Primary Constraints of Newer General Relativity
Pith reviewed 2026-06-29 06:26 UTC · model grok-4.3
The pith
Newer General Relativity produces either one or two scalar primary constraints depending on the choice of Lagrangian coefficients c_i.
A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.
Core claim
In Newer General Relativity the gravitational Lagrangian is a quadratic scalar built from the nonmetricity tensor with arbitrary coefficients c_i. After computing the canonical momenta conjugate to the metric and decomposing the velocity-momenta map into fully nonlinear scalar, vector and tensor sectors, the map is found to be non-invertible in the tensor sector for five independent reasons, in the vector sector for three independent reasons, and in the scalar sector for either one or two independent reasons according to the values of the c_i. The same non-invertibility conditions characterize the primary constraints of the covariant formulation of symmetric teleparallel gravity.
What carries the argument
Non-invertibility of the velocity-momenta map after a fully nonlinear scalar-vector-tensor decomposition of the Lagrangian.
If this is right
- The tensor sector always contributes five primary constraints and the vector sector three, independent of the c_i.
- The scalar sector contributes either one or two primary constraints according to algebraic conditions on the c_i.
- The identical primary constraints appear in the covariant formulation of symmetric teleparallel gravity.
- The total number of primary constraints is therefore either nine or ten according to the parameter region.
Where Pith is reading between the lines
- Different numbers of scalar constraints will produce different final counts of physical degrees of freedom once secondary constraints are derived.
- The parameter regions that yield two scalar constraints may admit additional scalar modes that are absent when only one scalar constraint appears.
- The degeneracy condition on the c_i supplies an explicit algebraic criterion that can be used to partition the theory's parameter space before any Hamiltonian analysis begins.
Load-bearing premise
Non-invertibility of the velocity-momenta map after the nonlinear decomposition is enough to identify every primary constraint without further secondary-constraint or gauge-fixing analysis.
What would settle it
Direct computation of the rank of the Hessian matrix formed by second derivatives of the Lagrangian with respect to the metric velocities, for concrete numerical choices of the c_i that the paper predicts should produce one versus two independent scalar null eigenvectors.
read the original abstract
We study the primary constraint structure of Newer General Relativity, a gravity theory based on a torsionless teleparallel geometry. The gravitational action is built from a scalar formed by quadratic combinations of the nonmetricity tensor, with arbitrary coefficients $c_i$ in the Lagrangian. We decompose the Lagrangian and compute the canonical momenta conjugate to the metric. We characterize the primary constraints arising from these momenta by identifying when the map between velocities and momenta becomes non-invertible, and organize the outcome through a fully nonlinear decomposition into scalar, vector and tensor sectors. Comparing with previous results in the literature, we recover five and three primary constraints associated with the tensor and vector sectors, respectively. We also identify a previously unreported degeneracy in the scalar sector, which yields either one or two scalar primary constraints depending on the conditions imposed on the parameters $c_i$. Finally, we obtain the primary constraints associated with the covariant formulation of symmetric teleparallel gravity.
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. The paper analyzes the primary constraint structure of Newer General Relativity, a torsionless teleparallel theory whose action is quadratic in the nonmetricity tensor with free coefficients c_i. After a fully nonlinear SVT decomposition of the Lagrangian and computation of the canonical momenta, the authors identify non-invertibility of the velocity-momenta map to obtain five tensor primary constraints and three vector primary constraints; they further report a previously unreported degeneracy in the scalar sector that produces either one or two scalar primary constraints depending on the values of the c_i. The same procedure is applied to the covariant formulation of symmetric teleparallel gravity.
Significance. If the results hold, the work supplies a concrete count of primary constraints in a broad class of quadratic nonmetricity theories, which is a necessary step toward determining the physical degrees of freedom. The identification of a parameter-dependent scalar-sector degeneracy is a novel contribution that distinguishes the analysis from earlier literature on teleparallel gravity. The use of a fully nonlinear decomposition, rather than a linearized one, is a methodological strength that supports the robustness of the reported counts.
minor comments (2)
- [Abstract] The abstract states that the scalar degeneracy depends on conditions imposed on the c_i but does not list the explicit conditions; adding a brief parenthetical statement of those conditions would improve immediate readability.
