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Article

Multi-Soliton Propagation and Interaction in Λ-Type EIT Media: An Integrable Approach

by
Ramesh Kumar Vaduganathan
1,*,
Prasanta K. Panigrahi
2,3 and
Boris A. Malomed
4,5
1
Department of Physics, Velammal Engineering College (Autonomous), Ambattur-RedHills Road, Surapet, Chennai 600066, India
2
Center for Quantum Science and Technology (CQST), Siksha ‘o’ Anusandhan University, Bhubaneswar 751030, India
3
Department of Physical Sciences, IISER-Kolkata, Mohanpur 741246, India
4
Department of Physical Electronics, School of Electrical Engineering, Faculty of Engineering, Center for Light-Matter Interaction, Tel Aviv P.O. Box 39040, Israel
5
Instituto de Alta Investigación, Universidad de Tarapacá, Casilla 7D, Arica 1000000, Chile
*
Author to whom correspondence should be addressed.
Photonics 2025, 12(10), 1034; https://doi.org/10.3390/photonics12101034
Submission received: 30 September 2025 / Revised: 16 October 2025 / Accepted: 17 October 2025 / Published: 19 October 2025
(This article belongs to the Section Quantum Photonics and Technologies)

Abstract

Electromagnetically induced transparency (EIT) is well known as a quantum optical phenomenon that permits a normally opaque medium to become transparent due to the quantum interference between transition pathways. This work addresses multi-soliton dynamics in an EIT system modeled by the integrable Maxwell–Bloch (MB) equations for a three-level Λ -type atomic configuration. By employing a generalized gauge transformation, we systematically construct explicit N-soliton solutions from the corresponding Lax pair. Explicit forms of one-, two-, three-, and four-soliton solutions are derived and analyzed. The resulting pulse structures reveal various nonlinear phenomena, such as temporal asymmetry, energy trapping, and soliton interactions. They also highlight coherent propagation, elastic collisions, and partial storage of pulses, which have potential implications for the design of quantum memory, slow light, and photonic data transport in EIT media. In addition, the conservation of fundamental physical quantities, such as the excitation norm and Hamiltonian, is used to provide direct evidence of the integrability and stability of the constructed soliton solutions.

1. Introduction

A weak probe laser can penetrate an initially opaque medium when a strong coherent coupling field is present, a phenomenon known as the electromagnetically induced transparency (EIT) [1,2,3,4]. In multi-level atomic systems, this phenomenon originates from destructive interference between excitation channels. It has attracted a lot of interest because of its crucial role in regulating light–matter interactions. Slow light, optical memory, nonlinear switching, and quantum data processing are optical phenomena and applications that are supported by EIT [5,6,7,8,9].
One of the most important models for understanding EIT is the three-level Λ -type atomic configuration, in which the combined evolution of the atomic population, coherence, and electromagnetic fields is governed by the system of Maxwell–Bloch (MB) equations. Under the conditions of the slowly evolving envelope and rotating-wave assumption, these equations characterize the coupled evolution of the optical fields and atomic coherence [10,11,12,13,14]. The MB system becomes integrable under certain resonance conditions, enabling the existence of soliton solutions.
The seminal work in [12] has shown that simulton-type soliton solutions are produced by the integrable MB system. Depending on the initial population distribution between the atomic states, the system exhibits many nonlinear phenomena, such as energy sharing, optical switching, transparency windows, and the pulse storage provided by adiabatically turning off the coupling beam [15,16,17,18,19,20,21,22,23,24,25,26]. The feasibility of using the relative phase and incoherent pumping to shape the optical response in quantum media has been demonstrated by recent studies, which have also examined the role of spontaneously generated coherence and phase control in achieving all-optical switching and coherent pulse manipulation in Λ -type systems [27].
In spite of these advancements, there is still a lack of systematic analysis of multi-soliton solutions in the MB framework, particularly concerning multi-pulse EIT dynamics that are essential for developing quantum network architectures. In this work, we aim to partly fill this gap by producing explicit N-soliton solutions of the MB system in the Λ -type EIT medium by means of a generalized iterative gauge transformation [28]. This method suggests a possibility to design scalable optical-data processing by means of the controlled creation of intricate soliton structures and evolution patterns.
Although the present formulation is strictly integrable under ideal resonance, realistic photonic and EIT platforms generally operate under conditions where small detuning, dephasing, or loss are inevitable. The multi-soliton states derived here provide analytical benchmarks that can serve as initial conditions or validation references for numerical simulations in such non-integrable regimes. Therefore, the present integrable analysis offers a theoretical guideline for exploring robust pulse propagation and coherent control in realistic quantum-optical systems.
The Maxwell–Bloch equations for the EIT configuration are formulated in Section 2 of this study, along with the respective integrability conditions. Using the generalized gauge transformation, we iteratively generate explicit N-soliton solutions in Section 3. In Section 4, we show one-, two-, three-, and four-soliton solutions by using this method, and in Section 5, we examine their spatiotemporal dynamics. In Section 6, we highlight the potential of multi-soliton interactions to enable improved photonic functions in EIT-based systems, and we address the ramifications of these findings for quantum data transfer and light storage, supported by the conserved quantities. The paper is concluded in Section 7.

