796,237 research outputs found
On Newman-Penrose constants of stationary electrovacuum spacetimes
A theorem related to the Newman-Penrose constants is proven. The theorem
states that all the Newman-Penrose constants of asymptotically flat,
stationary, asymptotically algebraically special electrovacuum spacetimes are
zero. Straightforward application of this theorem shows that all the
Newman-Penrose constants of the Kerr-Newman spacetime must vanish.Comment: 11pages, no figures accepted by PR
An explanation of the Newman-Janis Algorithm
After the original discovery of the Kerr metric, Newman and Janis showed that
this solution could be ``derived'' by making an elementary complex
transformation to the Schwarzschild solution. The same method was then used to
obtain a new stationary axisymmetric solution to Einstein's field equations now
known as the Kerr-newman metric, representing a rotating massive charged black
hole. However no clear reason has ever been given as to why the Newman-Janis
algorithm works, many physicist considering it to be an ad hoc procedure or
``fluke'' and not worthy of further investigation. Contrary to this belief this
paper shows why the Newman-Janis algorithm is successful in obtaining the
Kerr-Newman metric by removing some of the ambiguities present in the original
derivation. Finally we show that the only perfect fluid generated by the
Newman-Janis algorithm is the (vacuum) Kerr metric and that the only Petrov
typed D solution to the Einstein-Maxwell equations is the Kerr-Newman metric.Comment: 14 pages, no figures, submitted to Class. Quantum Gra
Accretion of New Variable Modified Chaplygin Gas and Generalized Cosmic Chaplygin Gas onto Schwarzschild and Kerr-Newman Black holes
In this work, we have studied accretion of the dark energies NVMCG and GCCG
onto the Schwarzschild and Kerr-Newman Black holes. We find the expression of
the critical four velocity component which gradually decreases for the fluid
flow towards the Schwarzschild as well as Kerr-Newman Black hole. We also find
the expression for change of masses of the black hole in both cases. For the
Kerr-Newman black hole which is rotating and charged we calculate the specific
angular momentum and total angular momentum. We showed that in both cases due
to accretion of the dark energy mass of the black hole increases and angular
momentum increases in case of Kerr-Newman black hole.Comment: 12 pages, 14 figures, Accepted for publication in European Physical
Journal
Spinning Higher Dimensional Einstein-Yang-Mills black holes
We construct a Kerr-Newman-like spacetimes starting from higher dimensional
(HD) Einstein-Yang-Mills black holes via complex transformations suggested by
Newman-Janis. The new metrics are HD generalization of Kerr-Newman spacetimes
which has a geometry precisely that of Kerr-Newman in 4D corresponding to
Yang-Mills (YM) gauge charge, but the sign of charge term gets flipped in the
HD spacetimes. It is interesting to note that gravitational contribution of YM
gauge charge, in HD, is indeed opposite (attractive rather than repulsive) that
of Maxwell charge. The effect of YM gauge charge on the structure and location
of static limit surface and apparent horizon is discussed. We find that static
limit surfaces become less prolate with increase in dimensions and are also
sensitive to YM gauge charge thereby affecting the shape of ergosphere. We also
analyze some thermodynamical properties of these BHs.Comment: Accepted for publication in EPJ
Newman and conversion
Ker, Ian T. Newman and conversion. Edinburgh: T & T Clark; Notre Dame, Ind: Univ of Notre Dame Pr, 1997
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