Exact 5D rotating Lifshitz black holes with electric and axionic charges were found and used to show that rotation weakens holographic superconductivity while higher z enhances it.
Title resolution pending
5 Pith papers cite this work. Polarity classification is still indexing.
5
Pith papers citing it
representative citing papers
Lorentzian-Euclidean black holes produce excess inner-shadow intensity and accumulate energy at the horizon with backreaction unlike stable light rings.
Explicit one-loop computation shows the constraint effective potential for scalars in de Sitter is free of infrared problems and supports its use in stochastic Starobinsky-Yokoyama inflation.
Weylian boundary terms generate geometric dark energy whose Friedmann equations match observations when a Barboza-Alcaniz equation of state is imposed.
Holographic duality equates cosmological constant acceleration with de Sitter horizon thermodynamics, extending to time-dependent GREA entropic acceleration when matter is present.
citing papers explorer
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Shadow signatures and energy accumulation in Lorentzian-Euclidean black holes
Lorentzian-Euclidean black holes produce excess inner-shadow intensity and accumulate energy at the horizon with backreaction unlike stable light rings.
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Dark energy and accelerating cosmological evolution in a Universe with a Weylian boundary
Weylian boundary terms generate geometric dark energy whose Friedmann equations match observations when a Barboza-Alcaniz equation of state is imposed.
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GREA and Dark Energy: A holographic correspondence
Holographic duality equates cosmological constant acceleration with de Sitter horizon thermodynamics, extending to time-dependent GREA entropic acceleration when matter is present.