Javascript must be enabled to continue!
An exact dyonic black hole at the integrable locus of quadratic nonlinear electrodynamics
View through CrossRef
In the quadratic nonlinear electrodynamics $-F+aF^{2}+bG^{2}$, dyonic black holes are known in closed form only when $a=0$, because the electric field solves a cubic whose coefficients carry the radius. We identify the locus $b=a/2$, where that dependence cancels, the magnetic charge decouples from the constitutive relation, and the field equations integrate exactly. Trading the areal radius for the field strength then gives an exact dyonic solution, the radial quadrature evaluating to Gauss hypergeometric functions, with the cosmological constant retained. It recovers the dyonic Reissner--Nordstr\"om, magnetic and Euler--Heisenberg branches, and at first order resums the perturbative dyonic lapse function, whose symmetry under interchange of the charges breaks at second order. The horizon structure contains a window of three horizons requiring both charges. The same change of variable renders the electric Smarr integral, previously stated to have no closed form, hypergeometric. Closed forms for the density and pressures show the electric charge enlarging the region where the dominant energy condition holds beyond the magnetic bound $\rH^{4}>4ap^{2}$; three curvature laws arise at the centre, one a relegated singularity. The extended thermodynamics closes with the coupling and pressure as variables, and the critical ratio falls below the Maxwell value $3/8$. The two photon cones split the shadow into a doublet reaching half a percent, while the geodesic light ring and scalar ringdown stay almost blind to the coupling.
Title: An exact dyonic black hole at the integrable locus of quadratic nonlinear electrodynamics
Description:
In the quadratic nonlinear electrodynamics $-F+aF^{2}+bG^{2}$, dyonic black holes are known in closed form only when $a=0$, because the electric field solves a cubic whose coefficients carry the radius.
We identify the locus $b=a/2$, where that dependence cancels, the magnetic charge decouples from the constitutive relation, and the field equations integrate exactly.
Trading the areal radius for the field strength then gives an exact dyonic solution, the radial quadrature evaluating to Gauss hypergeometric functions, with the cosmological constant retained.
It recovers the dyonic Reissner--Nordstr\"om, magnetic and Euler--Heisenberg branches, and at first order resums the perturbative dyonic lapse function, whose symmetry under interchange of the charges breaks at second order.
The horizon structure contains a window of three horizons requiring both charges.
The same change of variable renders the electric Smarr integral, previously stated to have no closed form, hypergeometric.
Closed forms for the density and pressures show the electric charge enlarging the region where the dominant energy condition holds beyond the magnetic bound $\rH^{4}>4ap^{2}$; three curvature laws arise at the centre, one a relegated singularity.
The extended thermodynamics closes with the coupling and pressure as variables, and the critical ratio falls below the Maxwell value $3/8$.
The two photon cones split the shadow into a doublet reaching half a percent, while the geodesic light ring and scalar ringdown stay almost blind to the coupling.
Related Results
On Flores Island, do "ape-men" still exist? https://www.sapiens.org/biology/flores-island-ape-men/
On Flores Island, do "ape-men" still exist? https://www.sapiens.org/biology/flores-island-ape-men/
<span style="font-size:11pt"><span style="background:#f9f9f4"><span style="line-height:normal"><span style="font-family:Calibri,sans-serif"><b><spa...
An exact dyonic black hole at the integrable locus of quadratic nonlinear electrodynamics
An exact dyonic black hole at the integrable locus of quadratic nonlinear electrodynamics
In the quadratic nonlinear electrodynamics $-F+aF^{2}+bG^{2}$, dyonic black holes are known in closed form only when $a=0$, because the electric field solves a cubic whose coeffici...
Revisiting chronology protection conjecture in the Dyonic Kerr–Sen black hole spacetime
Revisiting chronology protection conjecture in the Dyonic Kerr–Sen black hole spacetime
Abstract
The chronology protection conjecture (CPC) was first introduced by Hawking after his semi-classical investigation of the behaviour of a spacetime with cl...
Progress in Surface Theory
Progress in Surface Theory
The workshop
Progress in Surface Theory
, organised by Uwe Abresch (Bochum), Josef Dorfmeister (München), and Masaaki Umehara (Osaka) was he...
Development and Analysis of Novel Integrable Nonlinear Dynamical Systems on Quasi-One-Dimensional Lattices. Two-Component Nonlinear System with the On-Site and Spatially Distributed Inertial Mass Parameters
Development and Analysis of Novel Integrable Nonlinear Dynamical Systems on Quasi-One-Dimensional Lattices. Two-Component Nonlinear System with the On-Site and Spatially Distributed Inertial Mass Parameters
The main principles of developing the evolutionary nonlinear integrable systems on quasi-onedimensional lattices are formulated in clear mathematical and physical terms discarding ...
Stringy dyonic solutions and clifford structures
Stringy dyonic solutions and clifford structures
Using the toroidal compactification of string theory on [Formula: see text]-dimensional tori, [Formula: see text], we investigate dyonic objects in arbitrary dimensions. First, we ...
The Generalized Riemann Integral
The Generalized Riemann Integral
Riemann integration theory integrates functions on a bounded interval as a Riemann sum approach (integral) where the fineness of the partitions is controlled by a number (norm) of...
Theoretical study of Strong gravitational lensing around Dyonic ModMax black hole: constraints from EHT observations
Theoretical study of Strong gravitational lensing around Dyonic ModMax black hole: constraints from EHT observations
Abstract
In this study, we investigate the properties of the Dyonic ModMax black hole solution using strong gravitational lensing. Additionally, we calculate the tim...

