Covariant variation for point-particle Lagrangians
Pith reviewed 2026-06-25 20:49 UTC · model grok-4.3
The pith
Covariant variations defined along worldlines allow consistent Lagrangians for spinning particles and null light models in general relativity.
A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.
Core claim
Following DeWitt's construction, several types of variation are distinguished and the corresponding covariant variations are defined; the role of parallel transport is identified in models that couple worldline variables to tensor fields. The resulting framework simplifies the variational treatment of the MPD equations and produces a simple Lagrangian for the null-particle model of light propagation.
What carries the argument
The covariant variation for each type of variation, which incorporates parallel transport to maintain consistency when worldline quantities couple to spacetime tensor fields.
If this is right
- The MPD equations follow from a variational principle once the covariant variation is used.
- A simple Lagrangian exists for the null-particle model of light propagation.
- The same distinction of variation types applies to other point-particle models that couple to tensor fields along a worldline.
Where Pith is reading between the lines
- The method may be applied directly to higher-order multipole models without re-deriving variation rules from scratch.
- Numerical codes that evolve worldline quantities could incorporate the covariant variation to enforce consistency with the background metric.
- The construction could be tested by comparing conserved quantities obtained variationally with those obtained from the known MPD conserved quantities.
Load-bearing premise
The relevant dynamical quantities are defined only along the representative worldline and therefore require special care when coupled to tensor fields.
What would settle it
Derive the equations of motion from the proposed Lagrangian for the MPD model and check whether they match the standard Mathisson-Papapetrou-Dixon form; mismatch would falsify the construction.
read the original abstract
Structureless test particles in general relativity follow geodesics. For extended bodies, higher-order multipole moments lead to departures from geodesic motion; in particular, spinning test bodies obey the Mathisson--Papapetrou--Dixon (MPD) equations. Similarly, the leading correction to the eikonal approximation for electromagnetic-wave propagation can be formulated as the nongeodesic propagation of spinning null particles. When the resulting equations are treated as standalone worldline models, with the relevant dynamical quantities defined only along the representative worldline, their variational formulation requires particular care.Following DeWitt's construction, we distinguish several types of variation, define the corresponding covariant variation for each, and identify the role of parallel transport in models that couple worldline variables to tensor fields. This framework simplifies the variational treatment of the MPD equations and yields a simple Lagrangian for the null-particle model of light propagation.
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. The manuscript develops a covariant variation framework for point-particle Lagrangians in general relativity. Following DeWitt's construction, it distinguishes several types of variation, defines the corresponding covariant variants, and identifies the role of parallel transport when worldline quantities couple to tensor fields. The central claims are that this framework simplifies the variational treatment of the Mathisson-Papapetrou-Dixon (MPD) equations and yields a simple Lagrangian for the null-particle model of light propagation.
Significance. If the derivations and explicit checks hold, the framework would offer a useful technical tool for variational problems involving extended bodies and approximate wave propagation in GR, by cleanly handling the coupling of worldline variables to tensor fields via parallel transport. The approach is grounded in standard GR variational methods with independent grounding in the cited DeWitt construction and introduces no free parameters or ad-hoc entities.
major comments (1)
- Abstract: The abstract describes the approach at high level but provides no derivations, error analysis, or explicit checks; central claims cannot be verified from available text.
Simulated Author's Rebuttal
We thank the referee for their thoughtful review and positive assessment of the manuscript's potential utility. We address the single major comment below.
read point-by-point responses
-
Referee: [—] Abstract: The abstract describes the approach at high level but provides no derivations, error analysis, or explicit checks; central claims cannot be verified from available text.