2. The MB (Maxwell–Bloch) Equations

The MB equations describe the interaction of light with a three-level Λ -type atomic system under the EIT condition. These equations relate the density matrix components, which represent the atomic-state populations and coherence, to the evolution of the probe’s and coupling beams’ electric-field envelopes.
We consider the Λ -type atomic configuration, including three levels, viz., the ground state | 1 , metastable state | 2 , and the excited state | 3 . A weak probe field with electromagnetic frequency ω 1 is tuned to the | 1 | 3 transition, and a strong coupling field of frequency ω 2 drives the | 2 | 3 transition. Under the slowly varying envelope approximation, and assuming that the pulse durations are much shorter than the atomic relaxation times, the MB system is written as [10,11,12,13]
E 1 z + n c E 1 t = i 2 π N ω 1 c n μ 13 ρ 13 ,
E 2 z + n c E 2 t = i 2 π N ω 2 c n μ 23 ρ 23 ,
i ρ t = [ H , ρ ] ,
where E 1 and E 2 are the complex envelopes of the probe and coupling fields, respectively. Further, N is the atomic density, n is the refractive index, μ i j = d i j / are elements of the electric-dipole matrix for the atomic transitions, and ρ is the 3 × 3 density matrix of the atomic system.
The Hamiltonian that governs the dipole atomic dynamics under the rotating-wave approximation is
H = 0 0 μ 13 E 1 * 0 Δ ω 1 Δ ω 2 μ 32 E 2 * μ 31 E 1 μ 32 E 2 Δ ω 1 ,
where Δ ω 1 = ω 31 ω 1 and Δ ω 2 = ω 32 ω 2 are the Rabi frequencies of the probe and coupling fields, and Δ is the detuning parameter.
To simplify the system, we introduce the traveling coordinate, x = t n z / c , and the rescaled propagation variable, T = z / l , which allows us to cast the system in a more symmetric form. With suitable rescaling of the fields, q 1 = μ 31 E 1 and q 2 = μ 32 E 2 , and adopting the resonance condition ( Δ = 0 ), the system becomes
q 1 T = i ρ 31 ,
q 2 T = i ρ 32 ,
i ρ x = [ H res , ρ ] ,
where H res is the Hamiltonian corresponding to the resonance condition
H res = 0 0 q 1 * 0 0 q 2 * q 1 q 2 0 .
This system becomes integrable under specific conditions and admits Lax pair representation, enabling one to use analytical techniques, such as the inverse scattering transform [29], Bäcklund transform [30], and gauge/Darboux transform [31,32], to produce soliton solutions [33]. In this paper, we apply the gauge-transformation approach to systematically construct higher-order soliton solutions, which reveal diverse dynamical effects.

3. Constructing N-Soliton Solutions by Means of Gauge Transform

To obtain soliton solutions of the MB equations governing the EIT system, we utilize the integrability of the reduced system under the resonance condition and apply a generalized gauge transform [28]. This method makes it possible to systematically generate exact N-soliton solutions by successively applying elementary transformations to the vacuum solution of the associated Lax pair.

3.1. Lax Pair Operators

The integrable MB system, based on Equations (5)–(8), admits the following Lax pair representation:
Ψ x = U ( x , T ; λ ) Ψ ,
Ψ T = V ( x , T ; λ ) Ψ ,
where λ is a complex spectral parameter, with the operators
U ( x , T ; λ ) = i λ 0 i q 1 * 0 i λ i q 2 * i q 1 i q 2 i λ ,
V ( x , T ; λ ) = i 2 λ ρ 11 ρ 12 ρ 13 ρ 21 ρ 22 ρ 23 ρ 31 ρ 32 ρ 33 .
The compatibility condition, T U x V + [ U , V ] = 0 , recovers the integrable system of Equations (5)–(7) that govern the evolution of the fields and atomic population in the EIT system.

3.2. The Trivial Seed Solution

To generate soliton solutions by means of the gauge transformation, we begin with the trivial (vacuum) seed solution. It corresponds to the situation in which the probe and coupling fields are initially absent:
q 1 ( x , T ) = 0 , q 2 ( x , T ) = 0 .
Additionally, the atomic system is assumed to be in the incoherent state, with all off-diagonal density matrix elements vanishing,
ρ j k ( x , T ) = 0 , j k ,
with solely the populations in each state being nonzero:
ρ j j ( x , T ) = σ j j , j = 1 , 2 , 3 .
This initial condition defines the vacuum background of the system, which is employed, as usual, as the seed for constructing soliton solutions. In this case, the Lax pair becomes a diagonal system:
U [ 0 ] = i λ J = i λ 0 0 0 i λ 0 0 0 i λ ,
V [ 0 ] = i 2 λ σ 11 0 0 0 σ 22 0 0 0 σ 33 .
The eigenfunction of the Lax pair under this vacuum condition is
Ψ [ 0 ] ( x , T ; λ ) = e i λ x + i 2 λ σ 11 T 0 0 0 e i λ x + i 2 λ σ 22 T 0 0 0 e i λ x + i 2 λ σ 33 T .
This simple solution provides an appropriate starting point for constructing soliton solutions through successive iterations of the gauge transformation.

3.3. N-Fold Gauge Transformation

To construct N-soliton solutions, we apply an N-fold gauge transformation,
Ψ [ N ] ( x , T ; λ ) = G N ( λ ) Ψ [ 0 ] ( x , T ; λ ) ,
where the gauge matrix G N ( λ ) is built iteratively from the rank-one projection matrix (i.e., P 2 = P ):
G N ( λ ) = j = 1 N I λ j λ j * λ λ j * P j ,
with
P j = Ψ [ j 1 ] ( λ j ) Ψ [ j 1 ] ( λ j ) Ψ [ j 1 ] ( λ j ) Ψ [ j 1 ] ( λ j ) ,
and Φ j = Ψ [ j 1 ] ( x , T ; λ j ) · v j , where v j is an arbitrary constant polarization vector, v j = ( ε 1 j , ε 2 j , 1 ) tr ; I is the identity matrix.
At each stage, the fields q 1 and q 2 are updated recursively:
q 1 [ j ] = q 1 [ j 1 ] 2 i ( λ j λ j * ) ( P j ) 31 Φ j Φ j ,
q 2 [ j ] = q 2 [ j 1 ] 2 i ( λ j λ j * ) ( P j ) 32 Φ j Φ j .
These recursion relations start from the vacuum state q 1 [ 0 ] = q 2 [ 0 ] = 0 , with the respective projector,
P j = Φ j Φ j Φ j Φ j .

