一掃，訪問(wèn)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: 43555|回復(fù): 35
樓主
發(fā)表于 2025-3-21 16:25:54 | 只看該作者 |倒序?yàn)g覽 |閱讀模式
書(shū)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(shū)名稱SpringerBriefs in Physics
圖書(shū)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(shū)目名稱Dynamical Stabilization of the Fermi Scale影響因子(影響力)




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




書(shū)目名稱Dynamical Stabilization of the Fermi Scale網(wǎng)絡(luò)公開(kāi)度




書(shū)目名稱Dynamical Stabilization of the Fermi Scale網(wǎng)絡(luò)公開(kāi)度學(xué)科排名




書(shū)目名稱Dynamical Stabilization of the Fermi Scale被引頻次




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




書(shū)目名稱Dynamical Stabilization of the Fermi Scale年度引用




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




書(shū)目名稱Dynamical Stabilization of the Fermi Scale讀者反饋




書(shū)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(méi)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(ài)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, 2026-1-20 23:46
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
乳源| 库车县| 准格尔旗| 丹阳市| 阳信县| 苍溪县| 东辽县| 高台县| 修水县| 富川| 贵溪市| 红安县| 邯郸市| 诸城市| 樟树市| 裕民县| 扬州市| 定安县| 黑河市| 丹寨县| 北安市| 高安市| 原阳县| 卢氏县| 滨州市| 海阳市| 大英县| 望奎县| 哈尔滨市| 平湖市| 博野县| 长白| 张掖市| 西宁市| 阿尔山市| 伊春市| 凯里市| 桂阳县| 于都县| 长子县| 荔浦县|