Authors: We agree that the abstract is written at a high level and does not contain derivations or explicit checks, which is typical to maintain conciseness. The full manuscript provides the detailed construction following DeWitt, the definitions of covariant variations, the role of parallel transport, the simplified variational derivation of the MPD equations, and the explicit Lagrangian for the null-particle model together with its verification against known propagation equations. To improve verifiability of the central claims directly from the abstract, we will revise the abstract to briefly reference the key results and checks contained in the body of the paper. revision: yes
Circularity Check
No significant circularity
full rationale
The paper's central construction distinguishes variation types following the external DeWitt reference and defines a covariant variant to handle worldline-tensor couplings. This step is grounded in standard GR variational principles and does not reduce by definition or self-citation to the paper's own inputs. The claimed simplifications for MPD equations and the null-particle Lagrangian follow directly from the framework without fitted parameters, self-definitional loops, or load-bearing self-citations. The derivation remains self-contained against external benchmarks.
Axiom & Free-Parameter Ledger
Reference graph
Works this paper leans on
-
[1]
Sachs, Gravitational waves in general relativity
R. Sachs, Gravitational waves in general relativity. VI. The outgoing radiation condition, Proc. R. Soc. A264, 309 (1961)
1961
-
[2]
Kristian and R
J. Kristian and R. K. Sachs, Observations in Cosmology, Astro- phys. J.143, 379 (1966)
1966
-
[3]
Ehlers, Zum ¨Ubergang von der Wellenoptik zur geometrischen Optik in der allgemeinen Relativit¨atstheorie, Z
J. Ehlers, Zum ¨Ubergang von der Wellenoptik zur geometrischen Optik in der allgemeinen Relativit¨atstheorie, Z. Naturforsch. A 22, 1328 (1967)
1967
-
[4]
S. Seitz, P. Schneider, and J. Ehlers, Light propagation in arbi- trary spacetimes and the gravitational lens approximation, Class. Quantum Grav.11, 2345 (1994). arXiv:astro-ph/9403056 [astro- ph] (1994)
Pith/arXiv arXiv 1994
-
[5]
V . P. Frolov and A. A. Shoom, Spinoptics in a stationary space- time, Phys. Rev. D84, 044026 (2011). arXiv:1105.5629 [gr-qc] (2011)
Pith/arXiv arXiv 2011
-
[6]
C. M. Will, Theory and Experiment in Gravitational Physics (Cambridge University Press, Cambridge, 2018)
2018
-
[7]
M. A. Oanceaet al., Gravitational spin Hall effect of light, Phys. Rev. D102, 024075 (2020). arXiv:2003.04553 [gr-qc] (2020)
arXiv 2020
-
[8]
L. Andersson, J. Joudioux, M. A. Oancea, and A. Raj, Propaga- tion of polarized gravitational waves, Phys. Rev. D103, 044053 (2021). arXiv:2012.08363 [gr-qc] (2020)
arXiv 2021
-
[9]
V . P. Frolov and A. A. Shoom, Gravitational spinoptics in a curved space-time, J. Cosmol. Astropart. Phys.2024, 039 (2024). arXiv:2406.17905 [gr-qc] (2024)
arXiv 2024
-
[10]
S. R. Dolan, Higher-order geometrical optics for electromagnetic waves on a curved spacetime, arXiv:1801.02273 [gr-qc] (2018). 9
Pith/arXiv arXiv 2018
-
[11]
S. R. Dolan, Geometrical optics for scalar, electromagnetic and gravitational waves on curved spacetime, Int. J. Mod. Phys. D 27, 1843010 (2018). arXiv:1806.08617 [gr-qc] (2018)
