JOREK simulations demonstrate that increasing nitrogen seeding moves the X-point radiator upwards in ASDEX Upgrade while decreasing it moves the radiator downwards.
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Simpson-Visser regularization of Schwarzschild-AdS black holes yields a van der Waals-type temperature branch structure with three coexisting equilibria and topological charge W=+1 for regularization parameter below 1/sqrt(24), distinguishing it from the Schwarzschild-AdS case.
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JOREK simulations of the X-point radiator formation and its movement in ASDEX Upgrade
JOREK simulations demonstrate that increasing nitrogen seeding moves the X-point radiator upwards in ASDEX Upgrade while decreasing it moves the radiator downwards.
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Holographic Thermodynamic Signatures of Simpson--Visser--AdS Black Holes
Simpson-Visser regularization of Schwarzschild-AdS black holes yields a van der Waals-type temperature branch structure with three coexisting equilibria and topological charge W=+1 for regularization parameter below 1/sqrt(24), distinguishing it from the Schwarzschild-AdS case.