- [Introduction] The comparison with previous literature is described qualitatively; a short table or paragraph explicitly mapping the recovered tensor and vector counts to the corresponding references would make the validation step more transparent.
Simulated Author's Rebuttal
We thank the referee for their careful reading of the manuscript and for recommending acceptance. Their summary correctly reflects the scope and results of our analysis.
Circularity Check
No significant circularity identified
full rationale
The paper follows the standard procedure for primary constraints in the Hamiltonian formalism: it decomposes the Lagrangian into SVT sectors, computes the canonical momenta from the quadratic nonmetricity action with parameters c_i, and identifies constraints from non-invertibility of the velocity-momenta map. It recovers the expected five tensor and three vector constraints from prior literature and reports a parameter-dependent degeneracy in the scalar sector. No derivation step reduces by construction to a self-defined quantity, fitted input, or load-bearing self-citation; the central claims rest on direct computation rather than renaming or ansatz smuggling. The analysis is self-contained against external benchmarks for counting primary constraints.
Axiom & Free-Parameter Ledger
free parameters (1)
- c_i
axioms (1)
- domain assumption The gravitational action is built from a scalar formed by quadratic combinations of the nonmetricity tensor
Reference graph
Works this paper leans on
-
[1]
Will.Theory and Experiment in Gravitational Physics
Clifford M. Will.Theory and Experiment in Gravitational Physics. Cambridge Uni- versity Press, 1993
1993
-
[2]
Solar-system tests of the relativistic gravity.Int
Wei-Tou Ni. Solar-system tests of the relativistic gravity.Int. J. Mod. Phys. D, 25(14):1630003, 2016
2016
-
[3]
Testing general relativity in the solar system: present and future perspectives.Class
Fabrizio De Marchi and Gael Cascioli. Testing general relativity in the solar system: present and future perspectives.Class. Quant. Grav., 37(9):095007, 2020
2020
-
[4]
B. P. Abbott et al. GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral.Phys. Rev. Lett., 119(16):161101, 2017
2017
-
[5]
The population of merging compact binaries inferred using gravitational waves through GWTC-3
R. Abbott et al. The population of merging compact binaries inferred using gravita- tional waves through GWTC-3. 2021. arXiv:2111.03634 [astro-ph.HE]
work page internal anchor Pith review Pith/arXiv arXiv 2021
-
[6]
R. Abbott et al. GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run. 2021. arXiv:2111.03606 [gr-qc]
work page internal anchor Pith review Pith/arXiv arXiv 2021
-
[7]
Ingrid H. Stairs. Testing General Relativity with Pulsar Timing.Living Rev. Rel., 6(1):5, 2003
2003
-
[8]
Kramer, I
M. Kramer, I. H. Stairs, R. N. Manchester, N. Wex, A. T. Deller, W. A. Coles, M. Ali, M. Burgay, F. Camilo, I. Cognard, T. Damour, G. Desvignes, R. D. Ferdman, P. C. C. Freire, S. Grondin, L. Guillemot, G. B. Hobbs, G. Janssen, R. Karuppusamy, D. R. Lorimer, A. G. Lyne, J. W. McKee, M. McLaughlin, L. E. M¨ unch, B. B. P. Perera, N. Pol, A. Possenti, J. Sa...
