|
Photon sphere (''definition''〔K.S. Virbhadra and G. F.R. Ellis, Schwarzschild black hole lensing, Phys. Rev. D62, 084003 (2000); K.S. Virbhadra and G. F.R. Ellis, Gravitational lensing by naked singularities, Phys. Rev. D65, 103004 (2002).〕): A photon sphere of a static spherically symmetric metric is a timelike hypersurface if the deflection angle of a light ray with the closest distance of approach diverges as For a general static spherically symmetric metric the photon sphere equation is: The concept of a photon sphere in a static spherically metric was generalized to a photon surface of any metric. Photon surface (''definition''〔Clarissa-Marie Claudel, K.S. Virbhadra, and G.F.R. Ellis, The geometry of photon surfaces, J. Math. Phys. 42, 818-838 (2001).〕) : A photon surface of (M,g) is an immersed, nowhere spacelike hypersurface S of (M, g) such that, for every point p∈S and every null vector k∈''T''pS, there exists a null geodesic :(-ε,ε)→M of (M,g) such that (0)=k, |γ|⊂S. Both definitions give the same result for a general static spherically symmetric metric.〔See in ().〕 Theorem:〔See in ().〕 Subject to an energy condition, a black hole in any spherically symmetric spacetime must be surrounded by a photon sphere. Conversely, subject to an energy condition, any photon sphere must cover more than a certain amount of matter, a black hole, or a naked singularity. ==References== Category:General relativity 抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)』 ■ウィキペディアで「Photon surface」の詳細全文を読む スポンサード リンク
|