Reply to "Revisiting the solution of the second-class constraints of the Holst action"
F. Cianfrani, G. Montani

TL;DR
This paper provides a response to previous critiques regarding the handling of second-class constraints in the Holst action, clarifying the authors' approach and addressing concerns raised in earlier work.
Contribution
It offers a detailed rebuttal and clarification of the authors' method for solving second-class constraints in the Holst action, advancing understanding in this area.
Findings
Clarifies the authors' approach to second-class constraints
Addresses and refutes previous critiques
Strengthens the theoretical foundation of the Holst action
Abstract
Reply to arXiv:1903.09201.
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Taxonomy
TopicsQuantum chaos and dynamical systems · Control and Stability of Dynamical Systems
Reply to “Revisiting the solution of the second-class constraints of the Holst action”
Francesco Cianfrani1, Giovanni Montani23
[email protected]; [email protected]
1 University of Rome Tor Vergata, Department of Industrial Engineering, Via del Politecnico 1, Rome 00133, Italy
2 ENEA, Fusion and Nuclear Safety Department, C. R. Frascati, Via E. Fermi 45, 00044 Frascati (Roma), Italy
3 Physics Department, “Sapienza” University of Rome, P.le Aldo Moro 5, 00185 Roma (Italy)
Abstract
Reply to arXiv:1903.09201.
pacs:
04.60.Pp, 11.30.Cp
The authors of Montesinos:2019ypp completely misunderstood the results of our manuscript Cianfrani:2008zv . They claim that we “provided a certain parametrization of the solution of the second-class constraints resulting in a noncanonical symplectic structure (for which they also asserted to have found canonical variables). Nevertheless, such a symplectic structure is incorrect because it involves 21 variables and thus does not give the right count of the local degrees of freedom (d.o.f.) of general relativity.”
Indeed, we provided a parametrization of the phase space in terms of 24 variables, so providing the right number of degrees of freedom of General Relativity. These variables are:
- •
the connections and their conjugate momenta , that reduce to Ashtekar-Barbero connections and inverse densitized triads in the time-gauge,
- •
the boost variables and their conjugate momenta .
This is clear by looking at Eq.(12) of the paper, in which the action is written in terms of these variables.
Therefore, the motivation for the analysis given in Montesinos:2019ypp is inconsistent.
The reference list from the paper itself. Each links out to its DOI / PubMed record.
- 1(1) M. Montesinos, J. Romero and M. Celada, Phys. Rev. D 99 , no. 6, 064029 (2019)
- 2(2) F. Cianfrani and G. Montani, Phys. Rev. Lett. 102 , 091301 (2009)
