Cited by 6Cosmology and Gravitation TheoriesNoncommutative and Quantum Gravity TheoriesBlack Holes and Theoretical Physics

Cosmic bounce and phantom-like equation of state from tunnelling

Open access
Alexandre, Jean, Pla, Silvia·2023·Journal of High Energy Physics

Abstract

We allow a scalar field on a flat FLRW background metric to tunnel between two degenerate vacua. The resulting true vacuum state then violates the Null Energy Condition, and the corresponding homogeneous fluid induces a bounce, after which it has a phantom-like equation of state and asymptotically leads to a de Sitter phase. The mechanism presented here requires no exotic matter or modified gravity, it is purely generated by quantum fluctuations and is valid for a generic double well potential.

The claims and statistics of this paper haven’t been checked yet.

Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.

A few free checks a day · papers already verified open instantly · results are public

Integrity signals

Registry

Crossref · 10.1007/jhep05(2023)145

Cites

4 of 4 references verified0 citation errors · 0 not checkable

Statistics

Claims the paper makes

The claims and statistics of this paper haven’t been checked yet.

Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.

A few free checks a day · papers already verified open instantly · results are public

Claims other papers make about this one

Each is checked against this paper’s own text: does it say what the citing paper says it does?

  • In Refs. [13, 21], the instanton contribution to the ground state energy is calculated by only keeping homogeneous fluctuations.

    “In Refs. [13, 21], the instanton contribution to the ground state energy is calculated by only keeping homogeneous fluctuations.”

    From Double-well instantons in finite volume (2024) · cites this paper as [21]

    Section 2.2 says the calculation focuses on homogeneous saddle points, and Appendix B calculates fluctuation factors for the instanton contribution. But the paper does not say it keeps only homogeneous fluctuations: its discussion of quantum corrections describes using continuous momentum. The claim conflates a restriction on saddle points with a restriction on fluctuations. (LLM, conf=0.84)

    Experimental — accuracy not yet measured
  • Including the Casimir energy and one-loop corrections to the instanton jump should not modify the qualitative results in Ref. [21] since the NEC is still violated for any value of the comoving volume.

    “Including the Casimir energy and one-loop corrections to the instanton jump should not modify the qualitative results in Ref. [21] since the NEC is still violated for any value of the comoving volume, which means that we expect to find a bouncing solution to the Friedmann equations if we start from a contracting phase.”

    From Double-well instantons in finite volume (2024) · cites this paper as [21]

    Section 3.2 states that the ground-state fluid violates the NEC, and the Conclusions say that NEC violation produces a bounce after initial contraction. Appendix B includes fluctuations around instanton jumps. But the paper does not assess whether adding Casimir energy would leave those qualitative results unchanged; it mentions the Casimir effect only as a separate example of energy-condition violation. (LLM, conf=0.85)

    Experimental — accuracy not yet measured
  • The NEC is violated for any value of the comoving volume a3L03, and therefore a bouncing solution is obtained in FLRW independently of the initial conditions as long as H(t0) < 0.

    “It can be shown (see Ref. [21]) that the NEC is violated for any value of the comoving volume a 3 L 3 0 , and therefore a bouncing solution is obtained in FLRW independently of the initial conditions as long as H ( t 0 ) &lt; 0.”

    From Double-well instantons in finite volume (2024) · cites this paper as [21]

    Section 3.2, equation (3.11), states that the model’s ground-state fluid violates the NEC, and section 4 reports a bounce for a contracting FLRW solution. But section 4 studies numerical solutions with a fixed initial scale factor and varying parameter values; it does not establish a bounce independently of all initial conditions. Section 2.1 also assumes finite volume and adiabatic evolution, so the claim’s unqualified ‘any value’ is broader than the model’s stated scope. (LLM, conf=0.86)

    Experimental — accuracy not yet measured
  • In the simplified model analysed in Refs. [21, 22], where E_cas^(3)=0 and E_inst=E_inst^(hom), it was found L_bounce ≃ 10^-5 metres for U0=κ^-1Λ=10^-122 l_p^-4, m=10^-3 eV and λ∼1.

