On the physical meaning of the NUT parameter
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Publication:995861
DOI10.1007/s10714-006-0349-3zbMath1128.83316OpenAlexW2005504194WikidataQ125019538 ScholiaQ125019538MaRDI QIDQ995861
Ahmad Al Badawi, Mustafa Halilsoy
Publication date: 10 September 2007
Published in: General Relativity and Gravitation (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/s10714-006-0349-3
Black holes (83C57) Exact solutions to problems in general relativity and gravitational theory (83C15)
Related Items (9)
On the NUT-Born-Infeld-\(\Lambda\) spacetime ⋮ Stationary, charged Zipoy-Voorhees metric from colliding wave spacetime ⋮ Thermodynamic stability and holographic heat engine efficiency of a Kerr-Newmann-NUT-Kiselev-AdS black hole in Rastall gravity ⋮ Dynamics of charged and rotating NUT black holes in Rastall gravity ⋮ Fermionic and bosonic greybody factors as well as quasinormal modes for charged Taub NUT black holes ⋮ The Dirac equation in Schwarzschild black hole coupled to a stationary electromagnetic field ⋮ CFT duals on extremal rotating NUT black holes ⋮ Kerr-Newman-NUT-Kiselev black holes in Rastall theory of gravity and Kerr/CFT correspondence ⋮ EFFECT OF NUT PARAMETER ON THE ANALYTIC EXTENSION OF THE CAUCHY HORIZON THAT DEVELOP IN COLLIDING WAVE SPACE–TIMES
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