The Geometry of Black Hole Singularities. Advances in High Energy Physics , 2014:14, May 2014. http://www.hindawi.com/journals/ahep/2014/907518/ .O. C. Stoica, The geometry of black hole singularities, Advances in High Energy Physics 14 (2014), http://www...
https://youtu.be/q6RufF4a6LM 据说重力是空间和时间的曲率,但这种曲率实际上是什么样子的呢? 在本视频中,我们探索了爱因斯坦方程的最重要解法——史瓦西解法——以构建时空流形的具体可视化。 这种可视化会让我们对更高维度的现实有新的认识吗? 引力的秘密被锁在……黑洞的几何学中。
Thermodynamic geometry of BTZ black hole.black holephase transitionstabilitythermodynamic geometryIn this paper, we considered cosmological constant as a variable and studied properties and the thermodynamics stability of BTZ black hole from a geometric perspective. Also, we examined the correspondence ...
The geometry of the spinning black holes of standard Einstein theory in 2+1 dimensions, with a negative cosmological constant and without couplings to matter, is analyzed in detail. It is shown that the black hole arises from identifications of points of anti-de Sitter space by a discrete subg...
After undergoing a finite maximal temperature, the black hole will evaporate completely at zero temperature without any remnant left. Considering a more general metric ansatz and a special equation of state of the matter, we also find a regular NCBH in Rastall gravity, which has similar ...
1,BlackHoleandGeometry,舒富文中科院上海天文台浙江大学数学科学研究中心2006.11.6,2,目录,经典黑洞黑洞的量子效应黑洞的量子结构黑洞与几何流,3,自然界中的黑洞是宇宙中最完美的宏观物体:构成它们的唯一要素是我们
Weinvestigate whether the emitted waveforms can be used to strongly constrain thegeometry of the central massive object, and in essence check that itcorresponds to a Kerr black hole (BH). For a Kerr BH, all multipole moments ofthe spacetime have a simple, unique relation to $M$ and $S$,...
Geometry of the 2+1 Black Hole The geometry of the spinning black holes of standard Einstein theory in 2+1 dimensions, with a negative cosmological constant and without couplings to matt... M Banados,M Henneaux,C Teitelboim,... - 《Phys Rev D Part Fields》 被引量: 1980发表: 1993年...
Kerr黑洞最小质量Schwarzschild黑洞面积量子广义坐标规范变换相空间四维共轭Kerr black hole has only two parameters of M and J. M and J, as the general ... Jiang JiJian,Li ChuanAn,蒋继建,... - 《物理学报》 被引量: 4发表: 2005年 黑洞时空中微扰的演化与相对论框架下的量子信息 麦克斯韦伸缩子黑...
The greatest prospect for directly ‘seeing a black hole relies upon the identification of gravitational waves from an excited black hole. The diagrams below show the gravitational signal emitted by an excited black hole. 17 小扰动 扰动的 Einstein 方程 径向角向分离 ( , , , ) g g h t r ...