Quantum corrections to symmetron fifth forces for planar sources
Pith reviewed 2026-06-30 00:48 UTC · model grok-4.3
The pith
Quantum corrections suppress symmetron fifth forces near planar sources by order 10 percent.
A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.
Core claim
We provide a semi-analytic calculation of the first quantum corrections to the symmetron fifth force around a planar source with nonzero thickness. We find a suppression of the fifth force compared with the classical prediction within a Compton wavelength of the source, which is of order 10% in the parameter region relevant to experiments like CANNEX, while the fifth force is enhanced at larger distances from the source. The resulting change in the spatial profile of the fifth force may be relevant to current and near future terrestrial and astrophysical tests of force laws, and has implications for the optimisation of experimental geometries, including atom interferometers.
What carries the argument
Semi-analytic evaluation of one-loop quantum corrections to the symmetron scalar profile and the derived fifth force for a thick planar source.
If this is right
- The modified force profile affects the interpretation of current and near-future tests of force laws.
- Optimisation of experimental geometries, including atom interferometers, must account for the altered spatial dependence.
- The calculation supplies a benchmark for future numerical studies of quantum-corrected fifth forces in screened scalar-tensor theories.
- The distance-dependent change from suppression to enhancement can shift the effective range probed by different detector placements.
Where Pith is reading between the lines
- The same semi-analytic method could be applied to spherical or cylindrical sources to check whether the 10 percent scale persists.
- Higher-order loop corrections or different source densities might be checked numerically to confirm the leading term dominates.
- The enhancement at large distances could alter bounds extracted from astrophysical systems where the source-observer separation exceeds the Compton wavelength.
Load-bearing premise
The semi-analytic approximation used to compute the leading quantum corrections remains valid for the chosen planar source thickness and does not miss dominant higher-order contributions.
What would settle it
A precision measurement of the fifth-force profile around a planar source that shows no suppression of order 10 percent inside one Compton wavelength would falsify the reported quantum correction.
read the original abstract
We provide a semi-analytic calculation of the first quantum corrections to the symmetron fifth force around a planar source with nonzero thickness. We find a suppression of the fifth force compared with the classical prediction within a Compton wavelength of the source, which is of order 10% in the parameter region relevant to experiments like CANNEX, while the fifth force is enhanced at larger distances from the source. The resulting change in the spatial profile of the fifth force may be relevant to current and near future terrestrial and astrophysical tests of force laws, and has implications for the optimisation of experimental geometries, including atom interferometers. This work provides a key benchmark for future numerical studies of quantum-corrected fifth forces in screened scalar-tensor theories of gravity.
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. The manuscript presents a semi-analytic calculation of the leading quantum corrections to the symmetron fifth force for a planar source of finite thickness. It reports an approximately 10% suppression of the fifth force relative to the classical prediction within one Compton wavelength of the source (in the parameter regime relevant to CANNEX), together with an enhancement at larger distances, and discusses implications for experimental tests of modified gravity and optimization of geometries such as atom interferometers. The work is positioned as a benchmark for future numerical studies of quantum-corrected fifth forces in screened scalar-tensor theories.
Significance. If the quantitative result is reliable, the paper supplies a concrete benchmark for quantum effects in symmetron models that could affect the interpretation of near-future fifth-force searches; the explicit semi-analytic treatment of the first corrections and the identification of a sign change in the correction across the Compton scale are useful reference points even if higher-order terms ultimately modify the 10% figure.
major comments (3)
- [Calculation of quantum corrections / Results] The semi-analytic approximation employed for the leading quantum corrections (detailed in the calculation of the symmetron profile) supplies no explicit error bound on the neglected higher-order contributions nor a direct comparison against a fully numerical solution of the same effective theory; because the headline 10% suppression is extracted from this truncation, the absence of such validation is load-bearing for the central quantitative claim.
- [Setup and source model] The choice of planar source thickness is stated to be representative, yet no sensitivity analysis or demonstration is given that the reported suppression/enhancement profile remains stable under modest variations in thickness; this is required to confirm that the geometry does not introduce uncontrolled artifacts in the semi-analytic step.
- [Discussion / Implications] The abstract and introduction frame the result as directly relevant to CANNEX, but the parameter region in which the 10% figure is obtained is not cross-checked against the precise experimental constraints or screening lengths used in that experiment; a short table or explicit mapping would strengthen the claim.
minor comments (3)
- [Introduction] Notation for the Compton wavelength and the symmetron vacuum expectation value should be introduced once with a clear equation reference rather than assumed from prior literature.
- [Figures] Figure captions would benefit from explicit statements of the parameter values (e.g., λ, eta, source thickness) used to generate each curve, to allow immediate reproduction of the plotted profiles.