2021
-
[9]
Bonola.Non-Euclidean Geometry: A Critical and Historical Study of Its Develop- ment
R. Bonola.Non-Euclidean Geometry: A Critical and Historical Study of Its Develop- ment. Dover Books on Mathematics Series. Dover Publications, 1955
1955
-
[10]
M. K. Bennett.Affine and Projective Geometry. Wiley, 2011
2011
-
[11]
Clifton.Alternative Theories of Gravity
T. Clifton.Alternative Theories of Gravity. PhD thesis, -, 2006
2006
-
[12]
Thomas P. Sotiriou and Valerio Faraoni.f(R) theories of gravity.Rev. Mod. Phys., 82(1):451–497, 2010. arXiv:0805.1726 [gr-qc]. May 29, 2026 1:42 01˙main-ijgmmp 30
work page internal anchor Pith review Pith/arXiv arXiv 2010
-
[13]
Extended geometric trinity of gravity.Eur
Salvatore Capozziello, Sara Cesare, and Carmen Ferrara. Extended geometric trinity of gravity.Eur. Phys. J. C, 85(9):932, 2025. arXiv:2503.08167 [gr-qc]
-
[14]
’t Hooft and M
G. ’t Hooft and M. Veltman. One-loop divergencies in the theory of gravitation.Ann. Inst. H. Poincare Phys. Theor., 20(1):69–94, 1974
1974
-
[15]
Yuri N. Obukhov. Gravitational waves in Poincar´ e gauge gravity theory.Phys. Rev. D, 95(8):084028, 2017
2017
-
[16]
Springer, 2003
Domenico Giulini, Claus Kiefer, and Claus Laemmerzahl.Quantum Gravity: From Theory to Experimental Search, volume 631. Springer, 2003
2003
-
[17]
Cambridge Monographs on Mathematical Physics
Carlo Rovelli.Quantum Gravity. Cambridge Monographs on Mathematical Physics. Cambridge University Press, Cambridge, 2004
2004
-
[18]
Challenges for $\Lambda$CDM: An update
Leandros Perivolaropoulos and Foteini Skara. Challenges for ΛCDM: An update.New Astron. Rev., 95:101659, 2022. arXiv:2105.05208 [astro-ph.CO]
work page internal anchor Pith review Pith/arXiv arXiv 2022
-
[19]
A. G. Adame et al. DESI 2024 VI: cosmological constraints from the measurements of baryon acoustic oscillations.JCAP, 02:021, 2025. arXiv:2404.03002 [astro-ph.CO]
work page internal anchor Pith review Pith/arXiv arXiv 2024
-
[20]
A review of the discovery reach of directional Dark Matter detection
F. Mayet et al. A review of the discovery reach of directional Dark Matter detection. Phys. Rept., 627:1–49, 2016. arXiv:1602.03781 [astro-ph.CO]
work page internal anchor Pith review Pith/arXiv arXiv 2016
-
[21]
Addressing the missing matter problem in galaxies through a new fundamental gravitational radius
S. Capozziello, P. Jovanovi´ c, V. Borka Jovanovi´ c, and D. Borka. Addressing the missing matter problem in galaxies through a new fundamental gravitational radius. JCAP, 06:044, 2017. arXiv:1702.03430 [gr-qc]
work page internal anchor Pith review Pith/arXiv arXiv 2017
-
[22]
Kenath Arun, S. B. Gudennavar, and C. Sivaram. Dark matter, dark energy, and alternate models: A review.Adv. Space Res., 60(1):166–186, 2017
2017
- [23]
-
[24]
Planck 2018 results. VI. Cosmological parameters
N. Aghanim et al. Planck 2018 results. VI. Cosmological parameters.Astron. Astro- phys., 641:A6, 2020. arXiv:1807.06209 [astro-ph.CO]. [Erratum: Astron. Astrophys. 652, C4 (2021)]
work page internal anchor Pith review Pith/arXiv arXiv 2018
