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Faddeev–Jackiw Hamiltonian formulation for general exotic bi-gravity
by
Rodríguez-Tzompantzi, Omar
in
Astronomy
/ Astrophysics and Cosmology
/ Elementary Particles
/ Gravity
/ Hadrons
/ Heavy Ions
/ Measurement Science and Instrumentation
/ Nuclear Energy
/ Nuclear Physics
/ Physics
/ Physics and Astronomy
/ Quantum Field Theories
/ Quantum Field Theory
/ Regular Article - Theoretical Physics
/ String Theory
2024
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Faddeev–Jackiw Hamiltonian formulation for general exotic bi-gravity
by
Rodríguez-Tzompantzi, Omar
in
Astronomy
/ Astrophysics and Cosmology
/ Elementary Particles
/ Gravity
/ Hadrons
/ Heavy Ions
/ Measurement Science and Instrumentation
/ Nuclear Energy
/ Nuclear Physics
/ Physics
/ Physics and Astronomy
/ Quantum Field Theories
/ Quantum Field Theory
/ Regular Article - Theoretical Physics
/ String Theory
2024
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Do you wish to request the book?
Faddeev–Jackiw Hamiltonian formulation for general exotic bi-gravity
by
Rodríguez-Tzompantzi, Omar
in
Astronomy
/ Astrophysics and Cosmology
/ Elementary Particles
/ Gravity
/ Hadrons
/ Heavy Ions
/ Measurement Science and Instrumentation
/ Nuclear Energy
/ Nuclear Physics
/ Physics
/ Physics and Astronomy
/ Quantum Field Theories
/ Quantum Field Theory
/ Regular Article - Theoretical Physics
/ String Theory
2024
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Faddeev–Jackiw Hamiltonian formulation for general exotic bi-gravity
Journal Article
Faddeev–Jackiw Hamiltonian formulation for general exotic bi-gravity
2024
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Overview
General exotic bi-gravity, obtained in Ozkan et al. (Phys Rev Lett 123(3):031303, 2019), is a unitary parity-preserving model which describes two interacting spin-two fields in three-dimensional spacetime. Adopting a symplectic viewpoint, we investigate the dynamical structure of general exotic bi-gravity theory. In particular, by exploiting the properties of the corresponding pre-symplectic matrix and its associated zero-modes, we explicitly derive all constraints of the theory, including the integrability conditions and scalar relationships between all the parameters and fields defining the model. Then, as an application, these scalar relationships are used for studying the anti-de Sitter background. After that, we derive the gauge transformations for the dynamical variables from the structure of the remaining zero-modes, meaning that such zero-modes are indeed the generators of the gauge symmetry of the theory. Finally, by switching off one of the four coupling constants
β
n
and assuming the invertibility of some of the dreibeins, we find that the general exotic bi-gravity theory has two physical degrees of freedom.
Publisher
Springer Berlin Heidelberg,Springer,Springer Nature B.V,SpringerOpen
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