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Autori principali: Yu, Peng, Zhong, Yuan, Wang, Ziqi, Wang, Hui, Zhang, Mengyang
Natura: Preprint
Pubblicazione: 2025
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Accesso online:https://arxiv.org/abs/2505.16108
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author Yu, Peng
Zhong, Yuan
Wang, Ziqi
Wang, Hui
Zhang, Mengyang
author_facet Yu, Peng
Zhong, Yuan
Wang, Ziqi
Wang, Hui
Zhang, Mengyang
contents In this work, we present two brane-world-type solutions in a two-dimensional (2D) dilaton gravity model with singular space-time backgrounds. By employing a first-order superpotential formalism, we first construct the 2D analogues of the thick brane solution previously given by Gremm and analyze the corresponding linear scalar perturbations. We show that for a model with canonical scalar matter fields, the effective potential of the linear perturbation equation is a singular Pöschl--Teller~II type, which does not admit bound states. However, for a model with non-canonical scalar fields, the effective potential becomes an exactly solvable Pöschl--Teller~I potential, which has an infinite tower of normalizable bound states. We also present a second analytic solution inspired by the work of Girardello \emph{et al.}, but with non-canonical scalar field. In this case, the linear perturbation equation is a Schrödinger equation with the Eckart potential, which is also exactly solvable.
format Preprint
id arxiv_https___arxiv_org_abs_2505_16108
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Shape-invariant Potentials and Singular Spaces
Yu, Peng
Zhong, Yuan
Wang, Ziqi
Wang, Hui
Zhang, Mengyang
High Energy Physics - Theory
General Relativity and Quantum Cosmology
In this work, we present two brane-world-type solutions in a two-dimensional (2D) dilaton gravity model with singular space-time backgrounds. By employing a first-order superpotential formalism, we first construct the 2D analogues of the thick brane solution previously given by Gremm and analyze the corresponding linear scalar perturbations. We show that for a model with canonical scalar matter fields, the effective potential of the linear perturbation equation is a singular Pöschl--Teller~II type, which does not admit bound states. However, for a model with non-canonical scalar fields, the effective potential becomes an exactly solvable Pöschl--Teller~I potential, which has an infinite tower of normalizable bound states. We also present a second analytic solution inspired by the work of Girardello \emph{et al.}, but with non-canonical scalar field. In this case, the linear perturbation equation is a Schrödinger equation with the Eckart potential, which is also exactly solvable.
title Shape-invariant Potentials and Singular Spaces
topic High Energy Physics - Theory
General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2505.16108