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Auteurs principaux: Lozande, M. A., Fajardo, E. A.
Format: Preprint
Publié: 2026
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Accès en ligne:https://arxiv.org/abs/2604.16927
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author Lozande, M. A.
Fajardo, E. A.
author_facet Lozande, M. A.
Fajardo, E. A.
contents We explore the realization of distinct analog black hole horizons within tilted Weyl semimetals by comparing two models with contrasting spectral properties. We demonstrate that a spatially varying tilt in the Weyl cone structure creates an effect analogous to the tilting of light cones near a gravitational black hole horizon. By analyzing wave packet dynamics in both models, we reveal two fundamentally different types of analog horizons. The first model exhibits complete wave packet reflection, effectively mimicking an impenetrable barrier. In contrast, the second model permits wave packet transmission across the horizon. Critically, for both models, wave packets initialized with zero momentum ($k_0=0.0$) experience the strongest horizon effects, characterized by a dramatic slowing and significantly longer dwell times at the horizon region. Finally, we find that both systems exhibit substantial probability loss, which we demonstrate is directly correlated with the wave packet's dwell time near the horizon. Our findings establish tilted Weyl semimetals as a rich, tunable platform for investigating non-trivial quantum effects and information dynamics associated with analog black hole horizons.
format Preprint
id arxiv_https___arxiv_org_abs_2604_16927
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle Wave Packet Propagation in Tilted Weyl Semimetals for Black Hole Analog Systems
Lozande, M. A.
Fajardo, E. A.
Mesoscale and Nanoscale Physics
General Relativity and Quantum Cosmology
We explore the realization of distinct analog black hole horizons within tilted Weyl semimetals by comparing two models with contrasting spectral properties. We demonstrate that a spatially varying tilt in the Weyl cone structure creates an effect analogous to the tilting of light cones near a gravitational black hole horizon. By analyzing wave packet dynamics in both models, we reveal two fundamentally different types of analog horizons. The first model exhibits complete wave packet reflection, effectively mimicking an impenetrable barrier. In contrast, the second model permits wave packet transmission across the horizon. Critically, for both models, wave packets initialized with zero momentum ($k_0=0.0$) experience the strongest horizon effects, characterized by a dramatic slowing and significantly longer dwell times at the horizon region. Finally, we find that both systems exhibit substantial probability loss, which we demonstrate is directly correlated with the wave packet's dwell time near the horizon. Our findings establish tilted Weyl semimetals as a rich, tunable platform for investigating non-trivial quantum effects and information dynamics associated with analog black hole horizons.
title Wave Packet Propagation in Tilted Weyl Semimetals for Black Hole Analog Systems
topic Mesoscale and Nanoscale Physics
General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2604.16927