REVIEW 2 major objections 4 minor 29 references
In unbroken Weyl geometry no satisfactory proper time exists, because invariance, additivity, time dimension and affine parametrization cannot hold together.
Reviewed by Pith at T0; open to challenge. T0 means a machine referee read the full paper against a public rubric. the ladder, T0–T4 →
T0 review · grok-4.5
2026-07-30 18:38 UTC pith:HEWQLVX4
load-bearing objection Clean construction of the missing Weyl-invariant world-line action, plus a solid no-go for proper time in the unbroken phase; useful inside the subfield. the 2 major comments →
World-Line Actions in Weyl Geometry
The pith
A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.
Core claim
No quantity can simultaneously be Weyl-invariant, additive, of inverse-mass dimension and provide an affine parametrization of the geodesic equation in the unbroken phase of Weyl geometry; therefore no satisfactory notion of proper time exists until spontaneous symmetry breaking restores a mass scale and Riemannian geometry.
What carries the argument
The open Wilson line W(λ) on the world-line, solving the covariant-constancy condition D̂_λ W = 0. It supplies the non-local, Weyl-covariant dressing that turns the square-root length functional into a dimensionless, additive, gauge-invariant action whose Euler–Lagrange equation is the Weyl autoparallel equation.
Load-bearing premise
The claim rests on treating the four classical requirements—affine parametrization, inverse-mass dimension, additivity and Weyl invariance—as jointly necessary for any acceptable proper time; if a weaker operational definition is allowed, the no-go result need not hold.
What would settle it
Exhibit an explicit, additive, Weyl-invariant world-line parameter of inverse-mass dimension that still affinely parametrizes the Weyl geodesic equation in the symmetric phase, or show that after controlled symmetry breaking the predicted short-range corrections to Riemannian proper time are absent for dilaton-coupled particles.
If this is right
- Any second-clock-effect claim must be sought only in the broken phase, as residual Weyl corrections suppressed by the symmetry-breaking scale.
- Only particles that couple directly to the dilaton (e.g. the Higgs in minimal embeddings) can feel those corrections.
- The local einbein-plus-Lagrange-multiplier action supplies a practical starting point for path-integral quantization of particles in Weyl geometry.
- In the vacuum the world-line theory reduces exactly to the Riemannian massive-particle action with mass m = ξ⟨ϕ⟩.
Where Pith is reading between the lines
- If the no-go is accepted, historical arguments that used a non-local proper-time formula to prove a second clock effect were measuring something that is not an observable clock while symmetry is intact.
- Laboratory or astrophysical bounds on dilaton–Higgs couplings could indirectly constrain residual non-Riemannian corrections to clocks after breaking.
- The same Wilson-line dressing may organize other dimensionful observables (decay rates, cross sections) once they are required to be Weyl-invariant in the symmetric phase.
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. The paper constructs Weyl-invariant, dimensionless, additive world-line actions for a massive particle on a time-like curve in Weyl geometry, working from the modern gauge-theory formulation. In the integrable case the compensator is the local dilaton; in the general non-integrable case it is an open Wilson line built from the Weyl gauge field, yielding the non-local action (52). The Euler–Lagrange equations recover the autoparallel equation defined with the fully Weyl-covariant derivative. A classically equivalent quadratic einbein action is given, and non-locality is reinterpreted as the result of integrating out a constrained world-line field. The authors argue that the four classical requirements for proper time (affine parametrization, inverse-mass dimension, additivity, Weyl invariance) cannot be satisfied simultaneously in the unbroken phase, so no satisfactory proper time exists until spontaneous symmetry breaking reduces the action to the Riemannian one.
Significance. The work cleanly separates the construction of a consistent particle action from the long-standing debate on the second clock effect and proper time in Weyl geometry. By insisting on gauge invariance, dimensionality and additivity, it supplies an action suitable in principle for path-integral quantization and shows explicitly how the Riemannian massive-particle action and ordinary proper time re-emerge after scale symmetry breaking. The no-go statement for proper time in the symmetric phase, if accepted under the stated axioms, clarifies why earlier history-dependent proposals cannot serve as observables before breaking. The local constrained formulation (71) is a concrete technical contribution for future quantization studies.
major comments (2)
- [§3.3.2] §3.3.2, after Eq. (52): the derivation of the Euler–Lagrange equations is asserted to be “very similar to the pure gauge case” because W satisfies the covariant-constancy condition (43). Because W is a path-dependent open Wilson line, a careful functional variation with respect to x^μ(λ) must account for the change of the integration path inside the exponential. An explicit variation (or a short appendix) showing that no extra bulk terms arise beyond those already present for a local compensator would make the central claim fully rigorous.
