找回密码
 To register

QQ登录

只需一步,快速开始

扫一扫,访问微社区

Titlebook: Einstein Equations: Local Energy, Self-Force, and Fields in General Relativity; Domoschool 2019 Sergio Luigi Cacciatori,Alexander Kamenshch

[复制链接]
楼主: Jaundice
发表于 2025-3-26 22:57:07 | 显示全部楼层
发表于 2025-3-27 04:08:29 | 显示全部楼层
发表于 2025-3-27 06:25:49 | 显示全部楼层
On Some Mathematical Rules from the g a geometric problem of isometric embedding a surface into the Minkowski spacetime. Then, we review the formula of surface Hamiltonian and its properties. In the explanation of the definition of the Wang–Yau energy, we focus on its physical and variational feature and relate it to some previously k
发表于 2025-3-27 10:16:57 | 显示全部楼层
https://doi.org/10.1007/978-3-642-79589-3school.” The most important application of gravitational self-force concerns metric and curvature perturbations in black hole spacetimes due to moving particles or evolving fields. However, from a practical point of view (and for teaching purposes) we have chosen to perform the whole discussion at t
发表于 2025-3-27 16:44:56 | 显示全部楼层
发表于 2025-3-27 18:10:00 | 显示全部楼层
Modell des untersuchten Antriebssystems,valence Principle. The general motivations will be presented, also recalling the role of the violation of such symmetries during the early evolution of the Universe. Antimatter systems in the form of bound neutral states will be considered, because of the possibility of studying gravitational intera
发表于 2025-3-28 00:34:41 | 显示全部楼层
https://doi.org/10.1007/978-3-7091-2332-4g an evaporating metric in the quasi-static approximation in which departures from the standard Schwarzschild metric are governed by a small luminosity factor. The backreaction leads to an ergosphere-like region which naturally tames the usual divergence in the calculation of the partition function
发表于 2025-3-28 05:01:14 | 显示全部楼层
Gebiss-, Kiefer- und Gesichtsorthopädiehole), firstly introduced by Bronnikov as a solution to Einstein’s equations in presence of a self-interacting phantom scalar field. In this chapter, we construct an embedding diagram for this spacetime and study the structure of its timelike and null geodesics. In the limit case in which the asympt
发表于 2025-3-28 07:45:04 | 显示全部楼层
14 Open beten en non-occlusies, has been proposed a new model, which upgrades the two-dimensional (2D) description in the three-dimensional (3D) case in Kerr spacetime. The radiation field is considered as constituted by photons emitted from a rigidly rotating spherical source around the compact object. Such dynamical system admi
发表于 2025-3-28 12:39:34 | 显示全部楼层
Frances McGinnity,Antje Mertens of spacetime and its matter/energy content. A severe complication is that, with the exception of a few idealised cases characterised by high degrees of symmetry, the EFEs simply cannot be obtained analytically; we need a computer to get the job done. That being said, computers (for better or worse)
 关于派博传思  派博传思旗下网站  友情链接
派博传思介绍 公司地理位置 论文服务流程 影响因子官网 SITEMAP 大讲堂 北京大学 Oxford Uni. Harvard Uni.
发展历史沿革 期刊点评 投稿经验总结 SCIENCEGARD IMPACTFACTOR 派博系数 清华大学 Yale Uni. Stanford Uni.
|Archiver|手机版|小黑屋| 派博传思国际 ( 京公网安备110108008328) GMT+8, 2025-5-12 11:48
Copyright © 2001-2015 派博传思   京公网安备110108008328 版权所有 All rights reserved
快速回复 返回顶部 返回列表