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 Systems and Cosmology; A. A. Coley Book 2003 Springer Science+Business Media Dordrecht 2003 Cosmology.EFE.Gravity.Potential.Rela

[復制鏈接]
樓主: 無限
21#
發(fā)表于 2025-3-25 03:55:37 | 只看該作者
Trendüberwachung über Lebensdaueroduli space of a more fundamental, non-perturbative theory known as M-theory [376], and so no particular string theory is necessarily more fundamental since they are all related by duality symmetries (for a review see, e.g., Ref. [321]). Moreover, another point of this moduli space corresponds to el
22#
發(fā)表于 2025-3-25 11:32:56 | 只看該作者
23#
發(fā)表于 2025-3-25 12:37:37 | 只看該作者
,Einführung in die werteorientierte Führung, differential equations (ODE). Inhomogeneous cosmological models can also be studied, but since the evolution equations are autonomous partial differential equations (PDE) in this case the resulting state space is infinite-dimensional (i.e., a function space) , and the analysis is considerably more complicated.
24#
發(fā)表于 2025-3-25 18:17:21 | 只看該作者
Mehr Dinge zwischen Himmel und Erderedict steep exponential potentials [164] (i.e., .. > 2), effectively eliminating the possibility of power-law inflation. However, dimensionally reduced higher-dimensional theories also predict numerous scalar fields, and so it is of interest to study models with multiple scalar fields.
25#
發(fā)表于 2025-3-25 20:17:08 | 只看該作者
Introduction, differential equations (ODE). Inhomogeneous cosmological models can also be studied, but since the evolution equations are autonomous partial differential equations (PDE) in this case the resulting state space is infinite-dimensional (i.e., a function space) , and the analysis is considerably more complicated.
26#
發(fā)表于 2025-3-26 03:59:09 | 只看該作者
Multiple Scalar Fields,redict steep exponential potentials [164] (i.e., .. > 2), effectively eliminating the possibility of power-law inflation. However, dimensionally reduced higher-dimensional theories also predict numerous scalar fields, and so it is of interest to study models with multiple scalar fields.
27#
發(fā)表于 2025-3-26 06:58:42 | 只看該作者
Scalar Tensor Theories of Gravity,] and Brans and Dicke [60] and the most general scalar-tensor theories were formulated by Bergmann [40], Nordtvedt [289] and Wagoner [356] . The observational limits on scalar-tensor theories include solar system tests [2, 59, 64, 189] and cosmological tests such as Big Bang nucleosynthesis constraints [17, 322].
28#
發(fā)表于 2025-3-26 11:00:06 | 只看該作者
M-Theory, since they are all related by duality symmetries (for a review see, e.g., Ref. [321]). Moreover, another point of this moduli space corresponds to eleven-dimensional supergravity. This represents the low-energy limit of M-theory [337, 376] .
29#
發(fā)表于 2025-3-26 14:26:25 | 只看該作者
30#
發(fā)表于 2025-3-26 18:14:15 | 只看該作者
 關于派博傳思  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 論文服務流程 影響因子官網(wǎng) 吾愛論文網(wǎng) 大講堂 北京大學 Oxford Uni. Harvard Uni.
發(fā)展歷史沿革 期刊點評 投稿經(jīng)驗總結 SCIENCEGARD IMPACTFACTOR 派博系數(shù) 清華大學 Yale Uni. Stanford Uni.
QQ|Archiver|手機版|小黑屋| 派博傳思國際 ( 京公網(wǎng)安備110108008328) GMT+8, 2025-10-13 21:13
Copyright © 2001-2015 派博傳思   京公網(wǎng)安備110108008328 版權所有 All rights reserved
快速回復 返回頂部 返回列表
宁强县| 黎城县| 洛阳市| 湖南省| 平谷区| 湘西| 晋中市| 湟中县| 托克逊县| 噶尔县| 罗江县| 洪湖市| 阿拉善右旗| 河曲县| 安宁市| 长宁区| 维西| 苍南县| 于田县| 双城市| 四会市| 台南县| 信丰县| 自贡市| 博客| 进贤县| 兰考县| 民权县| 南华县| 敦煌市| 焉耆| 达孜县| 礼泉县| 景泰县| 绍兴市| 石景山区| 刚察县| 乐至县| 伊吾县| 芷江| 榕江县|