Abstract
The Schrödinger equation is solved analytically for a particle subject to an enhanced Pöschl-Teller (EPT) potential in the presence of an external magnetic field and an Aharonov-Bohm flux field that induces topological phase effects. The bound state ro-vibrational energy equations are obtained using the generalized fractional Nikiforov-Uvarov method in conjunction with the Pekeris approximation scheme. The fractional order is introduced as an effective parameter that accounts for nonlocal and anharmonic ro-vibrational interactions that are not fully represented within the standard integer order framework. Based on these energy expressions, the mean thermal magnetization is derived within the partition function formalism. Numerical applications to diatomic molecules such as CO (X 1Σ+), Cs2 (3 3Σg+), ICl (X 1Σg+), 7Li2 (1 3Δg), Na2 (C(2) 1Πu), and NaK (c 3Σ+) show that the mean percentage absolute deviation values decrease from 0.0990%, 0.1407%, 1.0027%, 1.9504%, 0.1234%, and 0.9811% to 0.0905%, 0.1020%, 0.5501%, 1.1756%, 0.0474%, and 0.4840% when fractional parameters are incorporated, indicating improved agreement with experimental data and enhanced flexibility of the ro-vibrational energy model. The analysis further shows that, at fixed temperatures, the mean thermal magnetization of the Na2 (C(2) 1Πu) dimer increases with increasing magnetic field strength, highlighting the sensitivity of the system to external field variations. These results establish the EPT potential combined with a fractional order formulation as a reliable and adaptable analytical framework for describing the quantum and thermomagnetic behavior of diatomic molecules influenced by magnetic and topological quantum fields.
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Appendices
Appendix A
This appendix presents the derivation of the expansion coefficients κk and λk for k = 0, 1, 2. For brevity, approximations (6) and (7) are restated in the compact form.
where the associated definitions are
The objective is to expand the functions f(ρ), g(ρ), u(ρ), and v(ρ) in a Taylor series around the equilibrium point ρ = ρe, giving
Here, a prime denotes differentiation with respect to ρ. The symbols fe, …, etc., represent the values of the corresponding functions evaluated at ρ = ρe. Using (A3) -(A6), the following expressions are obtained
r\(p=\alpha {\rho _{e} }\)The auxiliary quantities \(p=\alpha {\rho _\text{e} }\), and \(q=\alpha \left( {{\rho _\text{e} } - {\rho _0}} \right)\) are introduced for notational simplicity. Substituting expansions (A7), (A9), and (A10) into (A1), and equating coefficients of \({\left( {{\rho _\text{e} } - {\rho _0}} \right)^0}\), \({\left( {{\rho _\text{e} } - {\rho _0}} \right)^1}\), and \({\left( {{\rho _\text{e} } - {\rho _0}} \right)^2}\), results in the linear system
Solving (A15) -(A17) yields
To determine the general expressions for the coefficients κk (k = 0, 1, 2), expansions (A8)-(A10) are substituted into (A2), and coefficients of \({\left( {{\rho _\text{e} } - {\rho _0}} \right)^0}\), \({\left( {{\rho _\text{e} } - {\rho _0}} \right)^1}\), and \({\left( {{\rho _\text{e} } - {\rho _0}} \right)^2}\) are matched on both sides, giving
Solving (A21) -(A23) gives the expansion coefficients
where
Appendix B
This appendix provides the detailed derivation of the potential parameters α, q, U0, U1, and U2. For convenience, the EPT potential defined in Eq. (2) is rewritten in the more tractable form.
where the auxiliary functions are
Equations (B1) -(B3) are connected through the identity \({x^2} - {y^2}=1\), which is used repeatedly in subsequent simplifications. To enforce the boundary condition (29a), note that in the limit ρ → ∞, both x → ∞ and y → ∞. Consequently, 1/y2 → 0, x/y2 → 0, and applying these limits to (B1) gives
At the equilibrium point ρ = ρe, substituting (B2) and (B3) into (B1) yields
where
Inserting (B4) and (B5) into condition (29a) leads to
To satisfy the derivative-based conditions (29b) -(29d), direct differentiation of (2) with respect to ρ is algebraically unwieldy. A more manageable approach is to work from the total differential of U(ρ)
Differentiating (B2) and (B3) gives
Substituting (B10) and (B11) into (B9) yields the differential operator used to generate successive derivatives of the potential
Applying this operator to (B1) produces the first derivative
To simplify further differentiation, the identity \({y^2}={x^2} - 1\) is applied to (B13) so that the numerator depends only on x, and the denominator only on y, giving
Evaluating at ρ = ρe (where x = xe, y = ye), and applying condition (29b), results in
Solving the linear system formed by (B8) and (B15) yields
Next, applying operator (B12) to (B14) gives the second derivative
At equilibrium ρ = ρe, using (B16), (B17), (B18) with condition (29c) produces
Proceeding similarly, the third derivative at equilibrium is obtained as
Combining (B19), (B21), and condition (29d), and solving gives
where |x| denotes the absolute value of x.
The Varshni conditions determine expressions for U1, U2, α, and ρ0, but do not yield a direct formula for U0. To obtain U0, the constraint U(ρe) = 0 is imposed on the potential, giving U0 = De. This choice shifts the potential minimum to zero without altering the physical observables of the system48. The motivation for this constraint is: (a) It standardizes the reference energy for comparison with other diatomic oscillator models. (b) It preserves all thermodynamic and spectroscopic properties of the modeled system. This convention ensures that the equilibrium minimum of the EPT oscillator is fixed at zero potential while maintaining consistency with established results in the literature.
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Eyube, E.S., Kamaludeen, M., Vijinti, F.C. et al. Energy and thermal magnetization of diatomic molecules under the enhanced Pöschl-Teller potential. Sci Rep (2026). https://doi.org/10.1038/s41598-026-49748-w
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DOI: https://doi.org/10.1038/s41598-026-49748-w


