Hamiltonian analysis of ModMax nonlinear electrodynamics in the first-order formalism

Author:

Escobar C. A.1ORCID,Linares Román1,Tlatelpa-Mascote B.1

Affiliation:

1. Departamento de Física, Universidad Autónoma Metropolitana-Iztapalapa, San Rafael Atlixco 186, 09340 Ciudad de México, México

Abstract

In this work, we study the so-called ModMax nonlinear electrodynamics, which is a novel model designed to preserve duality rotations and conformal transformations, such as the Maxwell’s equations do. This model allows to study diverse gravitational phenomena when it is coupled to General Relativity, in particular charged black holes and gravitational waves. In this work, we focus in the dynamics and Hamiltonian analysis of the model. Specifically, we analyze the propagation of the discontinuities of the field and obtain the corresponding dispersion relations. To perform the Hamiltonian analysis we adopt the first-order formalism develop by Plebański and follow the Dirac method for theories with constraints. We derive the effective Hamiltonian, classify all the constraints and identify the degrees of freedom. We prove that the effective Hamiltonian is strictly bounded from below and investigate the existence of nontrivial minima.

Funder

PAPIIT

Publisher

World Scientific Pub Co Pte Ltd

Subject

Astronomy and Astrophysics,Nuclear and High Energy Physics,Atomic and Molecular Physics, and Optics

Cited by 12 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. Flows in the space of interacting chiral boson theories;Physical Review D;2024-08-05

2. Thermal Aspects and Joule–Thomson Expansion of ModMax Black Hole;The European Physical Journal Plus;2024-05-29

3. Analysis of Dyonic ModMax black hole through accretion disk;The European Physical Journal C;2024-05-04

4. Nearly static magnetized Kerr black-hole in nonlinear electrodynamics;International Journal of Modern Physics A;2023-10-10

5. $$\sqrt{T\overline{T}}$$-deformed oscillator inspired by ModMax;The European Physical Journal Plus;2023-02-02

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