- [§3.5] §3.5, Eqs. (63)–(65) and the surrounding text: the no-go result is presented as showing that “no satisfactory notion of proper time exists.” The argument is internally consistent once the four requirements are taken as jointly necessary, but that joint necessity is an interpretive axiom rather than a derived theorem. The manuscript should state the claim conditionally (“under the four classical requirements heta au cannot exist”) and briefly note that a weaker operational definition might evade the obstruction; this does not weaken the algebra but prevents over-statement.
minor comments (4)
- [Table 1, §3.5] Table 1 and the charge assignments: the Weyl charge p of ˙x^μ is left arbitrary throughout. A short remark on whether physical observables (or the path-integral measure) prefer a definite value (e.g. p = 0 or p = -1) would help the reader.
- [§3.3.2] Eq. (48) and the discussion of λ_0: the base point is left largely free (“-∞ or any point”). A sentence clarifying that physical predictions are independent of this choice once additivity (54) is imposed would remove a minor ambiguity.
- [Introduction / Conclusions] References: several closely related recent works on autoparallels and the inverse problem in non-metric geometries (e.g. the arXiv preprints cited as [16,17]) appeared nearly simultaneously; a slightly more comparative paragraph would better situate the novelty of (52) and (71).
- Typographical: “lenghts” (p. 2), “an einbeinon” (abstract), and occasional missing spaces around citations should be corrected in proof.
Circularity Check
No significant circularity: action and no-go follow from stated gauge/dimensional requirements without tautological redefinition or load-bearing self-citation loops.
full rationale
The paper’s load-bearing chain is: (i) adopt the autoparallel equation with the Weyl-covariant derivative as the geometric law of free fall; (ii) impose Weyl invariance, dimensionless-ness and additivity on a world-line functional and construct the unique (up to ξ and the integration constant W(λ₀)) action that reproduces that law—local dilaton for integrable Weyl geometry, open Wilson line for the general case; (iii) show that the four classical proper-time requirements (affine parametrization, inverse-mass dimension, additivity, Weyl invariance) are algebraically incompatible before spontaneous symmetry breaking. None of these steps reduces by construction to its own input. The EL equations of (52)/(66) are derived and matched to the autoparallel equation rather than assumed; the Wilson line is the explicit solution of the first-order covariant-constancy ODE on the world-line, not a renamed fit; the no-go is a direct charge-and-dimension counting argument (eqs. 63–65) once the four requirements are accepted as jointly necessary. Self-citations ([10], [26], etc.) supply the background gauge-theory formulation of Weyl geometry and are not used to close a uniqueness or existence loop inside the present derivations. There is no fitted parameter, no uniqueness theorem imported from the authors as an external fact, and no renaming of a known empirical pattern. Score 0 is therefore appropriate.
Axiom & Free-Parameter Ledger
free parameters (1)
- ξ
axioms (4)
- domain assumption Autoparallels of the Weyl-covariant derivative define the physical trajectories of free particles.
- domain assumption Physical observables must be Weyl-gauge invariant.
- ad hoc to paper An acceptable proper time must be additive, of inverse-mass dimension, Weyl invariant and affinely parametrize the geodesic equation.
- domain assumption The dilaton φ arises as the scalar mode of the R² term and carries Weyl charge -1.
invented entities (2)
-
Open Wilson-line compensator W(λ)
no independent evidence
-
Constrained world-line field W with Lagrange multiplier η
no independent evidence
read the original abstract
In this note we construct, from a gauge theory perspective, the world-line action for a particle moving on a time-like curve in Weyl geometry. The action we find is dimensionless, Weyl invariant, additive and, in general, non-local due to an open Wilson line which we have to add in order to account for a general Weyl field. In special cases, this Wilson line can be local, but the geometry becomes integrable. The action can not be used to measure the proper time as it is dimensionless and no mass parameter is allowed in the symmetric phase of the theory. We show that the usual conditions for defining proper time: affine parametrization, dimension of time and additivity supplemented by the requirement of Weyl invariance can not be fulfilled simultaneously and therefore no satisfactory notion of proper time exists in the symmetric phase. Under spontaneous symmetry breaking the particle acquires a mass, the action becomes Riemannian and the proper time can be again defined. We also construct a classically equivalent quadratic action by using an einbein on the world-line and show that the non-locality can be seen to arise from integrating out a constrained field.
Reference graph
Works this paper leans on
-
[1]
Eine neue Erweiterung der Relativit¨ atstheorie
Hermann Weyl, Gravitation und elektrizit¨ at, Sitzungsberichte der K¨ oniglich Preussischen Akademie der Wissenschaften zu Berlin (1918), pp.465; Einstein’s review appended, on atomic spectral lines changes due to non-metricity. Her- mann Weyl “Eine neue Erweiterung der Relativit¨ atstheorie” (“A new extension of the theory of relativity”), Ann. Phys. (Le...