    “For example, in the simplified model analysed in Refs. [21, 22], where E (3) cas = 0 and E inst = E (hom) inst with E (hom) inst given in Eq. (4.31), it was found L bounce ≃ 10 -5 metres for U 0 = κ -1 Λ = 10 -122 ℓ -4 p , m = 10 -3 eV and λ ∼ 1.”

    From Double-well instantons in finite volume (2024) · cites this paper as [21]

    Section 2.1 describes a finite-volume tunnelling model that focuses on tunnelling rather than the Casimir effect. The discussion around eqs. (5.1)–(5.2) estimates the bounce volume, but our copy does not report L_bounce ≃ 10⁻⁵ metres for the stated values of U₀, m and λ. Searches for the length and numerical values did not find that result. (LLM, conf=0.84)

    Experimental — accuracy not yet measured
  • In addition to the known Casimir effect, the tunnelling effect also contributes to NEC violation, extending the results in Ref. [21].

    “In addition to the known Casimir effect, we show that the tunnelling effect also contributes to NEC violation, extending the results in Ref. [21].”

    From Double-well instantons in finite volume (2024) · cites this paper as [21]

Self-check

Percentages, sums and reported differences re-computed from the paper’s own numbers.

The self-check needs the paper’s full text.

Cites

Flagged first, then by citations

Research works printed but not linked: 41

  1. K. Symanzik, Renormalizable models with simple symmetry breaking. 1. Symmetry breaking by a source term, Commun. Math. Phys. 16 (1970) 48 [INSPIRE]. · DOI · Paper page
  2. S.R. Coleman, R. Jackiw and H.D. Politzer, Spontaneous Symmetry Breaking in the O(N ) Model for Large N, Phys. Rev. D 10 (1974) 2491 [INSPIRE]. · DOI · Paper page
  3. J. Iliopoulos, C. Itzykson and A. Martin, Functional Methods and Perturbation Theory, Rev. Mod. Phys. 47 (1975) 165 [INSPIRE]. · DOI · Paper page
  4. R.W. Haymaker and J. Perez-Mercader, Convexity of the Effective Potential, Phys. Rev. D 27 (1983) 1948 [INSPIRE]. · DOI · Paper page
  5. Y. Fujimoto, L. O'Raifeartaigh and G. Parravicini, Effective Potential for Nonconvex Potentials, Nucl. Phys. B 212 (1983) 268 [INSPIRE]. · DOI · Paper page
  6. C.M. Bender and F. Cooper, Failure of the Naive Loop Expansion for the Effective Potential in φ 4 Field Theory When There Is 'Broken Symmetry', Nucl. Phys. B 224 (1983) 403 [INSPIRE]. · DOI · Paper page
  7. M. Hindmarsh and D. Johnston, Convexity of the Effective Potential, J. Phys. A 19 (1986) 141 [INSPIRE]. JHEP05(2023)145 · DOI · Paper page
  8. P. Millington and P.M. Saffin, Visualising quantum effective action calculations in zero dimensions, J. Phys. A 52 (2019) 405401 [arXiv:1905.09674] [INSPIRE]. · DOI · Paper page
  9. J. Alexandre and A. Tsapalis, Maxwell Construction for Scalar Field Theories with Spontaneous Symmetry Breaking, Phys. Rev. D 87 (2013) 025028 [arXiv:1211.0921] [INSPIRE]. · DOI · Paper page
  10. J. Alexandre and D. Backhouse, One-loop tunneling-induced energetics, Phys. Rev. D 105 (2022) 105018 [arXiv:2203.12543] [INSPIRE]. · DOI
  11. J. Alexandre and D. Backhouse, NEC violation: Tunnelling versus the Casimir effect, arXiv:2301.02455 [INSPIRE]. · arXiv
  12. V.A. Rubakov, The Null Energy Condition and its violation, Phys. Usp. 57 (2014) 128 [arXiv:1401.4024] [INSPIRE]. · DOI · Paper page
  13. T.W.B. Kibble, Topology of Cosmic Domains and Strings, J. Phys. A 9 (1976) 1387 [INSPIRE]. · DOI
  14. W.H. Zurek, Cosmological Experiments in Superfluid Helium?, Nature 317 (1985) 505 [INSPIRE]. · DOI · Paper page
  15. P.C.W. Davies and S.A. Fulling, Radiation from Moving Mirrors and from Black Holes, Proc. Roy. Soc. Lond. A 356 (1977) 237 [INSPIRE]. · DOI
  16. V.K. Onemli and R.P. Woodard, Superacceleration from massless, minimally coupled φ 4 , Class. Quant. Grav. 19 (2002) 4607 [gr-qc/0204065] [INSPIRE]. · DOI
  17. E.-A. Kontou and K.D. Olum, Energy conditions allow eternal inflation, JCAP 03 (2021) 097 [arXiv:2008.01878] [INSPIRE]. · DOI · Paper page
  18. S.R. Coleman, The Fate of the False Vacuum. 1. Semiclassical Theory, Phys. Rev. D 15 (1977) 2929 [Erratum ibid. 16 (1977) 1248] [INSPIRE]. · DOI
