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Energy and thermal magnetization of diatomic molecules under the enhanced Pöschl-Teller potential
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  • Published: 25 April 2026

Energy and thermal magnetization of diatomic molecules under the enhanced Pöschl-Teller potential

  • E. S. Eyube  ORCID: orcid.org/0000-0001-5059-03931,
  • M. Kamaludeen1,
  • F. C. Vijinti2,
  • I. I. Fwangle3 &
  • …
  • M. F. Isa1 

Scientific Reports , Article number:  (2026) Cite this article

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  • Chemistry
  • Mathematics and computing
  • Physics

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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Authors and Affiliations

  1. Department of Physics, Faculty of Physical Sciences, Modibbo Adama University, P.M.B. 2076, Yola, Adamawa State, Nigeria

    E. S. Eyube, M. Kamaludeen & M. F. Isa

  2. Department of Basic and Applied Science, College of Agriculture, Science and Technology, P.M.B. 1025, Jalingo, Taraba State, Nigeria

    F. C. Vijinti

  3. Department of Physical Science Education, Faculty of Education, Modibbo Adama University, P.M.B. 2076, Yola, Adamawa State, Nigeria

    I. I. Fwangle

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  1. E. S. Eyube
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  2. M. Kamaludeen
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Correspondence to E. S. Eyube.

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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.

$${\text{f}} \approx {\lambda _0}+{\lambda _1}{\text{u}}+{\lambda _2}{\text{v}}$$
(A1)
$${\text{g}} \approx {\kappa _0}+{\kappa _1}{\text{u}}+{\kappa _2}{\text{v}}$$
(A2)

where the associated definitions are

$${\text{f}}=\frac{{\rho _{\text{e} }^{2}}}{{{\rho ^2}}}$$
(A3)
$${\text{g}}=\frac{{{\rho _\text{e} }}}{\rho }\tanh \left( {\tfrac{1}{2}\alpha \rho } \right)$$
(A4)
$${\text{u}}={\text{csch} ^2}\alpha \left( {\rho - {\rho _0}} \right)$$
(A5)
$${\text{v}}={\text{csch} ^2}\alpha \left( {\rho - {\rho _0}} \right)\cosh \alpha \left( {\rho - {\rho _0}} \right)$$
(A6)

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

$${\text{f}} \approx {{\text{f}}_{\text{e}}}+{{{\text{f}^{\prime}}}_{\text{e}}} \cdot \left( {\rho - {\rho _\text{e} }} \right)+\frac{1}{2}{{{\text{f}^{\prime\prime}}}_{\text{e}}} \cdot {\left( {\rho - {\rho _\text{e} }} \right)^2}+ \cdots$$
(A7)
$${\text{g}} \approx {{\text{g}}_{\text{e}}}+{{{\text{g}^{\prime}}}_{\text{e}}} \cdot \left( {\rho - {\rho _\text{e} }} \right)+\frac{1}{2}{{{\text{g}^{\prime\prime}}}_{\text{e}}} \cdot {\left( {\rho - {\rho _\text{e} }} \right)^2}+ \cdots$$
(A8)
$${\text{u}} \approx {{\text{u}}_{\text{e}}}+{{{\text{u}^{\prime}}}_{\text{e}}} \cdot \left( {\rho - {\rho _\text{e} }} \right)+\frac{1}{2}{{{\text{u}^{\prime\prime}}}_{\text{e}}} \cdot {\left( {\rho - {\rho _\text{e} }} \right)^2}+ \cdots$$
(A9)
$${\text{v}} \approx {{\text{v}}_{\text{e}}}+{{{\text{v}^{\prime}}}_{\text{e}}} \cdot \left( {\rho - {\rho _\text{e} }} \right)+\frac{1}{2}{{{\text{v}^{\prime\prime}}}_{\text{e}}} \cdot {\left( {\rho - {\rho _\text{e} }} \right)^2}+ \cdots$$
(A10)