-
[25]
Alan H. Guth and David I. Kaiser. Inflationary cosmology: Exploring the Universe from the smallest to the largest scales.Science, 307:884–890, 2005. arXiv:astro- ph/0502328
-
[26]
A Step in understanding the Hubble tension.Phys
Daniel Aloni, Asher Berlin, Melissa Joseph, Martin Schmaltz, and Neal Weiner. A Step in understanding the Hubble tension.Phys. Rev. D, 105(12):123516, 2022. arXiv:2111.00014 [astro-ph.CO]
-
[27]
Mota, Adam G
Eleonora Di Valentino, Olga Mena, Supriya Pan, Luca Visinelli, Weiqiang Yang, Alessandro Melchiorri, David F. Mota, Adam G. Riess, and Joseph Silk. In the realm of the Hubble tension—a review of solutions.Class. Quant. Grav., 38(15):153001,
-
[28]
arXiv:2103.01183 [astro-ph.CO]
work page internal anchor Pith review Pith/arXiv arXiv
-
[29]
Status of theS 8 Tension: A 2026 Review of Probe Discrepancies.Phys
Ioannis Pantos and Leandros Perivolaropoulos. Status of theS 8 Tension: A 2026 Review of Probe Discrepancies.Phys. Dark Univ., 52:102286, 2026. arXiv:2602.12238 [astro-ph.CO]
-
[30]
Palatini’s method
M. Ferraris, M. Francaviglia, and C. Reina. Variational formulation of general rela- tivity from 1915 to 1925 “Palatini’s method” discovered by Einstein in 1925.Gen. Rel. Grav., 14:243–254, 1982
1915
-
[31]
Friedrich W. Hehl, J. Dermott McCrea, Eckehard W. Mielke, and Yuval Ne’eman. Metric-affine gauge theory of gravity: field equations, Noether identities, world spinors, and breaking of dilation invariance.Phys. Rept., 258(1):1–171, 1995
1995
-
[32]
Einstein
A. Einstein. Die Grundlage der allgemeinen Relativit¨ atstheorie.Annalen Phys., 354(7):769–822, 1916
1916
- [33]
-
[34]
Springer, Dor- drecht, 2013
Ruben Aldrovandi and Jos´ e Geraldo Pereira.Teleparallel Gravity. Springer, Dor- drecht, 2013
2013
-
[35]
Symmetric teleparallel general relativity
James M. Nester and Hwei-Jang Yo. Symmetric teleparallel general relativity.Chin. J. Phys., 37:113, 1999. arXiv:gr-qc/9809049
work page internal anchor Pith review Pith/arXiv arXiv 1999
-
[36]
Jose Beltr´ an Jim´ enez, Lavinia Heisenberg, and Tomi Koivisto. Coincident General Relativity.Phys. Rev. D, 98(4):044048, 2018. arXiv:1710.03116 [gr-qc]
work page internal anchor Pith review Pith/arXiv arXiv 2018
-
[37]
New General Relativity.Phys
Kenji Hayashi and Takeshi Shirafuji. New General Relativity.Phys. Rev. D, 19:3524– 3553, 1979. [Addendum: Phys. Rev. D 24, 3312–3314 (1982)]
1979
-
[38]
Hamiltonian and primary constraints of new general relativity
Daniel Blixt, Manuel Hohmann, and Christian Pfeifer. Hamiltonian and primary con- straints of new general relativity.Phys. Rev. D, 99(8):084025, 2019. arXiv:1811.11137 [gr-qc]
work page internal anchor Pith review Pith/arXiv arXiv 2019
-
[39]
Propagation of gravitational waves in symmetric teleparallel gravity theories.Phys
Manuel Hohmann, Christian Pfeifer, Jackson Levi Said, and Ulbossyn Ualikhanova. Propagation of gravitational waves in symmetric teleparallel gravity theories.Phys. Rev. D, 99(2):024009, 2019. arXiv:1808.02894 [gr-qc]
-
[40]
Post-Newtonian limit of generalized symmet- ric teleparallel gravity.Phys