3.4. The Final Form of the N-Soliton Solution

After performing N gauge transformations, the resulting soliton solution for the probe and coupling fields can be expressed in a compact form as
q 1 [ N ] ( x , T ) = j = 1 N 2 i ( λ j λ j * ) ( Φ j Φ j ) 31 Φ j Φ j ,
q 2 [ N ] ( x , T ) = j = 1 N 2 i ( λ j λ j * ) ( Φ j Φ j ) 32 Φ j Φ j .
It clearly reveals the additive contribution of each individual soliton to the total field and ensures the preservation of the integrability and coherence properties at each step. The spectral parameters λ j and polarizations v j control the velocity, amplitude, and relative phase of each soliton component.
It is relevant to clarify the novelty of the results reported here. The one- and two-soliton solutions of the MB system were discussed previously in Refs. [12,13], where their explicit form and basic interaction properties were analyzed. In contrast, to the best of our knowledge, the exact three- and four-soliton solutions have not been reported before. The present work, therefore, extends the known results by constructing the closed-form expressions for higher-order soliton states ( N > 2 ) in the MB EIT system. These solutions are derived here systematically, using the gauge-transformation method, and their physical properties, including conserved quantities, energy distribution, and interaction dynamics, are analyzed in detail. Thus, our results provide the comprehensive characterization of multi-soliton dynamics ( N = 3 , 4 ) in this integrable light-matter system.

4. The Construction of Multi-Soliton Solutions

4.1. The One-Soliton Solution

From the general N-soliton solution,
q k [ N ] ( x , T ) = j = 1 N 2 i ( λ j λ j * ) ( Φ j Φ j ) 3 k Φ j Φ j , k = 1 , 2 ,
we begin with the general one-fold (applying the gauge transform once, which generates the one-soliton solution from the seed (vacuum) state) gauge-transformed solution of the MB system:
q k [ 1 ] ( x , T ) = 2 i ( λ 1 λ 1 * ) ( Φ 1 Φ 1 ) 3 k Φ 1 Φ 1 , k = 1 , 2 .
We thus obtain the one-soliton solution ( N = 1 ) as
q 1 [ 1 ] ( x , T ) = 2 i ( λ 1 λ 1 * ) ( Φ 1 Φ 1 ) 31 Φ 1 Φ 1 ,
q 2 [ 1 ] ( x , T ) = 2 i ( λ 1 λ 1 * ) ( Φ 1 Φ 1 ) 32 Φ 1 Φ 1 ,
where Φ 1 = Ψ [ 0 ] ( x , T ; λ 1 ) v 1 , and v 1 = ( ε 11 , ε 21 , 1 ) T is a constant polarization vector. Using the vacuum eigenfunction Ψ [ 0 ] given by Equation (18) and applying the gauge transformation, we obtain the one-soliton solution in the following form:
q 1 [ 1 ] ( x , T ) = 4 2 β 1 ε 11 e Θ 1 2 e Ξ 1 + e Ξ 2 + e Ξ 3 ,
q 2 [ 1 ] ( x , T ) = 4 2 β 1 ε 21 e Θ 2 2 e Ξ 1 + e Ξ 2 + e Ξ 3 ,
where
Θ 1 = i T α 1 ( σ 22 + 2 σ 33 ) + β 1 T σ 22 + 4 β 1 ( δ 1 + i χ 1 ) + 4 α 1 2 ( δ 1 + i χ 1 ) 2 ( α 1 2 + β 1 2 ) , Θ 2 = i T α 1 ( σ 11 + 2 σ 33 ) + β 1 T σ 11 + 4 β 1 ( δ 1 + i χ 1 ) + 4 α 1 2 ( δ 1 + i χ 1 ) 2 ( α 1 2 + β 1 2 ) , Ξ 1 = i 2 4 x ( α 1 + i β 1 ) + T ( σ 11 + σ 22 ) α 1 + i β 1 + T σ 33 α 1 i β 1 , Ξ 2 = 2 x ( i α 1 + β 1 ) + 4 δ 1 + i T σ 22 2 ( α 1 i β 1 ) + i T ( σ 11 + σ 33 ) 2 ( α 1 + i β 1 ) , Ξ 3 = 2 x ( i α 1 + β 1 ) + 4 δ 1 + i T σ 11 2 ( α 1 i β 1 ) + i T ( σ 22 + σ 33 ) 2 ( α 1 + i β 1 ) .
This explicit expression demonstrates the structure of the one-soliton solution and reveals how each physical parameter shapes the resulting pulse behavior in the medium.
The one-soliton solution describes a localized, stable pair of pulses in the probe and coupling fields. Its shape and speed are controlled by the spectral parameter λ 1 α 1 + i β 1 , where α 1 produces the soliton’s propagation speed, while β 1 determines the soliton’s width. The population matrix entries σ i j affect the phase dynamics through the interaction with the medium, and parameters δ 1 and χ 1 provide tunable phase and position offsets through the gauge transformation.
The solution’s denominator in Equations (29) and (30) involves the combination of three exponentials, representing the interference contributions from the three-level structure of the atomic medium. These exponential terms ensure that the soliton maintains coherence and avoids spreading, which is consistent with the integrable nature of the system.

