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Oscillating instantons as homogeneous tunneling channels
High Energy Physics - Theory · Submitted 29 Jun 2012
abstract compiled · 2026-09-23 · no language-model review
The authors' main claim Thus, for a general vacuum decay problem, we should not ignore the oscillating instanton channels.
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The abstract, sentence by sentence
In this paper, we study Einstein gravity with a minimally coupled scalar field accompanied with a potential, assuming an O(4) symmetric metric ansatz. We call an Euclidean instanton is to be an oscillating instanton, if there exists a point where the derivative of the scale factor and the scalar field vanish at the same time. Then we can prove that the oscillating instanton can be analytically continued, both as inhomogeneous and homogeneous tunneling channels. Here, we especially focus on the possibility of a homogeneous tunneling channel. For the existence of such an instanton, we have to assume three things: (1) there should be a local maximum and the curvature of the maximum should be sufficiently large, (2) there should be a local minimum and (3) the other side of the potential should have a sufficiently deeper vacuum. Then, we can show that there exists a number of oscillating instanton solutions and their probabilities are higher compared to the Hawking-Moss instantons. We also check the possibility when the oscillating instantons are comparable with the Coleman-DeLuccia channels. Thus, for a general vacuum decay problem, we should not ignore the oscillating instanton channels.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | In this paper, we study Einstein gravity with a minimally coupled scalar field accompanied with a potential, assuming an O(4) symmetric metric ansatz. | contribution 0.54 | 0.70 | 0.02 | asserted 0.81 |
| s1 | We call an Euclidean instanton is to be an oscillating instanton, if there exists a point where the derivative of the scale factor and the scalar field vanish at the same time. | method 0.47 | 0.48 | 0.03 | asserted 1.00 |
| s2 | Then we can prove that the oscillating instanton can be analytically continued, both as inhomogeneous and homogeneous tunneling channels. | result 0.95 | 0.91 | 0.28 | asserted 1.00 |
| s3 | Here, we especially focus on the possibility of a homogeneous tunneling channel. | contribution 0.89 | 0.78 | 0.04 | asserted 0.67 |
| s4 | For the existence of such an instanton, we have to assume three things: (1) there should be a local maximum and the curvature of the maximum should be sufficiently large, (2) there should be a local minimum and (3) the other side of the potential should have a sufficiently deeper vacuum. | method 0.68 | 0.48 | 0.05 | asserted 0.93 |
| s5 | Then, we can show that there exists a number of oscillating instanton solutions and their probabilities are higher compared to the Hawking-Moss instantons. | result 1.00 | 0.93 | 0.21 | asserted 1.00 |
| s6 | We also check the possibility when the oscillating instantons are comparable with the Coleman-DeLuccia channels. | contribution 0.81 | 0.86 | 0.04 | hedged possibility 0.81 |
| s7 | Thus, for a general vacuum decay problem, we should not ignore the oscillating instanton channels. | interpretation 0.98 | 0.50 | 0.83 | asserted 0.79 |
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The paper
Original abstract
In this paper, we study Einstein gravity with a minimally coupled scalar field accompanied with a potential, assuming an O(4) symmetric metric ansatz. We call an Euclidean instanton is to be an oscillating instanton, if there exists a point where the derivative of the scale factor and the scalar field vanish at the same time. Then we can prove that the oscillating instanton can be analytically continued, both as inhomogeneous and homogeneous tunneling channels. Here, we especially focus on the possibility of a homogeneous tunneling channel. For the existence of such an instanton, we have to assume three things: (1) there should be a local maximum and the curvature of the maximum should be sufficiently large, (2) there should be a local minimum and (3) the other side of the potential should have a sufficiently deeper vacuum. Then, we can show that there exists a number of oscillating instanton solutions and their probabilities are higher compared to the Hawking-Moss instantons. We also check the possibility when the oscillating instantons are comparable with the Coleman-DeLuccia channels. Thus, for a general vacuum decay problem, we should not ignore the oscillating instanton channels.
Human review
How the literature uses it
12 arXiv papers cite this in 13 sentences
Papers citing it · 10 sentences without a confident label
Uses its method or tool 1 paper
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What we will use is the analytic continuation of $χ= π/2 + iT$ as is usual with inhomogeneous instantons [ref] .
Fuzzy Euclidean wormholes in anti-de Sitter space · Conceptual picture · 0.83
Cites it as background 2 papers
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Despite significant progress, the prescription for evaluating the pre-exponential factor $A$ in the transition probability amplitude remains a topic of debate, particularly concerning the existence and implications of single or multiple negative modes [ref] .
Nucleation of de Sitter from the anti de Sitter spacetime in scalar field models · Vacuum transition processes in presence of gravity · 0.91
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The oscillating instantons as homogeneous tunneling channels have been also studied [ref] .
Fubini instantons in curved space · Summary and Discussions · 0.93
What it cites · 30 sentences without a confident label
Uses the method or tool of 4 papers
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We use the steepest-descent method and consider only the on-shell solutions to count the probability from the path-integral [ref] .
The No-Boundary Measure of the Universe · Hawking-Moss instantons · 0.85
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We use the steepest-descent method and consider only the on-shell solutions to count the probability from the path-integral [ref] .
The Classical Universes of the No-Boundary Quantum State · Hawking-Moss instantons · 0.85
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We use the steepest-descent method and consider only the on-shell solutions to count the probability from the path-integral [ref] .
The no-boundary measure in scalar-tensor gravity · Hawking-Moss instantons · 0.85
Compares with 1 paper
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In this paper, we will call our new instanton solutions as the oscillating instantons (contrast to oscillating bounces [ref] , where these are not homogeneous in general).
Thermal derivation of the Coleman-De Luccia tunneling prescription · Introduction · 0.96
Cites as background 6 papers
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This type of solution has already been investigated in the literature [ref] .
Thermal derivation of the Coleman-De Luccia tunneling prescription · Introduction · 0.87
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The former case has already been applied and studied in depth as a bounce solution [ref] .
Oscillating instanton solutions in curved space · Motivation for this paper · 0.84
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Fourth, in string cosmology, there exist some phenomenological models with flux compactification [ref] .
de Sitter Vacua in String Theory · Introduction · 0.87
Discussion
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