1918
-
[2]
No-ghost theorem for the fourth-order derivative Pais-Uhlenbeck oscillator model,
C. M. Bender and P. D. Mannheim, “No-ghost theorem for the fourth-order derivative Pais-Uhlenbeck oscillator model,” Phys. Rev. Lett.100(2008), 110402 doi:10.1103/PhysRevLett.100.110402 [arXiv:0706.0207 [hep-th]]
Pith/arXiv arXiv 2008
-
[3]
Einstein Gravity from Conformal Gravity,
J. Maldacena, “Einstein Gravity from Conformal Gravity,” [arXiv:1105.5632 [hep-th]]
-
[4]
Solution to the ghost problem in higher-derivative gravity,
P. D. Mannheim, “Solution to the ghost problem in higher-derivative gravity,” Nuovo Cim. C45(2022) no.2, 27 doi:10.1393/ncc/i2022-22027-6 [arXiv:2109.12743 [hep-th]]
Pith/arXiv arXiv 2022
-
[5]
K. S. Kumar and J. Marto, “Quantum (quadratic) gravity: replacing the massive tensor ghost with an inverted harmonic oscillator-like instability,” [arXiv:2603.07150 [hep-th]]
-
[6]
Renormalization of Higher Derivative Quantum Gravity,
K. S. Stelle, “Renormalization of Higher Derivative Quantum Gravity,” Phys. Rev. D16(1977), 953-969 doi:10.1103/PhysRevD.16.953. 18
-
[7]
Weyl conformal geometry vs Weyl anomaly,
D. M. Ghilencea, “Weyl conformal geometry vs Weyl anomaly,” JHEP10(2023), 113 doi:10.1007/JHEP10(2023)113 [arXiv:2309.11372 [hep-th]]
Pith/arXiv arXiv 2023
-
[8]
Long range forces and broken symmetries,
P. A. M. Dirac, “Long range forces and broken symmetries,” Proc. Roy. Soc. Lond. A333(1973), 403-418 doi:10.1098/rspa.1973.0070
arXiv 1973
-
[9]
Weyl gauge theories of gravity do not predict a second clock effect,
M. P. Hobson and A. N. Lasenby, “Weyl gauge theories of gravity do not predict a second clock effect,” Phys. Rev. D102, no.8, 084040 (2020) doi:10.1103/PhysRevD.102.084040 [arXiv:2009.06407 [gr-qc]]. M. Hob- son and A. Lasenby, “Note on the absence of the second clock effect in Weyl gauge theories of gravity,” Phys. Rev. D105, no.2, L021501 (2022) doi:10....
Pith/arXiv arXiv 2020
-
[10]
Weyl quadratic gravity as a gauge theory and non-metricity vs torsion duality,
C. Condeescu, D. M. Ghilencea and A. Micu, “Weyl quadratic gravity as a gauge theory and non-metricity vs torsion duality,” Eur. Phys. J. C84, no.3, 292 (2024) doi:10.1140/epjc/s10052-024-12644-6 [arXiv:2312.13384 [hep-th]]
Pith/arXiv arXiv 2024
-
[11]
Characterization of Standard Clocks by Means of Light Rays and Freely Falling Particles,
V. Perlick, “Characterization of Standard Clocks by Means of Light Rays and Freely Falling Particles,” Gen. Rel. Grav.19, 1059-1073 (1987)
1987
-
[12]
A Note on the Problem of Proper Time in Weyl Space–Time,
R. Avalos, F. Dahia and C. Romero, “A Note on the Problem of Proper Time in Weyl Space–Time,” Found. Phys.48, no.2, 253-270 (2018) doi:10.1007/s10701- 017-0134-z [arXiv:1611.10198 [gr-qc]]
Pith/arXiv arXiv 2018
-
[13]
Conformally invariant proper time with general non-metricity,
A. Delhom, I. P. Lobo, G. J. Olmo and C. Romero, “Conformally invariant proper time with general non-metricity,” Eur. Phys. J. C80, no.5, 415 (2020) doi:10.1140/epjc/s10052-020-7974-y [arXiv:2001.10633 [gr-qc]]
Pith/arXiv arXiv 2020
-
[14]
Nonmetricity theories and aspects of gauge symmetry,
I. Quiros, “Nonmetricity theories and aspects of gauge symmetry,” Phys. Rev. D 105, no.10, 104060 (2022) doi:10.1103/PhysRevD.105.104060 [arXiv:2111.05490 [gr-qc]], I. Quiros, “Gauge invariant approach to nonmetricity theories and the second clock effect,” [arXiv:2201.03076 [gr-qc]]
Pith/arXiv arXiv 2022
-
[15]
Republication of: The geometry of free fall and light propagation,