  19. C.G. Callan Jr. and S.R. Coleman, The Fate of the False Vacuum. 2. First Quantum Corrections, Phys. Rev. D 16 (1977) 1762 [INSPIRE]. · DOI · Paper page
  20. A. Andreassen, D. Farhi, W. Frost and M.D. Schwartz, Precision decay rate calculations in quantum field theory, Phys. Rev. D 95 (2017) 085011 [arXiv:1604.06090] [INSPIRE]. · DOI
  21. W.-Y. Ai, B. Garbrecht and C. Tamarit, Functional methods for false vacuum decay in real time, JHEP 12 (2019) 095 [arXiv:1905.04236] [INSPIRE]. · DOI · Paper page
  22. K.J. Ludwick, The viability of phantom dark energy: A review, Mod. Phys. Lett. A 32 (2017) 1730025 [arXiv:1708.06981] [INSPIRE]. JHEP05(2023)145 · DOI
  23. P.J. Steinhardt and N. Turok, Cosmic evolution in a cyclic universe, Phys. Rev. D 65 (2002) 126003 [hep-th/0111098] [INSPIRE]. · DOI · Paper page
  24. J. Khoury, B.A. Ovrut, P.J. Steinhardt and N. Turok, The Ekpyrotic universe: Colliding branes and the origin of the hot big bang, Phys. Rev. D 64 (2001) 123522 [hep-th/0103239] [INSPIRE]. · DOI · Paper page
  25. J. Khoury et al., From big crunch to big bang, Phys. Rev. D 65 (2002) 086007 [hep-th/0108187] [INSPIRE]. · DOI · Paper page
  26. A.H. Guth, The Inflationary Universe: A Possible Solution to the Horizon and Flatness Problems, Phys. Rev. D 23 (1981) 347 [INSPIRE]. · DOI · Paper page
  27. A.D. Linde, A New Inflationary Universe Scenario: A Possible Solution of the Horizon, Flatness, Homogeneity, Isotropy and Primordial Monopole Problems, Phys. Lett. B 108 (1982) 389 [INSPIRE]. · DOI · Paper page
  28. J. Alexandre and K. Clough, Saving the universe with finite volume effects, Phys. Rev. D 100 (2019) 103522 [arXiv:1906.10662] [INSPIRE]. · DOI
  29. J. Alexandre and J. Polonyi, Tunnelling and dynamical violation of the Null Energy Condition, Phys. Rev. D 103 (2021) 105020 [arXiv:2101.08640] [INSPIRE]. · DOI
  30. M. Bordag, U. Mohideen and V.M. Mostepanenko, New developments in the Casimir effect, Phys. Rept. 353 (2001) 1 [quant-ph/0106045] [INSPIRE]. · DOI
  31. L.E. Parker and D. Toms, Quantum Field Theory in Curved Spacetime: Quantized Field and Gravity, Cambridge Monographs on Mathematical Physics, Cambridge University Press (2009) [DOI:10.1017/CBO9780511813924] [INSPIRE]. · DOI · Paper page
  32. B.L. Hu and D.J. O'Connor, Effective Lagrangian for λφ 4 Theory in Curved Space-time With Varying Background Fields: Quasilocal Approximation, Phys. Rev. D 30 (1984) 743 [INSPIRE]. · DOI
  33. T. Markkanen, S. Nurmi, A. Rajantie and S. Stopyra, The 1-loop effective potential for the Standard Model in curved spacetime, JHEP 06 (2018) 040 [arXiv:1804.02020] [INSPIRE]. · DOI
  34. D.V. Vassilevich, Heat kernel expansion: User's manual, Phys. Rept. 388 (2003) 279 [hep-th/0306138] [INSPIRE]. · DOI
  35. J.S. Schwinger, On gauge invariance and vacuum polarization, Phys. Rev. 82 (1951) 664 [INSPIRE]. · DOI · Paper page
  36. P.B. Gilkey, The Spectral geometry of a Riemannian manifold, J. Diff. Geom. 10 (1975) 601 [INSPIRE]. · DOI
  37. L. Parker and D.J. Toms, New Form for the Coincidence Limit of the Feynman Propagator, or Heat Kernel, in Curved Space-time, Phys. Rev. D 31 (1985) 953 [INSPIRE]. · DOI
  38. I. Jack and L. Parker, Proof of Summed Form of Proper Time Expansion for Propagator in Curved Space-time, Phys. Rev. D 31 (1985) 2439 [INSPIRE]. · DOI
  39. B.-L.B. Hu and E. Verdaguer, Semiclassical and Stochastic Gravity: Quantum Field Effects on Curved Spacetime, Cambridge Monographs on Mathematical Physics, Cambridge University Press (2020) [DOI:10.1017/9780511667497] [INSPIRE]. · DOI
  40. T. Markkanen and A. Tranberg, A Simple Method for One-Loop Renormalization in Curved Space-Time, JCAP 08 (2013) 045 [arXiv:1303.0180] [INSPIRE]. · DOI
  41. G.V. Dunne, Functional determinants in quantum field theory, in the proceedings of the 14th WE Heraeus Saalburg summer school Wolfersdorf, Thuringia (2009) [https://saalburg.aei.mpg.de/wp-content/uploads/sites/25/2017/03/dunne.pdf].