Kai Flathmann and Manuel Hohmann. Post-Newtonian limit of generalized symmet- ric teleparallel gravity.Phys. Rev. D, 103(4):044030, 2021. arXiv:2012.12875 [gr-qc]
-
[41]
Symmetric teleparallel connection and spherical solutions in symmetric teleparallel gravity.Phys
Manuel Hohmann and Vasiliki Karanasou. Symmetric teleparallel connection and spherical solutions in symmetric teleparallel gravity.Phys. Rev. D, 111(6):064057,
- [42]
-
[43]
Francesco D’Ambrosio and Lavinia Heisenberg. Classification of primary constraints of quadratic nonmetricity theories of gravity.JHEP, 02:170, 2021. arXiv:2007.05064 [gr-qc]
-
[44]
Alexey Golovnev, Sofia Klimova, Alla N. Semenova, and Vyacheslav P. Van- deev. Weak Gravity Limit in Newer General Relativity.Universe, 11(5):149, 2025. arXiv:2501.00376 [gr-qc]
-
[45]
Dynamical systems approach and cos- mological attractors in newer general relativity.Eur
Manuel Hohmann and Ulbossyn Ualikhanova. Dynamical systems approach and cos- mological attractors in newer general relativity.Eur. Phys. J. C, 85(10):1163, 2025. arXiv:2505.16917 [gr-qc]
-
[46]
Post-Newtonian limit of generalized scalar-teleparallel theories of gravity.Phys
Manuel Hohmann and Ulbossyn Ualikhanova. Post-Newtonian limit of generalized scalar-teleparallel theories of gravity.Phys. Rev. D, 109(4):044070, 2024
2024
-
[47]
Ver´ onica Errasti D´ ıez, Markus Maier, and Julio A. M´ endez-Zavaleta. Constraint char- acterization and degree of freedom counting in Lagrangian field theory.Phys. Rev. D, 109(2):025010, 2024. arXiv:2310.12218 [hep-th]
-
[48]
Foundations of Ghost Stability.Fortsch
Ver´ onica Errasti D´ ıez, Jordi Gaset Rif` a, and Georgina Staudt. Foundations of Ghost Stability.Fortsch. Phys., 73(4):2400268, 2025. arXiv:2408.16832 [hep-th]
-
[49]
Degrees of freedom of $f(T)$ gravity
Miao Li, Rong-Xin Miao, and Yan-Gang Miao. Degrees of freedom off(T) gravity. JHEP, 07:108, 2011. arXiv:1105.5934 [hep-th]
work page internal anchor Pith review Pith/arXiv arXiv 2011
-
[50]
Quest for the extra degree of freedom in f(T) gravity
Rafael Ferraro and Mar´ ıa Jos´ e Guzm´ an. Quest for the extra degree of freedom in f(T) gravity.Phys. Rev. D, 98(12):124037, 2018. arXiv:1810.07171 [gr-qc]
work page internal anchor Pith review Pith/arXiv arXiv 2018
-
[51]
Degrees of freedom and Hamiltonian formalism forf(T) gravity.Int
Mar´ ıa Jos´ e Guzm´ an and Rafael Ferraro. Degrees of freedom and Hamiltonian formalism forf(T) gravity.Int. J. Mod. Phys. A, 35(02n03):2040022, 2020. arXiv:1910.03100 [gr-qc]
-
[52]
Pseudoinvariance and the extra degree of freedom inf(T) gravity.Phys
Rafael Ferraro and Mar´ ıa Jos´ e Guzm´ an. Pseudoinvariance and the extra degree of freedom inf(T) gravity.Phys. Rev. D, 101(8):084017, 2020. arXiv:2001.08137 [gr-qc]
- [53]
-
[54]
Nontrivial Minkowski backgrounds in f(T) gravity.Phys
Alexey Golovnev and Mar´ ıa Jos´ e Guzm´ an. Nontrivial Minkowski backgrounds in f(T) gravity.Phys. Rev. D, 103(4):044009, 2021. arXiv:2012.00696 [gr-qc]
-
[55]
