Slowly rotating wormholes in Rényi, mixed, and Moradpour holographic dark energy produce distinct photon orbits and shadow morphologies, with Rényi models yielding smaller asymmetric shadows.
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HDE models with future event horizon IR cutoff partially ease the Hubble tension while Hubble-scale cutoffs do not, consistent across six models and multiple BAO/SN/CMB combinations.
A new vacuum energy definition using oscillator mass scales set by IR cutoff and black hole entropy bound derives entropic dark energy models.
citing papers explorer
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Holographic dark energy as a source for slowly rotating wormholes: Implications for null geodesics and shadows
Slowly rotating wormholes in Rényi, mixed, and Moradpour holographic dark energy produce distinct photon orbits and shadow morphologies, with Rényi models yielding smaller asymmetric shadows.
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Revisiting the Hubble tension problem in the framework of holographic dark energy
HDE models with future event horizon IR cutoff partially ease the Hubble tension while Hubble-scale cutoffs do not, consistent across six models and multiple BAO/SN/CMB combinations.
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Field theory vacuum and entropic dark energy models
A new vacuum energy definition using oscillator mass scales set by IR cutoff and black hole entropy bound derives entropic dark energy models.