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Auteurs principaux: Jangid, Nisha, Ray, Arnab K.
Format: Preprint
Publié: 2025
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Accès en ligne:https://arxiv.org/abs/2510.02411
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_version_ 1866912623955542016
author Jangid, Nisha
Ray, Arnab K.
author_facet Jangid, Nisha
Ray, Arnab K.
contents In a shallow-water radial outflow the horizon of a hydrodynamic white hole coincides with a standing circular hydraulic jump. The jump, caused by viscosity, makes the horizon visible as a circular front, standing as a barrier against the entry of waves within its circumference. The blocking of waves causes a pile-up at the horizon of the white hole, for which surface tension is mainly responsible. Conversely, it is also because of surface tension that the waves can penetrate the barrier. The penetrating waves (analogue Hawking quanta) tunnel through the barrier with a decaying amplitude, but a large-amplitude instability about the horizon is possible.
format Preprint
id arxiv_https___arxiv_org_abs_2510_02411
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Penetrating the horizon of a hydrodynamic white hole
Jangid, Nisha
Ray, Arnab K.
General Relativity and Quantum Cosmology
Fluid Dynamics
In a shallow-water radial outflow the horizon of a hydrodynamic white hole coincides with a standing circular hydraulic jump. The jump, caused by viscosity, makes the horizon visible as a circular front, standing as a barrier against the entry of waves within its circumference. The blocking of waves causes a pile-up at the horizon of the white hole, for which surface tension is mainly responsible. Conversely, it is also because of surface tension that the waves can penetrate the barrier. The penetrating waves (analogue Hawking quanta) tunnel through the barrier with a decaying amplitude, but a large-amplitude instability about the horizon is possible.
title Penetrating the horizon of a hydrodynamic white hole
topic General Relativity and Quantum Cosmology
Fluid Dynamics
url https://arxiv.org/abs/2510.02411