Foundational issues inf(T) gravity the- May 29, 2026 1:42 01˙main-ijgmmp 32 ory.Int
Alexey Golovnev and Mar´ ıa-Jos´ e Guzm´ an. Foundational issues inf(T) gravity the- May 29, 2026 1:42 01˙main-ijgmmp 32 ory.Int. J. Geom. Meth. Mod. Phys., 18(supp01):2140007, 2021. arXiv:2012.14408 [gr-qc]
-
[56]
M´ endez-Zavaleta, and Mojtaba Taslimi Tehrani
Ver´ onica Errasti D´ ıez, Markus Maier, Julio A. M´ endez-Zavaleta, and Mojtaba Taslimi Tehrani. Lagrangian constraint analysis of first-order classical field theories with an application to gravity.Phys. Rev. D, 102:065015, 2020. arXiv:2007.11020 [hep-th]
-
[57]
Disformal transformations in modified teleparallel gravity.Symmetry, 12(1):152, 2020
Alexey Golovnev and Mar´ ıa Jos´ e Guzm´ an. Disformal transformations in modified teleparallel gravity.Symmetry, 12(1):152, 2020. arXiv:1912.04604 [gr-qc]
-
[58]
Primary constraints in general teleparallel quadratic gravity.Phys
Francesco Bajardi and David Blixt. Primary constraints in general teleparallel quadratic gravity.Phys. Rev. D, 109(8):084078, 2024. arXiv:2401.11591 [gr-qc]
-
[59]
A Solution to Symmetric Teleparallel Gravity
Muzaffer Adak and Ozcan Sert. A Solution to symmetric teleparallel gravity.Turk. J. Phys., 29:1–7, 2005. arXiv:gr-qc/0412007
work page internal anchor Pith review Pith/arXiv arXiv 2005
-
[60]
Lagrange formulation of the symmetric teleparallel gravity
Muzaffer Adak, M. Kalay, and Ozcan Sert. Lagrange formulation of the symmetric teleparallel gravity.Int. J. Mod. Phys. D, 15:619–634, 2006. arXiv:gr-qc/0505025
work page internal anchor Pith review Pith/arXiv arXiv 2006
-
[61]
The Symmetric Teleparallel Gravity
Muzaffer Adak. The Symmetric teleparallel gravity.Turk. J. Phys., 30:379–390, 2006. arXiv:gr-qc/0611077
work page internal anchor Pith review Pith/arXiv arXiv 2006
-
[62]
The early history of symmetric teleparallel gravity: An overlooked period
Muzaffer Adak. The early history of symmetric teleparallel gravity: An overlooked period. 2026. arXiv:2602.19194 [gr-qc]
-
[63]
Comparing equiva- lent gravities: common features and differences.Eur
Salvatore Capozziello, Vittorio De Falco, and Carmen Ferrara. Comparing equiva- lent gravities: common features and differences.Eur. Phys. J. C, 82(10):865, 2022. arXiv:2208.03011 [gr-qc]
-
[64]
Hamiltonian formulation of teleparallel gravity
Rafael Ferraro and Mar´ ıa Jos´ e Guzm´ an. Hamiltonian formulation of teleparallel grav- ity.Phys. Rev. D, 94(10):104045, 2016. arXiv:1609.06766 [gr-qc]
work page internal anchor Pith review Pith/arXiv arXiv 2016
-
[65]
Hamiltonian formalism for f(T) gravity
Rafael Ferraro and Mar´ ıa Jos´ e Guzm´ an. Hamiltonian formalism forf(T) gravity. Phys. Rev. D, 97(10):104028, 2018. arXiv:1802.02130 [gr-qc]
work page internal anchor Pith review Pith/arXiv arXiv 2018
-
[66]
Classification of primary con- straints for new general relativity in the premetric approach.Int
Mar´ ıa Jos´ e Guzm´ an and Shymaa Khaled Ibraheem. Classification of primary con- straints for new general relativity in the premetric approach.Int. J. Geom. Meth. Mod. Phys., 18(supp01):2140003, 2021. arXiv:2009.13430 [gr-qc]