4.2. The Derivation of the Two-Soliton Solution

The two-soliton solution of the MB system, produced by gauge transformation, is given by the general formula
q k [ 2 ] ( x , T ) = j = 1 2 2 i ( λ j λ j * ) ( Φ j Φ j ) 3 k Φ j Φ j , k = 1 , 2 ,
where each auxiliary vector is constructed as
Φ j = Ψ [ 0 ] ( x , T ; λ j ) v j , with v j = ( ε 1 j , ε 2 j , 1 ) tr , j = 1 , 2 .
Repeating the same approach and using the one-soliton solution, we construct the explicit form of the two-soliton solution as
q 1 [ 2 ] ( x , T ) = 4 2 β 1 ε 11 exp Ξ 12 2 k = 1 3 exp Ω k ( 1 ) 4 2 β 2 ε 12 exp Ξ 22 2 k = 1 3 exp Ω k ( 2 ) ,
q 2 [ 2 ] ( x , T ) = 4 2 β 1 ε 21 exp Ξ 12 2 k = 1 3 exp Ω k ( 1 ) 4 2 β 2 ε 22 exp Ξ 22 2 k = 1 3 exp Ω k ( 2 ) ,
where
Ξ 12 = i T α 1 ( σ 22 + 2 σ 33 ) + β 1 T σ 22 + 4 β 1 ( δ 1 + i χ 1 ) + 4 α 1 2 ( δ 1 + i χ 1 ) 2 ( α 1 2 + β 1 2 ) , Ξ 12 = i T α 1 ( σ 11 + 2 σ 33 ) + β 1 T σ 11 + 4 β 1 ( δ 1 + i χ 1 ) + 4 α 1 2 ( δ 1 + i χ 1 ) 2 ( α 1 2 + β 1 2 ) ,
and
Ξ 22 = 1 2 4 δ 2 + i T ( α 2 + i β 2 ) σ 33 + ( α 2 i β 2 ) T ( σ 22 + σ 33 ) + 4 ( α 2 + i β 2 ) χ 2 ( α 2 i β 2 ) ( α 2 + i β 2 ) , Ξ 22 = 1 2 4 δ 2 + i T ( α 2 + i β 2 ) σ 33 + ( α 2 i β 2 ) T ( σ 11 + σ 33 ) + 4 ( α 2 + i β 2 ) χ 2 ( α 2 i β 2 ) ( α 2 + i β 2 ) ,
with the arguments of the denominator exponentials (for j = 1 , 2 )
Ω 1 ( j ) = i 2 4 x ( α j + i β j ) + T ( σ 11 + σ 22 ) α j + i β j + T σ 33 α j i β j , Ω 2 ( j ) = 2 x ( i α j + β j ) + 4 δ j + i T σ 22 2 ( α j i β j ) + i T ( σ 11 + σ 33 ) 2 ( α j + i β j ) , Ω 3 ( j ) = 2 x ( i α j + β j ) + 4 δ j + i T σ 11 2 ( α j i β j ) + i T ( σ 22 + σ 33 ) 2 ( α j + i β j ) .
The two-soliton solution reflects the interplay of two localized wave packets co-evolving in the Λ -type EIT medium. Each soliton is produced by its spectral parameter λ j = α j + i β j , which determines its speed and shape. Expressions (32) and (33) clearly distinguish the contributions of each soliton to both fields q 1 and q 2 , while the exponentials in the shared denominators account for their interference. The denominator includes population coefficients σ i j , which mediate soliton–soliton interaction through atomic coherence.
This solution represents the situation in which two light pulses propagate with different group velocities, embedded in the probe and coupling beams. The variation of the amplitude and phase results from their mutual impact, which is enhanced by the atomic ensemble. The interference terms in the denominator exhibit beat-like structures, resulting in intensity oscillations and transient trapping. Such effects are hallmarks of coherent population trapping and nonlinear pulse steering, which are inherent in multi-soliton EIT dynamics.

4.3. The Explicit Form of the Three-Soliton Solution

Similarly, by applying the gauge-transformation iteration to the two-soliton solution, we obtain the three-soliton solution of the MB equation in a sufficiently compact form as
q 1 [ 3 ] ( x , T ) = 4 2 β 1 ε 11 · exp i T α 1 ( σ 22 + 2 σ 33 ) + β 1 ( T σ 22 + 4 β 1 ( δ 1 + i χ 1 ) ) + 4 α 1 2 ( δ 1 + i χ 1 ) 2 ( α 1 2 + β 1 2 ) 2 ( D 1 ( 1 ) + D 2 ( 1 ) + D 3 ( 1 ) ) j = 2 3 4 2 β j ε 1 j · exp 1 2 4 δ j + i T ( α j + i β j ) σ 33 + ( α j i β j ) ( T σ 22 + t σ 33 + 4 ( α j + i β j ) χ j ) ( α j i β j ) ( α j + i β j ) 2 ( D 1 ( j ) + D 2 ( j ) + D 3 ( j ) ) ,
and
q 2 [ 3 ] ( x , t ) = 4 2 β 1 ε 21 · exp i T α 1 ( σ 11 + 2 σ 33 ) + β 1 ( T σ 11 + 4 β 1 ( δ 1 + i χ 1 ) ) + 4 α 1 2 ( δ 1 + i χ 1 ) 2 ( α 1 2 + β 1 2 ) 2 ( D 1 ( 1 ) + D 2 ( 1 ) + D 3 ( 1 ) ) j = 2 3 4 2 β j ε 2 i · exp 1 2 4 δ j + i T ( α j + i β j ) σ 33 + ( α j i β j ) ( T σ 11 + t σ 33 + 4 ( α j + i β j ) χ j ) ( α j i β j ) ( α j + i β j ) 2 ( D 1 ( j ) + D 2 ( j ) + D 3 ( j ) ) ,
with the denominator terms for j = 1 , 2 , 3 being
D 1 ( j ) = exp i 2 4 x ( α j + i β j ) + T ( σ 11 + σ 22 ) α j + i β j + T σ 33 α j i β j , D 2 ( j ) = exp 2 x ( i α j + β j ) + 4 δ j + i T σ 22 2 ( α j i β j ) + i T ( σ 11 + σ 33 ) 2 ( α j + i β j ) , D 3 ( j ) = exp 2 x ( i α j + β j ) + 4 δ j + i T σ 11 2 ( α j i β j ) + i T ( σ 22 + σ 33 ) 2 ( α j + i β j ) .
The three-soliton solution introduces diverse field structures arising from the interaction between the three coherent pulses. The polarization vectors v j = ( ε 1 j , ε 2 j , 1 ) T and gauge parameters δ j , χ j determine the individual soliton contributions to each term in the solution, providing precise control over the relative phase and position. The exponential phase terms in the denominators represent the spatiotemporal shifts of the solitons caused by cross-modulation.
These multi-soliton arrangements pave the way for soliton-based multiplexing, which is essential for quantum switching and photonic logic because it allows multiple data channels to propagate concurrently and interact coherently without degrading.

