Anti-Instability of Complex Ghost

We argue that Lee–Wick’s complex ghost appearing in any higher derivative theory is stable and its asymptotic field exists. It may be more appropriate to call it “anti-unstable”, in the sense that the more the ghost "decays" into lighter ordinary particles, the larger the probability that...

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Published inProgress of theoretical and experimental physics Vol. 2024; no. 5
Main Authors Kubo, Jisuke, Kugo, Taichiro
Format Journal Article
LanguageEnglish
Published Oxford Oxford University Press 01.05.2024
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ISSN2050-3911
2050-3911
DOI10.1093/ptep/ptae053

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Abstract We argue that Lee–Wick’s complex ghost appearing in any higher derivative theory is stable and its asymptotic field exists. It may be more appropriate to call it “anti-unstable”, in the sense that the more the ghost "decays" into lighter ordinary particles, the larger the probability that the ghost remains as itself becomes. This is explicitly shown by analyzing the two-point functions of the ghost Heisenberg field which is obtained as an exact result in the N → ∞ limit in a massive scalar ghost theory with light O(N)-vector scalar matter. The anti-instability is a consequence of the fact that the poles of the complex ghost propagator are located on the physical sheet in the complex plane of four-momentum squared. This should be contrasted with the case of the ordinary unstable particle, whose propagator has no pole on the physical sheet.
AbstractList We argue that Lee–Wick’s complex ghost appearing in any higher derivative theory is stable and its asymptotic field exists. It may be more appropriate to call it “anti-unstable”, in the sense that the more the ghost "decays" into lighter ordinary particles, the larger the probability that the ghost remains as itself becomes. This is explicitly shown by analyzing the two-point functions of the ghost Heisenberg field which is obtained as an exact result in the N → ∞ limit in a massive scalar ghost theory with light O(N)-vector scalar matter. The anti-instability is a consequence of the fact that the poles of the complex ghost propagator are located on the physical sheet in the complex plane of four-momentum squared. This should be contrasted with the case of the ordinary unstable particle, whose propagator has no pole on the physical sheet.
Author Kugo, Taichiro
Kubo, Jisuke
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CitedBy_id crossref_primary_10_1140_epjp_s13360_025_06009_5
crossref_primary_10_1002_prop_202400268
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Cites_doi 10.1103/PhysRevD.79.105019
10.1103/PhysRevD.5.1968
10.1016/S0031-8914(63)80277-3
10.1103/PhysRevD.96.045009
10.1103/PhysRevD.100.105006
10.1143/PTP.20.822
10.1103/PhysRevD.104.045010
10.1103/PhysRevD.2.1033
10.1016/0550-3213(69)90098-4
10.1093/ptep/ptad143
10.1143/PTP.19.607
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Copyright The Author(s) 2024. Published by Oxford University Press on behalf of the Physical Society of Japan. 2024
The Author(s) 2024. Published by Oxford University Press on behalf of the Physical Society of Japan. This work is published under https://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.
Copyright_xml – notice: The Author(s) 2024. Published by Oxford University Press on behalf of the Physical Society of Japan. 2024
– notice: The Author(s) 2024. Published by Oxford University Press on behalf of the Physical Society of Japan. This work is published under https://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.
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Physics
Title Anti-Instability of Complex Ghost
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