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20062026
most citedTraversable Wormholes Supported by GUP Corrected Casimir Energy

121 citations · 1.1k across the 97 of their papers we have counts for

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gr-qc2026

Higher-order generalized uncertainty principle corrections to Casimir-supported traversable wormholes

Jureeporn Yuennan, Allah Ditta, Thammarong Eadkhong +2

We investigate traversable wormholes supported by Casimir vacuum energy with second-order generalized uncertainty principle (GUP) corrections. For two representative GUP models, we…

gr-qc2026

Yukawa modification of Traversable Wormholes supported by Holographic Dark Energy

Remo Garattini, Phongpichit Channuie, Kirill Zatrimaylov

Inspired by holographic dark energy models, we extend the analysis performed in Ref.\cite{RGPC} taking into account Yukawa deformations on the different energy density (HDE) profil…

gr-qc2026

Removability criterion for radiative corrections to the Starobinsky attractor in weakly nonlocal gravity

Ekapob Kulchoakrungsun, Phongpichit Channuie, Daris Samart

Radiative corrections at the percent level can shift the predictions of -attractor and Starobinsky-like models into the region of the plane preferred by ACT DR6. We sh…

gr-qc2026

Probing scalarized wormholes through quasi-periodic oscillations and spinning particle dynamics

Asalkhon Alimova, Akbar Davlataliev, Farruh Atamurotov +3

We investigate the dynamics of test particles in a three-parameter scalarized wormhole spacetime within Einstein-scalar field theory. For spinless particles, we derive the orbital…

gr-qc2026

Noncommutative black holes: Topological bulk-boundary correspondence and Binary Merger Bounds

Ankit Anand, Anshul Mishra, Aditya Singh +3

We investigate the thermodynamic topology of charged AdS black holes in a non-commutative spacetime sourced by Lorentzian-smeared matter distributions. Since exact analytical solut…

gr-qc2026

Transient Dynamical Wormholes with Decaying Radial Energy Flux

Allah Ditta, Phongpichit Channuie

We investigate a class of time-dependent traversable wormholes within the framework of general relativity by allowing the shape function to vary with time. In this setting, the evo…