4.4. The Construction of the Four-Soliton Solution

Next, we construct the four-soliton solution of the integrable MB equations by means of the gauge iterative method:
q 1 [ 4 ] ( x , T ) = 4 2 β 1 ε 11 · exp i T α 1 ( σ 22 + 2 σ 33 ) + β 1 T σ 22 + 4 β 1 ( δ 1 + i χ 1 ) + 4 α 1 2 ( δ 1 + i χ 1 ) 2 ( α 1 2 + β 1 2 ) 2 D 1 ( 1 ) + D 2 ( 1 ) + D 3 ( 1 ) j = 2 4 4 2 β j ε 1 j · exp 1 2 4 δ j + i T ( α j + i β j ) σ 33 + ( α j i β j ) T σ 22 + t σ 33 + 4 ( α j + i β j ) χ j ( α j i β j ) ( α j + i β j ) 2 D 1 ( j ) + D 2 ( j ) + D 3 ( j ) ,
and
q 2 [ 4 ] ( x , T ) = 4 2 β 1 ε 21 · exp i T α 1 ( σ 11 + 2 σ 33 ) + β 1 T σ 11 + 4 β 1 ( δ 1 + i χ 1 ) + 4 α 1 2 ( δ 1 + i χ 1 ) 2 ( α 1 2 + β 1 2 ) 2 D 1 ( 1 ) + D 2 ( 1 ) + D 3 ( 1 ) j = 2 4 4 2 β j ε 2 j · exp 1 2 4 δ j + i T ( α j + i β j ) σ 33 + ( α j i β j ) T σ 11 + t σ 33 + 4 ( α j + i β j ) χ j ( α j i β j ) ( α j + i β j ) 2 D 1 ( j ) + D 2 ( j ) + D 3 ( j ) ,
with the following common denominator terms for j = 1 , 2 , 3 , 4 :
D 1 ( j ) = exp i 2 4 x ( α j + i β j ) + T ( σ 11 + σ 22 ) α j + i β j + T σ 33 α j i β j , D 2 ( j ) = exp 2 x ( i α j + β j ) + 4 δ j + i T σ 22 2 ( α j i β j ) + i T ( σ 11 + σ 33 ) 2 ( α j + i β j ) , D 3 ( j ) = exp 2 x ( i α j + β j ) + 4 δ j + i T σ 11 2 ( α j i β j ) + i T ( σ 22 + σ 33 ) 2 ( α j + i β j ) .
The four-soliton solution represents the most intricate version considered here, encapsulating the interactions of four independently tunable soliton components. The algebraic structure of the solution underscores the additive nature of the coherent excitations in the integrable MB system, while the denominators, again, enforce the nonlinear coupling mediated by the system’s three-level structure. The population terms σ 11 , σ 22 , σ 33 now have a substantial impact on how the solitons split energy between fields and sustain coherence, highlighting the prominent significance of atomic coherence.

5. Discussion of the Soliton States and Their Interactions

5.1. The Interpretation of the One-Soliton Profile

Figure 1 displays the one-soliton solution, given by Equations (29) and (30), for the integrable MB system of Equations (5)–(7). The distinctive temporal asymmetry between the components q 1 ( x , t ) and q 2 ( x , t ) in the one-soliton solution is directly caused by the initial density matrix configuration and the complicated phase structure of the solution. We consider the initial condition where the population is fully placed in the ground state | 1 ( σ 11 = 1 , σ 22 = σ 33 = 0 ), and the coupling amplitudes are ε 11 = 0.5 , ε 21 = 1 ε 11 2 0.866 . In this configuration, the probing pulse q 1 emerges and propagates in the negative time direction, while pulse q 2 evolves in the positive time direction. This temporal asymmetry is caused by the different phase contributions from the σ i j factors in each component, which leads to group delay between the pulses.
The spectral parameter λ 1 = α 1 + i β 1 controls the soliton kinematics, where the real part α 1 = 0.4 sets the group velocity, and the imaginary part β 1 = 0.7 determines the temporal confinement of the pulse. The small gauge offsets δ 1 = 0.02 and χ 1 = 0.03 introduce slight temporal and phase displacements between the probe and coupling components in Figure 1. Hence, while the polarization and population parameters define the energy distribution, the spectral and gauge parameters tune the width, velocity, and phase evolution of the soliton during propagation.
The soliton associated with q 1 can be physically understood as entering the medium from the negative time domain and becoming trapped by the coherent interaction with atoms. This stored excitation is then re-emitted as the soliton in q 2 , which is generated and travels forward in time. Pulse trapping and re-emission can be observed in Figure 1, being a soliton counterpart of the behavior of stationary light pulses demonstrated in Refs. [9,15,19].

5.2. The Interpretation of Two-Soliton Pulse Propagation

Figure 2 displays the coherent population dynamics primarily distributed between the two ground states for the initial density matrix values σ 11 = 0.6 , σ 22 = 0.4 , and σ 33 = 0 for the two-soliton solution given by Equations (32) and (33). The absence of the population in the excited state ensures low absorption and provides a suitable medium for the production of the soliton through destructive quantum interference. The spectral parameters α 1 , 2 and β 1 , 2 dictate the relative velocities and temporal widths of the two pulses, while the gauge parameters δ i and χ i ( i = 1 , 2 ) introduce phase shifts that generate the oscillatory interference observed in Figure 2. The chosen values α 1 = 0.4 , α 2 = 0.6 , β 1 = 0.2 , and β 2 = 0.3 , together with δ 1 = 0.3 , δ 2 = 0.2 , χ 1 = 0.03 , and χ 2 = 0.01 , demonstrate how differential group velocities and small phase offsets produce beating-like intensity oscillations and transient energy trapping between the soliton components. The successful trapping of the probe pulses and their subsequent release in the form of coupling-field pulses demonstrates a partial storage and retrieval mechanism integrated into EIT, Refs. [15,20,23].

