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.
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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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Novel five-dimensional rotating Lifshitz black holes with electric and axionic charges
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.
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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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Scalar field effective potentials in de Sitter spacetime
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.
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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.