Cited by

Sorted by citations

Authors
Alexandre, J., & Pla, S.
Affiliations
King's College London (GB)
Corresponding author
Pla, Silvia
Venue
Journal of High Energy Physics
Published
2023-05-17
Volume
2023
Issue
5
ISSN
1029-8479 (ISSN-L)
OpenAlex
W4377107801
Cited by
6
References
4
Citations by year
2025: 2 · 2024: 3 · 2023: 1
FWCI
0.70
Type
journal article
Language
en
Open access
Locations
  • Journal of High Energy Physics (publishedVersion, cc-by)
  • arXiv (Cornell University) (submittedVersion, cc-by)
  • DOAJ (DOAJ: Directory of Open Access Journals) (submittedVersion, cc-by-sa)
  • Research Portal (King's College London) (submittedVersion, other-oa)
  • arXiv (Cornell University) (cc-by)
Funders
  • Leverhulme Trust (RPG-2021-299)
  • Engineering and Physical Sciences Research Council (EP/V002821/1)
  • Science and Technology Facilities Council (ST/T000759/1, STFC-ST/T000759/1)
Topics
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
  • Physical Sciences › Physics and Astronomy › Statistical and Nonlinear Physics › Noncommutative and Quantum Gravity Theories
  • Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Black Holes and Theoretical Physics
Keywords
bounce cosmology, phantom equation of state, tunneling, scalar field, degenerate vacua, null energy condition violation, de Sitter phase, double-well potential, quantum fluctuations, FLRW metric, true vacuum

About these checks

Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.

Statistics and arithmetic are recomputed, not judged.

Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.

What counts as a claim ›How we measure confidence ›How we check this ›

Are you an author, or do you see a problem with this page? Request a review