5.3. The Elastic Collisional Behavior of the Three-Soliton Solution

The pulse dynamics of the three-soliton solution of the MB system are characterized by localized structures in | q 1 [ 3 ] ( x , T ) | and | q 2 [ 3 ] ( x , T ) | , as shown in Figure 3. The initial values of the density matrix chosen here, σ 11 = 0.4 , σ 22 = 0.4 , and σ 33 = 0.2 , demonstrate that the atomic population is nearly evenly distributed in the lower states, with a very small share in the excited state. In this configuration, EIT allows several solitons to move across the atomic medium. The spectral parameters α j and β j ( j = 1 , 2 , 3 ) determine the distinct velocities and compressions of each soliton. A larger β 3 = 0.9 yields a narrower and faster pulse, whereas a smaller β 1 = 0.3 produces a broader, slower one. The gauge parameters δ j and χ j ( δ 1 , 2 , 3 = 0.2 , 0.3 , 0.5 ; χ 1 , 2 , 3 = 0.03 , 0.05 , 0.07 ) set the relative temporal offsets and fine-tune the phase coherence among the three interacting pulses. The coupling coefficients ε 11 = 0.35 , ε 12 = 0.31 , and ε 13 = 0.331 modulate the amplitude ratio between the probe and coupling fields. These parameter combinations reproduce the elastic collision behaviour and coherent population redistribution shown in Figure 3.
In contrast to the one- and two-soliton solutions, the three-soliton configurations displayed in Figure 3 exhibit the continuous and forward-directed evolution of all pulses without any obvious indication of field trapping. The solitons in | q 1 [ 3 ] | and | q 2 [ 3 ] | freely travel throughout the medium and produce complex wave interactions due to the improved nonlinear coupling. This fact highlights the connection between the optical-field coherence and atomic-population distribution in the multi-soliton regimes, demonstrating that the system transitions from the trapping-dominant scenario to soliton transmission, Ref. [18].

5.4. Four-Soliton Pulse Propagation

The four-soliton solution given by Equations (36) and (37) is displayed in Figure 4. In this case, fields q 1 and q 2 exhibit a pronounced asymmetry. The probe field q 1 displays four well-separated soliton pulses, while the coupling field q 2 carries just one dominant soliton. In particular, the values σ 11 = 0.2 , σ 22 = 0.4 , and σ 33 = 0.4 restrict the coupling dynamics to a more confined structure while allowing the medium to support numerous nonlinear excitations in the probe channel. The sequence of small α j values ( 0.01 0.04 ) and comparatively large β j values ( 0.5 0.9 ) produces strong temporal compression and well-separated localized peaks in the probe field. The gradual increase in the gauge parameters δ j and χ j ( 0.02 0.06 and 0.03 0.07 ) introduces ordered phase delays that generate the pulse train observed in Figure 4. These spectral and gauge variations, together with fixed polarization and population parameters, confirm that the multi-peak structure and asymmetric energy distribution can be precisely engineered by tuning α j , β j , δ j , and χ j . This configuration increases the possibility of storing several information channels in a single atomic ensemble by enabling the selective and coherent transmission of energy from the coupling field to numerous probing solitons [34].
The presence of many compressed solitons in the probing field is a certain manifestation of soliton-induced slow light, where the effective group velocity is significantly reduced due to the temporal compression and enhanced nonlinear interaction. This is essential for the realization of quantum data storage and delay lines [16,21,25]. Furthermore, the ability to generate and send a large number of coherent controllable soliton pulses offers possibilities for multi-qubit encoding, quantum-memory architectures, and optical logic gates, all being crucially important elements of quantum computing systems. Thus, the observed asymmetry not only illustrates the system’s intrinsic nonlinear dynamics but also its potential use in the frameworks of quantum communications and computations, where tunable soliton structures can serve as reliable, non-dispersive carriers of quantum information.
As mentioned above, the imaginary part of the spectral parameter λ j = α j + i β j governs the temporal breadth and localization of the soliton, whereas the real part α j determines its group velocity. Narrower and more peaked solitons are associated with larger values of β j . The internal structure of the soliton is shaped by the polarization vector v j = ( ε 1 j , ε 2 j , 1 ) tr , which also controls the amplitude and phase link between multi-soliton components.

6. Conserved Quantities in Multi-Soliton Dynamics

A fundamental characteristic of integrable systems is the existence of an infinite number of dynamical invariants. In this section, we analyze two key conserved quantities for the derived N-soliton solutions: the norm (N), which represents the total number of excitations (or total field intensity), and the Hamiltonian (H), which represents the total energy of the system.

6.1. Analytical Expressions for the Conserved Quantities

For the integrable MB system under consideration, the conserved quantities can be derived from the Lax pair structure [4]. The total norm and Hamiltonian are given by
N = + | q 1 ( x , T ) | 2 + | q 2 ( x , T ) | 2 d x , H = + E ( x , T ) d x = + | q 1 | 2 + | q 2 | 2 + ( q 1 * ρ 31 + q 1 ρ 31 * + q 2 * ρ 32 + q 2 ρ 32 * ) d x ,
where the energy density E ( x , T ) comprises the energy stored in the electromagnetic fields ( | q 1 | 2 + | q 2 | 2 ) and the interaction energy between the fields and the atomic dipoles.
For the N-soliton solutions constructed by means of the gauge-transformation method, these integrals can be evaluated analytically. The results confirm that the total norm and Hamiltonian amount to the sum of the contributions from individual solitons (as it should be for the integrable system):
N total = j = 1 N N j , H total = j = 1 N H j ,
where the contributions for a single soliton, characterized by the spectral parameter λ j = α j + i β j and polarization vector v j = ( ε 1 j , ε 2 j , 1 ) T , are
N j = 8 β j ( ε 1 j 2 + ε 2 j 2 ) , H j = ( α j 2 β j 2 ) N j .