Pith/arXiv arXiv 2018
-
[12]
V . P. Frolov, Maxwell equations in a curved spacetime: Spin optics approximation, Phys. Rev. D102, 084013 (2020). arXiv:2007.03743 [gr-qc] (2020)
arXiv 2020
-
[13]
L. Andersson and M. A. Oancea, Spin Hall effects in the sky, Class. Quantum Grav.40, 154002 (2023). arXiv:2302.13634 [gr-qc] (2023)
arXiv 2023
-
[14]
Souriau, Mod `ele de particule `a spin dans le champ ´electromagn´etique et gravitationnel, Ann
J.-M. Souriau, Mod `ele de particule `a spin dans le champ ´electromagn´etique et gravitationnel, Ann. Inst. Henri Poincar´e A20, 315 (1974)
1974
-
[15]
Mashhoon, Massless spinning test particles in a gravitational field, Ann
B. Mashhoon, Massless spinning test particles in a gravitational field, Ann. Phys.89, 254 (1975)
1975
-
[16]
Saturnini, Un mod`ele de particule `a spin de masse nulle dans le champ de gravitation,
P. Saturnini, Un mod`ele de particule `a spin de masse nulle dans le champ de gravitation,
-
[17]
Bailyn and S
M. Bailyn and S. Ragusa, Pole-dipole model of massless parti- cles, Phys. Rev. D15, 3543 (1977)
1977
-
[18]
Bailyn and S
M. Bailyn and S. Ragusa, Pole-dipole model of massless parti- cles. II, Phys. Rev. D23, 1258 (1981)
1981
-
[19]
O. Semer ´ak, Spinning particles in vacuum spacetimes of dif- ferent curvature types: Natural reference tetrads and massless particles, Phys. Rev. D92, 124036 (2015). arXiv:1512.06253 [gr-qc] (2015)
Pith/arXiv arXiv 2015
-
[20]
A. A. Deriglazov and W. Guzm ´an Ram ´ırez, Mathisson– Papapetrou–Tulczyjew–Dixon equations in ultra-relativistic regime and gravimagnetic moment, Int. J. Mod. Phys. D26, 1750047 (2017). arXiv:1509.05357 [gr-qc] (2015)
Pith/arXiv arXiv 2017
-
[21]
Mathisson, Neue Mechanik materieller Systeme, Acta Phys
M. Mathisson, Neue Mechanik materieller Systeme, Acta Phys. Pol.6, 163 (1937)
1937
-
[22]
Papapetrou, Spinning test-particles in general relativity
A. Papapetrou, Spinning test-particles in general relativity. I, Proc. Roy. Soc. Lond. A209, 248 (1951)
1951
-
[23]
W. G. Dixon, Dynamics of extended bodies in general relativity. I. Momentum and angular momentum, Proc. Roy. Soc. Lond. A 314, 499 (1970)
1970
-
[24]
W. G. Dixon, Dynamics of extended bodies in general relativity III. Equations of motion, Phil. Trans. Roy. Soc. Lond. A277, 59 (1974)
1974
-
[25]
DeWitt and S
B. DeWitt and S. M. Christensen (Ed.), Bryce DeWitt’s Lectures on Gravitation (Springer, Berlin, Heidelberg, 2011)
2011
-
[26]
J. Steinhoff, Spin and Quadrupole Contributions to the Motion of Astrophysical Binaries in Equations of Motion in Relativis- tic Gravity (Springer, Cham, 2015). arXiv:1412.3251 [gr-qc] (2014)
arXiv 2015
-
[27]
V . A. Sharafutdinov, Integral Geometry of Tensor Fields (De Gruyter, Berlin, New York, 1994)
1994
-
[28]
M. Cariglia, V . P. Frolov, P. Krtouˇs, and D. Kubizˇn´ak, Geometry of Lax pairs: Particle motion and Killing-Yano tensors, Phys. Rev. D87, 024002 (2013). arXiv:1210.3079 [math-ph] (2012)
Pith/arXiv arXiv 2013
-
[29]
L. Anderssonet al., Pseudodifferential Weyl calculus on vector bundles, arXiv:2507.11965 [math-ph] (2025)
arXiv 2025
-
[30]
Steinhoff, Canonical formulation of spin in general relativity, Ann
J. Steinhoff, Canonical formulation of spin in general relativity, Ann. Phys. (Berlin)523, 296 (2011). arXiv:1106.4203 [gr-qc] (2011)