-
[67]
Ge- ometry and covariance of symmetric teleparallel theories of gravity.Phys
Daniel Blixt, Alexey Golovnev, Mar´ ıa Jos´ e Guzm´ an, and Ramazan Maksyutov. Ge- ometry and covariance of symmetric teleparallel theories of gravity.Phys. Rev. D, 109(4):044061, 2024. arXiv:2306.09289 [gr-qc]
-
[68]
International Series of Monographs on Physics
Miguel Alcubierre.Introduction to 3+1 Numerical Relativity. International Series of Monographs on Physics. Oxford University Press, Oxford, 2008
2008
-
[69]
The Hamiltonian formulation of General Relativity: myths and reality
N. Kiriushcheva and S. V. Kuzmin. The Hamiltonian formulation of General Rela- tivity: Myths and reality.Central Eur. J. Phys., 9:576–615, 2011. arXiv:0809.0097 [gr-qc]
work page internal anchor Pith review Pith/arXiv arXiv 2011
- [70]
-
[71]
G. Darboux. On a proposition relative to linear equations. 1999. arXiv:physics/9908003 [physics.hist- ph]
work page internal anchor Pith review Pith/arXiv arXiv 1999
-
[72]
Alexey Golovnev. On the Role of Constraints and Degrees of Freedom in the Hamil- tonian Formalism.Universe, 9(2):101, 2023. arXiv:2212.11260 [hep-th]
-
[73]
Prokhorov and Sergei V
Lev V. Prokhorov and Sergei V. Shabanov.Hamiltonian mechanics of gauge systems. Cambridge Monographs on Mathematical Physics. Cambridge University Press, 2011
2011
-
[74]
J´ anos Bogn´ ar.Indefinite Inner Product Spaces, volume 78 ofErgebnisse der Mathe- matik und ihrer Grenzgebiete. 2. Folge. Springer, Berlin, Heidelberg, 1 edition, 1974
1974
-
[75]
ADM formulation and Hamiltonian analysis of Coincident General Relativity
Fabio D’Ambrosio, Mudit Garg, Lavinia Heisenberg, and Stefan Zentarra. ADM formulation and Hamiltonian analysis of Coincident General Relativity. 2020. May 29, 2026 1:42 01˙main-ijgmmp 33 arXiv:2007.03261 [gr-qc]
-
[76]
Paul A. M. Dirac. The Theory of gravitation in Hamiltonian form.Proc. Roy. Soc. Lond. A, 246:333–343, 1958
1958
-
[77]
Bello-Morales, Jose Beltr´ an Jim´ enez, Alejandro Jim´ enez Cano, Tomi S
Antonio G. Bello-Morales, Jose Beltr´ an Jim´ enez, Alejandro Jim´ enez Cano, Tomi S. Koivisto, and Antonio L. Maroto. A class of ghost-free theories in symmetric telepar- allel geometry.JHEP, 12:146, 2024. arXiv:2406.19355 [gr-qc]
-
[78]
Richard P. Woodard. Ostrogradsky’s theorem on Hamiltonian instability.Scholarpe- dia, 10(8):32243, 2015. arXiv:1506.02210 [hep-th]
work page internal anchor Pith review Pith/arXiv arXiv 2015
-
[79]
Lorentz symmetries and primary con- straints in covariant teleparallel gravity.Phys
Alexey Golovnev and Mar´ ıa Jos´ e Guzm´ an. Lorentz symmetries and primary con- straints in covariant teleparallel gravity.Phys. Rev. D, 104(12):124074, 2021. arXiv:2110.11273 [gr-qc]
-
[80]
Hamilton’s equations in the covariant teleparallel equivalent of general relativity.Phys
Laxmipriya Pati, Daniel Blixt, and Mar´ ıa-Jos´ e Guzm´ an. Hamilton’s equations in the covariant teleparallel equivalent of general relativity.Phys. Rev. D, 107(4):044071,
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.