6.2. Numerical Values and the Physical Interpretation

The calculated values of these conserved quantities for the one-, two-, three-, and four-soliton solutions at various times are presented in Table 1.
The conservation of the norm N and Hamiltonian H in all soliton configurations, validated numerically, ensures that the gauge-transformation method produces consistent solutions. Importantly, the norm is additive so that the total excitation number for the multi-soliton states is the sum of their constituents (e.g., N = 8.0 for the two-soliton case, obtained from N 1 = 5.6 and N 2 = 2.4 ). This particle-like property is a characteristic of integrable soliton dynamics and confirms that each soliton acts as an independent carrier of the conserved excitations. The negative values of the Hamiltonian further demonstrate that all soliton states correspond to bound configurations, with the interaction energy between the light fields and atomic coherence outweighing the free-field contribution. This binding mechanism prevents the dispersion and underpins the integrity of the solitons.
Small-amplitude linear excitations of the Maxwell–Bloch system correspond to positive energy values ( H > 0 ). In contrast, the localized soliton solutions obtained here exhibit negative Hamiltonians ( H < 0 ), which indicates that they represent energetically bound states below the continuum of linear waves. This situation guarantees that the solitons cannot spontaneously decay into linear radiation while conserving the excitation norm. Hence, a negative H provides energetic protection for the soliton against dispersive decay. At the same time, the specific numerical value of H depends on the soliton parameters α j and β j , which determine the balance between kinetic and potential (field–matter interaction) energies. The negative interaction energy supports stable self-trapped light–matter EIT solitons.
The results also reveal the scalable data capacity of the EIT medium. The progression of the norm from one- to four-soliton solutions ( N = 5.6 8.0 13.6 20.0 ) demonstrates the ability of the medium to support multiple coherent data-carrying channels without degradation. Each soliton thus functions as a distinct channel for photonic data storage or transfer, aligning with the requirements of optical buffering, quantum memory, and coherent switching devices [35,36,37]. Moreover, while the total conserved energy is constant, its spatial distribution between the field and atomic components is dynamic. These findings confirm that the MB–EIT solitons feature both the mathematical elegance of integrability and the physical robustness needed for applications in nonlinear photonics and quantum information technology.

6.3. Experimental Observability and Robustness

The multi-soliton configurations predicted here can be experimentally observed through intensity and phase measurements of the probe and coupling pulses in Λ -type atomic vapors or cold-atom ensembles. In particular, for N = 3 and N = 4, the sequential temporal peaks in the probe field correspond to multiple stored and retrieved light channels, which may be detected as slow-light pulse trains or energy-exchange oscillations between the probe and coupling beams.
In realistic EIT systems, deviations from the perfect resonance or moderate decoherence slightly break integrability but do not destroy the soliton-like profiles, as confirmed in previous numerical studies of the Maxwell–Bloch system. Small detuning mainly leads to smooth phase shifts and amplitude damping, implying that the multi-soliton states are robust against the action of weak perturbations. Consequently, the exact solutions obtained here provide a reliable foundation for designing stable optical-memory and photonic-switching experiments under near-resonant conditions.

7. Conclusions

In this paper, N-soliton solutions to the MB (Maxwell–Bloch) equations, which govern EIT (electromagnetically induced transparency) in the Λ -type atomic system, have been systematically constructed. We have obtained explicit analytical expressions for the one-, two-, three-, and four-soliton solutions using an extended gauge transformation. Our analysis has revealed diverse dynamical behaviors, such as the temporal asymmetry, energy trapping, and elastic collisions of solitons. The spectral, polarization, and gauge factors govern phase-controlled pulse propagation and interaction in the multi-soliton solutions. The field-selective propagation and observed asymmetry highlight the usefulness of EIT for highly controllable manipulations of light–matter interactions. These findings offer new possibilities for the design of multi-channel quantum communication schemes, slow-light delay lines, and optical memory components. The analysis of the conserved quantities not only provides a fundamental check of the validity of the solutions, but also reveals the potential of the EIT medium as a reliable, scalable platform for advanced photonic operations based on multi-soliton dynamics.
The framework considered here suggests possibilities for the design of scalable soliton-based protocols in quantum photonics, particularly where robustness and coherence are crucial requirements. Further extension of the analysis may address dissipative effects, non-integrable perturbations, and soliton control in higher-dimensional or multi-field generalizations of the MB system.

Author Contributions

R.K.V.: Conceptualization of the study, Methodology, Formal analysis, Investigation, Validation of analytical results, Writing—original draft, Writing—review & editing; P.K.P.: Guidance in theoretical framework, Critical review of methodology, Interpretation of physical implications; B.A.M.: Supervision, Contribution to integrability analysis, Interpretation of nonlinear phenomena, Critical suggestions on mathematical derivations, Refinement of results, review & editing. All authors have read and agreed to the published version of the manuscript.

Funding

This research received no external funding.

Data Availability Statement

Data are contained within the article.

Conflicts of Interest

The authors declare no conflicts of interest.