- [Methods] A brief statement on the range of validity of the semi-analytic expansion (e.g., in terms of the coupling strength or source density) would improve clarity without altering the technical content.
Simulated Author's Rebuttal
We thank the referee for their thoughtful review and constructive suggestions. We address each of the major comments below.
read point-by-point responses
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Referee: [Calculation of quantum corrections / Results] The semi-analytic approximation employed for the leading quantum corrections (detailed in the calculation of the symmetron profile) supplies no explicit error bound on the neglected higher-order contributions nor a direct comparison against a fully numerical solution of the same effective theory; because the headline 10% suppression is extracted from this truncation, the absence of such validation is load-bearing for the central quantitative claim.
Authors: We agree that an explicit error bound would strengthen the presentation. However, deriving rigorous bounds on the truncation error in this semi-analytic approach is technically involved and beyond the scope of the current work, which focuses on the leading correction. We have added a paragraph in the discussion section explaining the perturbative nature of the expansion and estimating the size of higher-order terms based on the small parameter in the regime considered. A full numerical validation is left for future work, as stated in the manuscript's positioning as a benchmark. revision: partial
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Referee: [Setup and source model] The choice of planar source thickness is stated to be representative, yet no sensitivity analysis or demonstration is given that the reported suppression/enhancement profile remains stable under modest variations in thickness; this is required to confirm that the geometry does not introduce uncontrolled artifacts in the semi-analytic step.
Authors: The thickness was chosen to be representative of experimental setups like CANNEX. To address this, we will include in the revised manuscript a sensitivity analysis demonstrating that the qualitative features (suppression within one Compton wavelength and enhancement beyond) persist under variations of the thickness by factors of order 1 within the screened regime. revision: yes
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Referee: [Discussion / Implications] The abstract and introduction frame the result as directly relevant to CANNEX, but the parameter region in which the 10% figure is obtained is not cross-checked against the precise experimental constraints or screening lengths used in that experiment; a short table or explicit mapping would strengthen the claim.
Authors: We will add a short table in the revised version mapping the parameters used in our calculation to the experimental constraints and screening lengths relevant to CANNEX, to make the connection explicit. revision: yes
Circularity Check
No significant circularity in derivation chain
full rationale
The paper presents a direct semi-analytic computation of leading quantum corrections to the symmetron profile and fifth force for a finite-thickness planar source. The reported suppression (order 10% within one Compton wavelength) and enhancement at larger distances are framed as outputs of this calculation applied to the symmetron effective theory, not as quantities fitted to data or defined in terms of themselves. No load-bearing self-citations, ansatzes smuggled via prior work, or self-definitional steps are described in the abstract or context; the result is positioned as a benchmark for future numerics rather than a tautological renaming or forced prediction. The derivation chain is therefore self-contained against the model equations.
Axiom & Free-Parameter Ledger
Reference graph
Works this paper leans on
-
[1]
Mehta, P
K. Mehta, P. Kumar and A. Beesham,Thermodynamics and energy conditions of accelerating brans–dicke universe,International Journal of Geometric Methods in Modern Physics(2026)
2026
-
[2]
Kepuladze,Radiative dark energy in a seesaw framework,Physics Letters B876(2026) 140422
Z. Kepuladze,Radiative dark energy in a seesaw framework,Physics Letters B876(2026) 140422
