Abstract
The paper addresses optical solitons in magneto-optic waveguides that are studied using Kudryashov’s law of nonlinear refractive index in the presence of chromatic dispersion and Hamiltonian-type perturbation terms. The trial solution approach yielded a variety of soliton solutions, which are listed in this paper.
1. Introduction
Optical soliton dynamics is an essential feature in the telecommunications industry. The current world is paralyzed without Internet activity, which means with no solitons, life comes to a pure standstill. Therefore, it is imperative to address the soliton science dynamics to the fullest extent [1,2,3,4,5,6,7,8,9]. Incidentally, it is always wise to take into account magneto-optic waveguides as opposed to regular waveguides. Such forms of waveguides are always helpful considering the data load that is transmitted across trans-continental and trans-oceanic distances. The presence of a magnetic field can loosen up the solitons from their state of clutter. This only protects the spill-over of information between the solitons when they are very close together. Thus, it is of paramount importance to address the soliton science dynamics in nonlinear optics.
Incidentally, a variety of models that have been studied in the context of magneto-optic solitons. The various forms of the non-Kerr law of nonlinearity, apart from the Kerr law itself, studied in this context are parabolic law, power law, quadratic-cubic law, dual-power law and various others. The current work addresses the same issue, but with Kudryashov’s proposed form of nonlinear refractive index [10,11,12,13,14,15]. The trial solutions approach will be implemented to secure the solitons. The analytical results are displayed, along with the respective parameter constraints, and the corresponding numerical simulations are also exhibited. The derivation and display of the solitons and their numerics are presented after an overview of the model.
Governing Model
The model equations are introduced below [10,11,12,13,14,15]:
and
where and for come from the nonlinear dispersions, while stem from the magneto-optic parameters. , , and arise from the cross-phase modulation, while emerge from the self-steepening terms. , , and yield the self-phase modulation, while give the inter-modal dispersions. x and t are the spatial and temporal variables in sequence, while stem from the chromatic dispersion. and depict the soliton wave profiles, while n comes from the full nonlinearity. Lastly, the first terms stem from the linear temporal evolution of the solitons, where .
2. Mathematical Analysis
The soliton wave profiles shape up as
where and are the soliton amplitude components, while the wave variable and soliton phase component evolve as
Here c, , and represent the velocity, frequency, wave number and phase constant in the sequence. Inserting (3) and (4) into (1) and (2), the real parts stick out as
and
while the imaginary parts stand out as
and
Equations (8) and (9) leave us with the following restrictions:
and
while Equations (10) and (12) provide the frequency
Set
Thus, Equations (6) and (7) come out as
and
Considering Equations (16) and (17), one can be addressed by the aid of the constraint relations
and
Equations (18) and (21) give way to the wave number
With this restriction, simplifies (16) to
where
We take the trial equation
then we derive
Substituting (27) and (28) into (25) and the next balancing with decreases (27) to
where
Take transformation
Rewrite Equation (32) as
where . According to Liu [16], the fourth-order complete discrimination system for the polynomial is given as
We can classify the roots of [16,17,18,19,20,21,22,23,24] and solve the integral (34).
3. Exact Solutions
(1) , then , we get the rational wave
(2) , then , we get the singular periodic wave
where and are real constants.
(3) , then , we get the singular soliton
and the dark soliton
where and are real constants.
(4) , then , we get the rational wave
where and are real constants.
(5) , then , we get the bright soliton
and the singular soliton
where , and are real constants.
(6) , then , we get the rational wave
where , and are real constants.
(7) , then , we get the snoidal periodic waves
and
where , , and are real constants, and .
(8) , then , we get the cnoidal periodic wave
where , , and are real constants, and
(9) , then , we get the combo snoidal and cnoidal periodic wave
where , , and are real constants, and
Figure 1 and Figure 2 exhibit the plots of dark and bright magneto-optic solitons (39) and (41), respectively.
Figure 1.
Surface plots of dark magneto-optic solitons (39) with , , and .
Figure 2.
Surface plots of bright magneto-optic solitons (41) with , , and .
4. Conclusions
The current paper displays solitons in magneto-optic waveguides that are studied using Kudryashov’s proposed law of refractive index. The trial solutions approach gave way to the solitons. The results are displayed, along with the numerical simulations. These results give a further insight into such waveguides with the form of self-phase modulation, as studied. These results give way to a number of future avenues of research. An immediate thought would be to handle the conservation laws. The conservation laws, when computed, would lead to further openings. The issue of quasi-monochromatic dynamics of optical solitons in a magneto-optic waveguide would subsequently follow through. The stochastically perturbed version of the model can also be pursued and studied once the conservation laws are in place. This would lead to the Langevin equations to finally depict the mean-free velocity of the soliton. Such studies are all underway and the results would be sequentially reported.
Author Contributions
Conceptualization, M.-Y.W.; methodology, A.B.; software, Y.Y.; writing—original draft preparation, L.M.; writing—review and editing, S.M.; project administration, A.A.A. All authors have read and agreed to the published version of the manuscript.
Funding
This research received no external funding.
Institutional Review Board Statement
Not applicable.
Informed Consent Statement
Not applicable.
Data Availability Statement
Not applicable.
Acknowledgments
The authors thank the anonymous referees whose comments helped to improve this paper.
Conflicts of Interest
The authors declare no conflict of interest.
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