UV stability of 1-loop radiative corrections in higher-derivative scalar field theory
Yugo Abe, Takeo Inami, Keisuke Izumi

TL;DR
This paper investigates the stability of the effective potential in a higher-derivative scalar field theory at one-loop level, showing that radiative corrections ensure stability at high energies despite ghost contributions.
Contribution
It demonstrates that higher-derivative scalar theories maintain UV stability of the effective potential through one-loop corrections, including ghost effects.
Findings
The one-loop correction to the potential is positive at large field values.
Ghost contributions do not destabilize the effective potential.
Higher-derivative theories can be UV stable at quantum level.
Abstract
We consider the theory of a higher-derivative (HD) real scalar field coupled to a complex scalar , the coupling of the and being given by two types, and . We evaluate one-loop corrections to the effective potential of , both the contribution from the positive norm part of and that from the {\it negative norm part} (ghost). We show that at , where is a classical value of , is positive, implying the stability of by the HD 1-loop radiative corrections at high energy.
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Taxonomy
TopicsAtmospheric Ozone and Climate · Cosmology and Gravitation Theories · Gas Dynamics and Kinetic Theory
