Kerr black holegravitational wave memoryKerr-Schild metricThe Minkowski background intrinsic to the Kerr-Schild version of the Kerr metric provides a definition of a boosted spinning black hole. There are two Kerr-Schild versions corresponding to ingoing or outgoing principal null directions. The two...
克尔黑洞(Kerr black hole)是爱因斯坦场方程预言下的一类带有角动量的黑洞,是两种旋转黑洞(rotating black hole)中的一种。 用来描述克尔黑洞的时空度规叫做克尔度规,是由新西兰数学家Roy Kerr于1963年解出的。另一种是同时带有角动量和电荷的黑洞,叫做克尔-纽曼黑洞(Kerr-Newman black hole)。 相比于静态的史瓦西...
For vanishing NUT parameter, the metric describes a Kerr–Newman black hole. For nonvanishing NUT parameter, there are two string singularities corresponding to the two Misner strings. Besides the string singularities and horizon, there is a spacetime singularity for \( n\le a .\) For \( n\...
Kerr Lake State Recreation Area Kerr Lens Modelocking Kerr Machine Shop Group Inc. Kerr magnetooptical effect Kerr McGee Corp Kerr metric Kerr Newman Black Hole Kerr solution Kerr Walter Francis Kerr, Archibald John Kerr Clark Kerr, Clark Kerr, Harry Hyland Kerr, Jean Collins Kerr, John ▼Comple...
Define Kerr. Kerr synonyms, Kerr pronunciation, Kerr translation, English dictionary definition of Kerr. Walter Francis 1913-1996. American playwright, writer, and drama critic for the New York Herald Tribune and the New York Times . In 1978 he won a Pul
We study black hole thermodynamics of the non-extremal Kerr metric via the introduction of a new Kerr-like AdS2xS2 vacuum solution within an AdS2/CFT1 correspondence. This new Kerr-like black hole exhibits several unique useful properties and maps into the extremal Kerr throat, first introduced...
In this short contribution we carried out an analytical electrodynamical study of the magnetized Kerr-Newman metric. This study is limited to a spacetime region in which the dimensional parameter尾 (= MB << 1), whereMandB, are the black hole mass, and the asymptotical external magnetic field...
When the Cauchy and event horizons coincide, one can obtain an extremal black hole. When the cosmological and event horizon coincide, the resulting metric will be Nariai solution. Furthermore, when all three horizons coincide, the ultracold solution will be produced. The first holographic ...
III. SPACE-TIME FEATURES OF KERR BLACK HOLES In 1963, Roy Kerr solved the Einstein equations for a black hole with the presence of angular momentum. Kerr’s solution for a rotating black hole is called the Kerr metric (Visser, 2008): where a=J/m (the angular momentum to mass ratio)...
Introducing the notion of the local thermal equilibrium,the Hawking effect and the entropy of a nonstationary Kerr Newman black hole whose metric changes slowly are studied by the method of Damour Ruffini and the thin film model.First,we obtain the Hawking radiation temperature and the thermal ...