Pith/arXiv arXiv 2011
-
[31]
Tulczyjew, Motion of Multipole Particles in General Relativ- ity Theory, Acta Phys
W. Tulczyjew, Motion of Multipole Particles in General Relativ- ity Theory, Acta Phys. Pol.18, 393 (1959)
1959
-
[32]
F. A. E. Pirani, On the Physical Significance of the Riemann Tensor, Acta Phys. Pol.15, 389 (1956)
1956
-
[33]
Ohashi, Multipole particle in relativity, Phys
A. Ohashi, Multipole particle in relativity, Phys. Rev. D68, 044009 (2003). arXiv:gr-qc/0306062 [gr-qc] (2003)
Pith/arXiv arXiv 2003
-
[34]
Kyrian and O
K. Kyrian and O. Semer´ak, Spinning test particles in a Kerr field – II, Mon. Not. R. Astron. Soc.382, 1922 (2007)
1922
-
[35]
L. F. O. Costa and J. Nat´ario, Center of Mass, Spin Supplemen- tary Conditions, and the Momentum of Spinning Particles in Equations of Motion in Relativistic Gravity (Springer, Cham, 2015). arXiv:1410.6443 [gr-qc] (2014)
Pith/arXiv arXiv 2015
-
[36]
H. Bauke, S. Ahrens, C. H. Keitel, and R. Grobe, Relativistic spin operators in various electromagnetic environments, Phys. Rev. A89, 052101 (2014). arXiv:1403.0550 [quant-ph] (2014)
Pith/arXiv arXiv 2014
-
[37]
D. R. Terno, Localization of relativistic particles and uncertainty relations, Phys. Rev. A89, 042111 (2014). arXiv:1308.0479 [hep-th] (2013)
Pith/arXiv arXiv 2014
-
[38]
L. C. C´eleri, V . Kiosses, and D. R. Terno, Spin and localization of relativistic fermions and uncertainty relations, Phys. Rev. A 94, 062115 (2016). arXiv:1607.00123 [hep-th] (2016)
Pith/arXiv arXiv 2016
-
[39]
C. De Rosa and V . Moretti, Quantum particle localization ob- servables on Cauchy surfaces of Minkowski spacetime and their causal properties, Lett. Math. Phys.114, 72 (2024). arXiv:2402.13894 [math-ph] (2024)
arXiv 2024
-
[40]
E. Barausse, E. Racine, and A. Buonanno, Hamiltonian of a spinning test particle in curved spacetime, Phys. Rev. D80, 104025 (2009). arXiv:0907.4745 [gr-qc] (2009). Erratum: Phys. Rev. D85, 069904 (2012)
Pith/arXiv arXiv 2009
-
[41]
A. J. Hanson and T. Regge, The relativistic spherical top, Ann. Phys.87, 498 (1974)
1974
-
[42]
R. A. Porto, Post-Newtonian corrections to the motion of spin- ning bodies in nonrelativistic general relativity, Phys. Rev. D73, 104031 (2006). arXiv:gr-qc/0511061 [gr-qc] (2005)
Pith/arXiv arXiv 2006
-
[43]
Newman and R
E. Newman and R. Penrose, An Approach to Gravitational Ra- diation by a Method of Spin Coefficients, J. Math. Phys.3, 566 (1962)
1962
-
[44]
Chandrasekhar, The Mathematical Theory of Black Holes (Oxford University Press, Oxford, 1992)
S. Chandrasekhar, The Mathematical Theory of Black Holes (Oxford University Press, Oxford, 1992)
1992
-
[45]
S. Murk, D. R. Terno, and R. Vadapalli, Gravity-induced bire- fringence in spherically symmetric spacetimes, Phys. Rev. D 111, 044001 (2025). arXiv:2408.02729 [gr-qc] (2024)
arXiv 2025
-
[46]
L. Andersson, F. Gray, and M. A. Oancea, Conserved quanti- ties and integrability for massless spinning particles in general relativity, Phys. Rev. D113, 064061 (2026). arXiv:2512.07677 [gr-qc] (2025)
arXiv 2026
-
[47]
M. A. Oancea and A. Kumar, Semiclassical analysis of Dirac fields on curved spacetime, Phys. Rev. D107, 044029 (2023). arXiv:2212.04414 [gr-qc] (2022). 10
arXiv 2023
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.