2026
-
[3]
Beesham, A.M
A. Beesham, A.M. Msomi and S.C. Gumede,Scalar field dark energy model via observational constraints,Gravitation and Cosmology32(2026) 70–86
2026
-
[4]
Almurr and J.C
E. Almurr and J.C. Assaf,Finite-range scalar–tensor gravity: Constraints from cosmology and galaxy dynamics,Galaxies14(2026) 7
2026
-
[5]
Zaregonbadi, N
R. Zaregonbadi, N. Saba and M. Farhoudi,Chameleon gravity as an alternative to dark matter, The European Physical Journal C85(2025)
2025
-
[6]
Dabbaghsaz and A
E. Dabbaghsaz and A. Mohebalhojeh,Integrated collective dynamics: A purely theoretical scalar-tensor framework for gravitational dynamics without dark components,Nuclear Physics B1018(2025) 117029
2025
-
[7]
Feleppa, W.M
F. Feleppa, W.M. de Graaf, P. Brax and G. Lambiase,Bounds on screened dark energy from near-earth space-based measurements,Physical Review Letters136(2026)
2026
-
[8]
Gallardo, K
P. Gallardo, K. Pardo, O. Philcox, N. Battaglia, E. Battistelli, R. Bean et al.,Test of the gravitational force law on cosmological scales using the kinematic sunyaev-zeldovich effect, Physical Review Letters136(2026) . – 24 –
2026
-
[9]
Will,The confrontation between general relativity and experiment,Living Reviews in Relativity4(2001)
C.M. Will,The confrontation between general relativity and experiment,Living Reviews in Relativity4(2001)
2001
-
[10]
Clifton, P.G
T. Clifton, P.G. Ferreira, A. Padilla and C. Skordis,Modified gravity and cosmology,Physics Reports513(2012) 1–189
2012
-
[11]
Amendola, C
L. Amendola, C. Bernal and R. Gannouji,Nonlinear dynamics in horndeski gravity: A renormalized approach to effective gravitational coupling,Physical Review D112(2025)
2025
-
[12]
K. Hinterbichler, J. Khoury, A. Levy and A. Matas,Symmetron Cosmology,Phys. Rev. D84 (2011) 103521 [1107.2112]
Pith/arXiv arXiv 2011
-
[13]
K¨ ading,Lensing with Generalized Symmetrons,Astronomy2(2023) 128 [2304.05875]
C. K¨ ading,Lensing with Generalized Symmetrons,Astronomy2(2023) 128 [2304.05875]
arXiv 2023
-
[14]
Bachs-Esteban, I
J. Bachs-Esteban, I. Lopes and J. Rubio,Screening mechanisms on white dwarfs: Symmetron and dilaton,Universe11(2025) 158
2025
-
[15]
Burrage, A
C. Burrage, A. Kuribayashi-Coleman, J. Stevenson and B. Thrussell,Constraining symmetron fields with atom interferometry,J. Cosmol. Astropart. Phys.2016(2016) 041
2016
-
[16]
P. Brax, A.-C. Davis and B. Elder,(g-2)µand screened modified gravity,Phys. Rev. D106 (2022) 044040 [2111.01188]
arXiv 2022
-
[17]
L. Sun, B.J.J. Slagmolen and J. Qin,Differential torsion sensor for direct detection of ultralight vector dark matter,Phys. Rev. D111(2025) 063064 [2402.08935]
arXiv 2025
-
[18]
A. Krishak and S. Desai,Model comparison tests of modified gravity from the e¨ ot-wash experiment,JCAP07(2020) 006 [2003.10127]
arXiv 2020
-
[19]
T.A. Wagner, S. Schlamminger, J.H. Gundlach and E.G. Adelberger,Torsion-balance tests of the weak equivalence principle,Class. Quant. Grav.29(2012) 184002 [1207.2442]
Pith/arXiv arXiv 2012
-
[20]
Sedmik and M
R.I.P. Sedmik and M. Pitschmann,Next generation design and prospects for cannex,Universe 7(2021) 234
2021
-
[21]
H. Fischer, C. K¨ ading and M. Pitschmann,Quantum and thermal pressures from light scalar fields,Phys. Dark Univ.47(2025) 101756 [2407.20658]
arXiv 2025
-
[22]
Brax, A.-C
P. Brax, A.-C. Davis and B. Elder,Screened scalar fields in hydrogen and muonium,Phys. Rev. D107(2023) 044008
2023
-
[23]
A. Dvorak, K. Obigane, H. Lemmel, T. Jenke and S. Sponar,Experimental test of symmetron-field based dark energy model using neutron interferometry,2606.03440
-
[24]
H. Fischer, C. K¨ ading, H. Lemmel, S. Sponar and M. Pitschmann,Search for dark energy with neutron interferometry,PTEP2024(2024) 023E02 [2310.18109]
arXiv 2024
- [25]
-
[26]
Jenke et al.,Testing gravity at short distances: Gravity resonance spectroscopy with qbounce, EPJ Web Conf.219(2019) 05003
T. Jenke et al.,Testing gravity at short distances: Gravity resonance spectroscopy with qbounce, EPJ Web Conf.219(2019) 05003
2019
-
[27]
Yin et al.,Experimental constraints on the symmetron field with a magnetically levitated force sensor,Nature Astron.9(2025) 598
