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 in | Progress of theoretical and experimental physics Vol. 2024; no. 5 |
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Main Authors | , |
Format | Journal Article |
Language | English |
Published |
Oxford
Oxford University Press
01.05.2024
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ISSN | 2050-3911 2050-3911 |
DOI | 10.1093/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. |
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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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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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