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Figure 1. The one-soliton solution given by Equations (29) and (30) for the parameter set α 1 = 0.4 , β 1 = 0.7 , δ 1 = 0.02 , χ 1 = 0.03 , ε 11 = 0.5 , and ε 21 = 1 ε 11 2 0.866 , with the initial density matrix values of σ 11 = 1 and σ 22 = σ 33 = 0 .
Figure 1. The one-soliton solution given by Equations (29) and (30) for the parameter set α 1 = 0.4 , β 1 = 0.7 , δ 1 = 0.02 , χ 1 = 0.03 , ε 11 = 0.5 , and ε 21 = 1 ε 11 2 0.866 , with the initial density matrix values of σ 11 = 1 and σ 22 = σ 33 = 0 .
Photonics 12 01034 g001
Figure 2. The two-soliton solution given by Equations (32) and (33) for the parameter set α 1 = 0.4 , α 2 = 0.6 , β 1 = 0.2 , β 2 = 0.3 , δ 1 = 0.3 , δ 2 = 0.2 , χ 1 = 0.03 , χ 2 = 0.01 , ε 11 = 0.6 , and ε 12 = 0.5 , with the initial density matrix values of σ 11 = 0.6 , σ 22 = 0.4 , and σ 33 = 0 .
Figure 2. The two-soliton solution given by Equations (32) and (33) for the parameter set α 1 = 0.4 , α 2 = 0.6 , β 1 = 0.2 , β 2 = 0.3 , δ 1 = 0.3 , δ 2 = 0.2 , χ 1 = 0.03 , χ 2 = 0.01 , ε 11 = 0.6 , and ε 12 = 0.5 , with the initial density matrix values of σ 11 = 0.6 , σ 22 = 0.4 , and σ 33 = 0 .
Photonics 12 01034 g002
Figure 3. The three-soliton solution given by Equations (34) and (35) for the parameter set α 1 = 0.4 , α 2 = 0.2 , α 3 = 0.5 , β 1 = 0.3 , β 2 = 0.7 , β 3 = 0.9 , δ 1 = 0.2 , δ 2 = 0.3 , δ 3 = 0.5 , χ 1 = 0.03 , and χ 2 = 0.05 , χ 3 = 0.07 , with the coupling coefficients ε 11 = 0.35 , ε 12 = 0.31 , and ε 13 = 0.331 , and the initial values of the density matrix as σ 11 = 0.4 , σ 22 = 0.4 , and σ 33 = 0.2 .
Figure 3. The three-soliton solution given by Equations (34) and (35) for the parameter set α 1 = 0.4 , α 2 = 0.2 , α 3 = 0.5 , β 1 = 0.3 , β 2 = 0.7 , β 3 = 0.9 , δ 1 = 0.2 , δ 2 = 0.3 , δ 3 = 0.5 , χ 1 = 0.03 , and χ 2 = 0.05 , χ 3 = 0.07 , with the coupling coefficients ε 11 = 0.35 , ε 12 = 0.31 , and ε 13 = 0.331 , and the initial values of the density matrix as σ 11 = 0.4 , σ 22 = 0.4 , and σ 33 = 0.2 .
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Figure 4. The four-soliton solution of Equations (36) and (37) for the parameter set α 1 = 0.04 , α 2 = 0.01 , α 3 = 0.02 , α 4 = 0.03 ; β 1 = 0.8 , β 2 = 0.7 , β 3 = 0.9 , β 4 = 0.5 ; δ 1 = 0.02 , δ 2 = 0.03 , δ 3 = 0.05 , δ 4 = 0.06 ; χ 1 = 0.03 , χ 2 = 0.05 , χ 3 = 0.07 , and χ 4 = 0.06 , with the initial density matrix values of σ 11 = 0.2 , σ 22 = 0.4 , σ 33 = 0.4 ; ε 11 = 0.35 , ε 12 = 0.51 , and ε 13 = 0.331 .
Figure 4. The four-soliton solution of Equations (36) and (37) for the parameter set α 1 = 0.04 , α 2 = 0.01 , α 3 = 0.02 , α 4 = 0.03 ; β 1 = 0.8 , β 2 = 0.7 , β 3 = 0.9 , β 4 = 0.5 ; δ 1 = 0.02 , δ 2 = 0.03 , δ 3 = 0.05 , δ 4 = 0.06 ; χ 1 = 0.03 , χ 2 = 0.05 , χ 3 = 0.07 , and χ 4 = 0.06 , with the initial density matrix values of σ 11 = 0.2 , σ 22 = 0.4 , σ 33 = 0.4 ; ε 11 = 0.35 , ε 12 = 0.51 , and ε 13 = 0.331 .
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Table 1. Conserved quantities for the multi-soliton solutions. The norm (N) and Hamiltonian (H) remain constant for each soliton type at all times, confirming the integrability of the system.
Table 1. Conserved quantities for the multi-soliton solutions. The norm (N) and Hamiltonian (H) remain constant for each soliton type at all times, confirming the integrability of the system.
Soliton TypeNorm (N)Hamiltonian (H)
One-soliton solution5.600 1.848
Two-soliton solution8.000 0.880
Three-soliton solution13.600 8.264
Four-soliton solution20.000 12.400
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Vaduganathan, R.K.; Panigrahi, P.K.; Malomed, B.A. Multi-Soliton Propagation and Interaction in Λ-Type EIT Media: An Integrable Approach. Photonics 2025, 12, 1034. https://doi.org/10.3390/photonics12101034

AMA Style

Vaduganathan RK, Panigrahi PK, Malomed BA. Multi-Soliton Propagation and Interaction in Λ-Type EIT Media: An Integrable Approach. Photonics. 2025; 12(10):1034. https://doi.org/10.3390/photonics12101034

Chicago/Turabian Style

Vaduganathan, Ramesh Kumar, Prasanta K. Panigrahi, and Boris A. Malomed. 2025. "Multi-Soliton Propagation and Interaction in Λ-Type EIT Media: An Integrable Approach" Photonics 12, no. 10: 1034. https://doi.org/10.3390/photonics12101034

APA Style

Vaduganathan, R. K., Panigrahi, P. K., & Malomed, B. A. (2025). Multi-Soliton Propagation and Interaction in Λ-Type EIT Media: An Integrable Approach. Photonics, 12(10), 1034. https://doi.org/10.3390/photonics12101034

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