4.7 Article

Confinement in the tricritical Ising model

Journal

PHYSICS LETTERS B
Volume 828, Issue -, Pages -

Publisher

ELSEVIER
DOI: 10.1016/j.physletb.2022.137008

Keywords

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Funding

  1. grant Prin 2017-FISI
  2. National Research Development and Innovation Office of Hungary [132118]
  3. National Research, Development and Innovation Office (NKFIH) through the OTKA [K 138606]
  4. R/MTA Italy-Hungary

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This study investigates the effects of leading and sub-leading magnetic perturbations on the thermal E7 integrable deformation of the tricritical Ising model, revealing the confinement of excitations in different phases and analyzing the meson spectrum using semiclassical quantization with two different types of excitations.
We study the leading and sub-leading magnetic perturbations of the thermal E7 integrable deformation of the tricritical Ising model. In the low-temperature phase, these magnetic perturbations lead to the confinement of the kinks of the model. The resulting meson spectrum can be obtained using the semiclassical quantisation, here extended to include also mesonic excitations composed of two different kinks. An interesting feature of the integrable sub-leading magnetic perturbation of the thermal E7 deformation of the model is the possibility to swap the role of the two operators, i.e. the possibility to consider the model as a thermal perturbation of the integrable A(3) model associated to the sub-leading magnetic deformation. Due to the occurrence of vacuum degeneracy unrelated to spontaneous symmetry breaking in A(3), the confinement pattern shows novel features compared to previously studied models. Interestingly enough, the validity of the semi-classical description in terms of the A(3) endpoint extends well beyond small fields, and therefore the full parameter space of the joint thermal and sub-leading magnetic deformation is well described by a combination of semi-classical approaches. All predictions are verified by comparison to finite volume spectrum resulting from truncated conformal space. (C)& nbsp;2022 The Author(s). Published by Elsevier B.V.

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