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Иш: How do rotating black holes form in higher dimensions?
Self-force as a cosmic censor in the Kerr overspinning problem
M. Colleoni, Leor Barack, Abhay Shah +1
Мақола201512 иқтибосABIThe Lovelock gravity in the critical spacetime dimension
Naresh Dadhich, Sushant G. Ghosh, Sanjay Jhingan
Мақола201211 иқтибосABIBound orbits and gravitational theory
Naresh Dadhich, Sushant G. Ghosh, Sanjay Jhingan
Мақола20135 иқтибосABIOn the static Lovelock black holes
Naresh Dadhich, Josep M. Pons, Kartik Prabhu
Мақола20134 иқтибосABIPure Lovelock black holes in dimensions <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>d</mml:mi><mml:mo>=</mml:mo><mml:mn>3</mml:mn><mml:mi>N</mml:mi><mml:mo>+</mml:mo><mml:mn>1</mml:mn></mml:math> are stable
Radouane Gannouji, Yolbeiker Rodríguez Baez, Naresh Dadhich
Мақола20194 иқтибосABI