J. Ehlers, F. A. E. Pirani and A. Schild, “Republication of: The geometry of free fall and light propagation,” Gen. Rel. Grav.44, no.6, 1587-1609 (2012) doi:10.1007/s10714-012-1353-4
-
[16]
Autoparallels and the Inverse Problem of the Calculus of Vari- ations,
L. Heisenberg, “Autoparallels and the Inverse Problem of the Calculus of Vari- ations,” [arXiv:2603.11581 [math-ph]]
-
[17]
On the Finsler variational nature of autoparallels in metric-affine geometry,
L. Csillag, N. Voicu, S. Elgendi and C. Pfeifer, “On the Finsler variational nature of autoparallels in metric-affine geometry,” [arXiv:2603.18416 [math-ph]]
-
[18]
Standard Model in Weyl conformal geometry,
D. M. Ghilencea, “Standard Model in Weyl conformal geometry,” Eur. Phys. J. C82(2022) no.1, 23 doi:10.1140/epjc/s10052-021-09887-y [arXiv:2104.15118 [hep-ph]]. 19
Pith/arXiv arXiv 2022
-
[19]
Scale- independentR 2 inflation,
P. G. Ferreira, C. T. Hill, J. Noller and G. G. Ross, “Scale- independentR 2 inflation,” Phys. Rev. D100, no.12, 123516 (2019) doi:10.1103/PhysRevD.100.123516 [arXiv:1906.03415 [gr-qc]]
Pith/arXiv arXiv 2019
-
[20]
Weyl R 2 inflation with an emergent Planck scale,
D. M. Ghilencea, “Weyl R 2 inflation with an emergent Planck scale,” JHEP10, 209 (2019) doi:10.1007/JHEP10(2019)209 [arXiv:1906.11572 [gr-qc]]
Pith/arXiv arXiv 2019
-
[21]
Testing Weyl geometric gravity with the SPARC galactic rotation curves database,
M. Cr˘ aciun and T. Harko, “Testing Weyl geometric gravity with the SPARC galactic rotation curves database,” Phys. Dark Univ.43, 101423 (2024) doi:10.1016/j.dark.2024.101423 [arXiv:2311.16893 [gr-qc]]
arXiv 2024
-
[22]
Weyl gauge symmetry at LIGO-Virgo- KAGRA,
D. M. Ghilencea and V. M. Mandric, “Weyl gauge symmetry at LIGO-Virgo- KAGRA,” [arXiv:2607.13146 [gr-qc]]
-
[23]
R. M. Wald, “General Relativity,” Chicago Univ. Pr., 1984, doi:10.7208/chicago/9780226870373.001.0001
arXiv 1984
-
[24]
Spacetime and Geometry: An Introduction to General Rela- tivity,
S. M. Carroll, “Spacetime and Geometry: An Introduction to General Rela- tivity,” Cambridge University Press, 2019, ISBN 978-0-8053-8732-2, 978-1-108- 48839-6, 978-1-108-77555-7 doi:10.1017/9781108770385
-
[25]
Spontaneous breaking of Weyl quadratic grav- ity to Einstein action and Higgs potential,
D. M. Ghilencea, “Spontaneous breaking of Weyl quadratic grav- ity to Einstein action and Higgs potential,” JHEP1903(2019) 049 doi:10.1007/JHEP03(2019)049 [arXiv:1812.08613 [hep-th]]. D. M. Ghilencea, “Stueckelberg breaking of Weyl conformal geometry and applications to grav- ity,” Phys. Rev. D101(2020) no.4, 045010 doi:10.1103/PhysRevD.101.045010 [arXiv:...
Pith/arXiv arXiv 2019
-
[26]
The gauge theory of Weyl group and its interpre- tation as Weyl quadratic gravity,
C. Condeescu and A. Micu, “The gauge theory of Weyl group and its interpre- tation as Weyl quadratic gravity,” Class. Quant. Grav.42, no.6, 065011 (2025) doi:10.1088/1361-6382/adb3e8 [arXiv:2408.07159 [hep-th]]
Pith/arXiv arXiv 2025
-
[28]
Conformalons: a new class of black hole mimickers,
L. Modesto, A. Akil and C. Bambi, “Conformalons: a new class of black hole mimickers,” Eur. Phys. J. C85(2025) no.6, 603 doi:10.1140/epjc/s10052-025- 14340-5 [arXiv:2106.03914 [gr-qc]]
Pith/arXiv arXiv 2025
-
[29]
Weyl conformal geometry vs Riemannian geometry of Weyl gauge invariant dressed metric,
D. M. Ghilencea and V. M. Mandric, “Weyl conformal geometry vs Riemannian geometry of Weyl gauge invariant dressed metric,” [arXiv:2606.08080 [hep-th]]
-
[30]
In preparation
C. Condeescu and A. Micu, “In preparation”. 20
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.