Kerr-newman Metric

The Kerr-Newman metric is a solution of Einstein's field equations that describes the spacetime geometry around a charged (Q\neq0), rotating (J\neq0) black hole of mass m. The Kerr-Newman metric is: ds^{2}=-\frac{\Delta}{\rho^{2}}\left(dt-a\sin^{2}\theta d\phi\right)^{2}+\frac{\sin^{2}\theta}{\rho^{2}}\left\left(r^{2}+a^{2}\right)d\phi-adt\right^{2} +\frac{\rho^{2}}{\Delta}dr^{2}+\rho^{2}d\theta^{2} \rho^{2}\equiv r^{2}+a^{2}\cos^{2}\theta a\equiv\frac{J}{m}

Source(s)

 

<< PreviousWord BrowserNext >>
crozet
kamen rider knight
robert east
jeffrey lundgren
forum of young global leaders
franchi
list of young global leaders
delta ii class submarine
ferdinand gotthelf hand
kyle reese
national nine news
iota subscript
sako
eighth avenue (bmt canarsie line station)
alfred wetzler
jamie wingo
hollow flame
bishop of croydon
b cas
helen greiner
ted willis
multi facial
wilfred wood (bishop)
uberti
nina wadia
solon (disambiguation)
jon blair
streamlinenet
murder mile
chungang university
pp wave metrics
rick strassman
jingo
plane gravitational waves
gatekeeper butterfly
victor ludorum
anne frank remembered
chemical coast
leo ford (actor)
polish codepages
ra'ad
west pennant hills, new south wales
mayumi yamamoto
hankyoreh shinmun
Copyright 2005-2009 OnPedia.com. All Rights Reserved