Quantum Effective Dynamics and Stability of Vacuum in Anti-de Sitter Spacetimes

Fuente: arXiv
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Autores principales: Li, Shi-Yuan, Liu, Chengwu
Formato: Preprint
Publicado: 2026
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author Li, Shi-Yuan
Liu, Chengwu
author_facet Li, Shi-Yuan
Liu, Chengwu
contents We investigate the details of the canonical quantization of effective quantum field theories in anti-de Sitter spacetime, emphasizing the stability of the quantum vacuum. We take the scalar and Maxwell fields as examples. For the non-minimally coupled massless real scalar field with ξRϕ^2 term in the Lagrangian (mass can be introduced by shift of ξ), only when ξ\le 5/48, the quantized Hamiltonian is spontaneously non-negative and the vacuum is well defined. For ξ> 5/48, one has to assign the negative energy spectrum as that of the ghost particles, introducing anti-commutation relations to make the corresponding part of the Hamiltonian trivial, ensuring the Hamiltonian non-negative and the vacuum (and the Hilbert space) well defined. This method of ghost states is applicable once the proper radial boundary conditions guarantee the Hamiltonian self-adjoint. The resulting dynamics can be compared with those resulting from the positive self-adjoint extensions when the latter is available for ξ\le 9/48. For the Maxwell fields, the gauge invariant canonical energy momentum tensor straightforwardly leads to the gauge invariant non-negative Hamiltonian (well-defined vacuum). Hence the redundant gauge degree of freedom is irrelevant, and the 2-dimensional dynamical degrees of freedom are quantized in a concrete, e.g., temporal gauge. The energy momentum tensors for both quantized fields are renormalized to be finite at operator level, which renders the stable vacuum maximally symmetric. The back-reactions to the background spacetime by excited states via the semi-classical Einstein equations are also discussed.
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id arxiv_https___arxiv_org_abs_2602_06583
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle Quantum Effective Dynamics and Stability of Vacuum in Anti-de Sitter Spacetimes
Li, Shi-Yuan
Liu, Chengwu
General Relativity and Quantum Cosmology
High Energy Physics - Phenomenology
High Energy Physics - Theory
We investigate the details of the canonical quantization of effective quantum field theories in anti-de Sitter spacetime, emphasizing the stability of the quantum vacuum. We take the scalar and Maxwell fields as examples. For the non-minimally coupled massless real scalar field with ξRϕ^2 term in the Lagrangian (mass can be introduced by shift of ξ), only when ξ\le 5/48, the quantized Hamiltonian is spontaneously non-negative and the vacuum is well defined. For ξ> 5/48, one has to assign the negative energy spectrum as that of the ghost particles, introducing anti-commutation relations to make the corresponding part of the Hamiltonian trivial, ensuring the Hamiltonian non-negative and the vacuum (and the Hilbert space) well defined. This method of ghost states is applicable once the proper radial boundary conditions guarantee the Hamiltonian self-adjoint. The resulting dynamics can be compared with those resulting from the positive self-adjoint extensions when the latter is available for ξ\le 9/48. For the Maxwell fields, the gauge invariant canonical energy momentum tensor straightforwardly leads to the gauge invariant non-negative Hamiltonian (well-defined vacuum). Hence the redundant gauge degree of freedom is irrelevant, and the 2-dimensional dynamical degrees of freedom are quantized in a concrete, e.g., temporal gauge. The energy momentum tensors for both quantized fields are renormalized to be finite at operator level, which renders the stable vacuum maximally symmetric. The back-reactions to the background spacetime by excited states via the semi-classical Einstein equations are also discussed.
title Quantum Effective Dynamics and Stability of Vacuum in Anti-de Sitter Spacetimes
topic General Relativity and Quantum Cosmology
High Energy Physics - Phenomenology
High Energy Physics - Theory
url https://arxiv.org/abs/2602.06583