P. Yin et al.,Experimental constraints on the symmetron field with a magnetically levitated force sensor,Nature Astron.9(2025) 598
2025
-
[28]
J. Li and K.-d. Zhu,Constraining symmetron fields with a levitated optomechanical system, JCAP04(2025) 036 [2411.17744]
arXiv 2025
-
[29]
Brax and S
P. Brax and S. Fichet,Quantum chameleons,Physical Review D99(2019)
2019
-
[30]
Brax and S
P. Brax and S. Fichet,Scalar-mediated quantum forces between macroscopic bodies and interferometry,Physics of the Dark Universe42(2023) 101294. – 25 –
2023
-
[31]
Millington and M
P. Millington and M. Udemba,Quantum corrections to symmetron fifth-force profiles,Journal of Cosmology and Astroparticle Physics2026(2026) 087
2026
-
[32]
Coleman,Fate of the false vacuum: Semiclassical theory,Physical Review D15(1977) 2929
S. Coleman,Fate of the false vacuum: Semiclassical theory,Physical Review D15(1977) 2929
1977
-
[33]
Coleman,Erratum: Fate of the false vacuum: semiclassical theory,Physical Review D16 (1977) 1248
S. Coleman,Erratum: Fate of the false vacuum: semiclassical theory,Physical Review D16 (1977) 1248
1977
-
[34]
Callan and S
C.G. Callan and S. Coleman,Fate of the false vacuum. ii. first quantum corrections,Physical Review D16(1977) 1762
1977
-
[35]
B. Garbrecht and P. Millington,Green’s function method for handling radiative effects on false vacuum decay,Phys. Rev. D91(2015) 105021 [1501.07466]
Pith/arXiv arXiv 2015
-
[36]
Burrage, B
C. Burrage, B. Elder and P. Millington,Particle level screening of scalar forces in1 + 1 dimensions,Phys. Rev. D99(2019) 024045
2019
-
[37]
Brax and M
P. Brax and M. Pitschmann,Exact solutions to nonlinear symmetron theory: One- and two-mirror systems,Phys. Rev. D97(2018) 064015
2018
-
[38]
Pitschmann,Exact solutions to nonlinear symmetron theory: One- and two-mirror systems
M. Pitschmann,Exact solutions to nonlinear symmetron theory: One- and two-mirror systems. ii.,Phys. Rev. D103(2021) 084013
2021
-
[39]
Hinterbichler and J
K. Hinterbichler and J. Khoury,Screening long-range forces through local symmetry restoration, Physical Review Letters104(2010)
2010
-
[40]
Burrage, B
C. Burrage, B. Elder, P. Millington, D. Saadeh and B. Thrussell,Fifth-force screening around extremely compact sources,Journal of Cosmology and Astroparticle Physics2021(2021) 052
2021
-
[41]
A. Almasi, P. Brax, D. Iannuzzi and R.I. Sedmik,Force sensor for chameleon and casimir force experiments with parallel-plate configuration,Physical Review D91(2015) . [42]Heun’s Differential Equations, Oxford University PressOxford (1995), 10.1093/oso/9780198596950.001.0001
-
[42]
P. Millington and M. Udemba,Quantum corrections to symmetron fifth-force profiles,JCAP 02(2026) 087 [2508.16726]
Pith/arXiv arXiv 2026
-
[43]
Garbrecht and P
B. Garbrecht and P. Millington,Self-consistent solitons for vacuum decay in radiatively generated potentials,Phys. Rev. D92(2015) 125022
2015
-
[44]
Birkandan, P.-L
T. Birkandan, P.-L. Giscard and A. Tamar,Computations of general heun functions from their integral series representations, in2021 Days on Diffraction (DD), p. 12–18, IEEE, May, 2021, DOI
2021
-
[45]
Udemba,mudemba/heun path sum, 2026
M. Udemba,mudemba/heun path sum, 2026. 10.5281/zenodo.20732181
- [46]
-
[47]
C. Briddon, C. Burrage, A. Moss and A. Tamosiunas,Using machine learning to optimise chameleon fifth force experiments,JCAP02(2024) 011 [2308.00844]
arXiv 2024
-
[48]
G.E. Andrews, R. Askey and R. Roy,Special Functions, Cambridge University Press (Jan., 1999), 10.1017/cbo9781107325937
-
[49]
Ruby and M
V.C. Ruby and M. Lakshmanan,A quantum approach to the continuum heisenberg spin-chain model: Position-dependent mass formalism and pre-canonical quantization,Journal of Mathematical Physics66(2025)
2025
-
[50]
L.-B. Wu, L. Xie, L.-M. Cao, M.-F. Ji and Y.-S. Zhou,Quasinormal modes of schwarzschild-de sitter black holes in semi-open systems,Science China Physics, Mechanics and Astronomy69 (2026)
2026
-
[51]
E.T. Whittaker and G.N. Watson,A Course of Modern Analysis, Cambridge University Press (Sept., 1996), 10.1017/cbo9780511608759. – 26 –
-
[52]
Arscott,Periodic Differential Equations, Elsevier (1964), 10.1016/c2013-0-01721-5
F.M. Arscott,Periodic Differential Equations, Elsevier (1964), 10.1016/c2013-0-01721-5. – 27 –
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