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

$${{\text{f}}_{\text{e}}}=1,\quad {{{\text{f}^{\prime}}}_{\text{e}}}= - \frac{2}{{{\rho _\text{e} }}},\quad {{{\text{f}^{\prime\prime}}}_{\text{e}}}=\frac{6}{{\rho _{\text{e} }^{2}}}$$
(A11)
$${{\text{g}}_{\text{e}}}=\tanh \left( {\tfrac{1}{2}p} \right),\;{{{\text{g}^{\prime}}}_{\text{e}}}={{\text{g}}_{\text{e}}}\left( {\alpha \text{sech} p - \frac{1}{{{\rho _\text{e} }}}} \right),\;{{{\text{g}^{\prime\prime}}}_{\text{e}}}={{\text{g}}_{\text{e}}}\left\{ {\frac{1}{2}{\alpha ^2}{{\tanh }^2}\left( {\tfrac{1}{2}p} \right) - \frac{{2\alpha }}{{{\rho _\text{e} }}}\text{csch} p+\frac{2}{{\rho _{\text{e} }^{2}}}} \right\}$$
(A12)
$${{\text{u}}_{\text{e}}}={\text{csch} ^2}q,\quad {{{\text{u}^{\prime}}}_{\text{e}}}= - 2\alpha {{\text{u}}_{\text{e}}}\coth q,\quad {{{\text{u}^{\prime\prime}}}_{\text{e}}}=2{\alpha ^2}{{\text{u}}_{\text{e}}}\left( {2{{\coth }^2}q+{{\text{csch} }^2}q} \right)$$
(A13)
$${{\text{v}}_{{e}}}={\text{csch} ^2}q\cosh q,\quad {{{\text{v}^{\prime}}}_{\text{e}}}= - \alpha {{\text{v}}_{\text{e}}}\left( {2\coth q - \tanh q} \right),\quad {{{\text{v}^{\prime\prime}}}_{\text{e}}}={\alpha ^2}{{\text{v}}_{\text{e}}}\left( {{{\coth }^2}q+5{{\text{csch} }^2}q} \right)$$
(A14)

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

$${\lambda _0}+{{\text{u}}_\text{e} }{\lambda _1}+{{\text{v}}_{\text{e}}}{\lambda _2}={{\text{f}}_{\text{e}}}$$
(A15)
$${{{\text{u}^{\prime}}}_{e} }{\lambda _1}+{{{\text{v}^{\prime}}}_{\text{e}}}{\lambda _2}={{{\text{f}^{\prime}}}_{\text{e}}}$$
(A16)
$${{{\text{u}^{\prime\prime}}}_\text{e} }{\lambda _1}+{{{\text{v}^{\prime\prime}}}_{\text{e}}}{\lambda _2}={{{\text{f}^{\prime\prime}}}_{\text{e}}}$$
(A17)

Solving (A15) -(A17) yields

$${\lambda _2}=\frac{{{{{{\text{u}^{\prime}}}}_{\text{e}}}{{{{\text{f}^{\prime\prime}}}}_{\text{e}}} - {{{{\text{u}^{\prime\prime}}}}_{\text{e}}}{{{{\text{f}^{\prime}}}}_{\text{e}}}}}{{{{{{\text{u}^{\prime}}}}_{\text{e}}}{{{{\text{v}^{\prime\prime}}}}_{\text{e}}} - {{{{\text{u}^{\prime\prime}}}}_{\text{e}}}{{{{\text{v}^{\prime}}}}_{\text{e}}}}}=\frac{{2{{\cosh }^2}q+1}}{{p\sinh q}} - \frac{{3\cosh q}}{{{p^2}}}$$
(A18)
$${\lambda _1}=\frac{{{{{{\text{f}^{\prime}}}}_{\text{e}}}{{{{\text{v}^{\prime\prime}}}}_{\text{e}}} - {{{{\text{f}^{\prime\prime}}}}_{\text{e}}}{{{{\text{v}^{\prime}}}}_{\text{e}}}}}{{{{{{\text{u}^{\prime}}}}_{\text{e}}}{{{{\text{v}^{\prime\prime}}}}_{\text{e}}} - {{{{\text{u}^{\prime\prime}}}}_{\text{e}}}{{{{\text{v}^{\prime}}}}_{\text{e}}}}}= - \frac{{{{\cosh }^2}q+5}}{{2p\tanh q}}+\frac{{6{{\cosh }^2}q+3}}{{2{p^2}}}$$
(A19)
$${\lambda _0}={{\text{f}}_{\text{e}}} - {{\text{u}}_\text{e} }{\lambda _1} - {{\text{v}}_{\text{e}}}{\lambda _2}=1 - \frac{{3\coth q}}{{2p}}+\frac{3}{{2{p^2}}}$$
(A20)

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

$${\kappa _0}+{{\text{u}}_{e} }{\kappa _1}+{{\text{v}}_{\text{e}}}{\kappa _2}={{\text{g}}_{\text{e}}}$$
(A21)
$${{{u^{\prime}}}_{e} }{\kappa _1}+{{{v^{\prime}}}_{\text{e}}}{\kappa _2}={{{g^{\prime}}}_{\text{e}}}$$
(A22)
$${{{u^{\prime\prime}}}_{e} }{\kappa _1}+{{{v^{\prime\prime}}}_{\text{e}}}{\kappa _2}={{{g^{\prime\prime}}}_{\text{e}}}$$
(A23)

Solving (A21) -(A23) gives the expansion coefficients

$${\kappa _2}=\frac{{{{{{\text{u}^{\prime}}}}_{\text{e}}}{{{{\text{g}^{\prime\prime}}}}_{\text{e}}} - {{{{\text{u}^{\prime\prime}}}}_{\text{e}}}{{\text{g}^{\prime}}_{\text{e}}}}}{{{{{{\text{u}^{\prime}}}}_{\text{e}}}{{{{\text{v}^{\prime\prime}}}}_{\text{e}}} - {{{{\text{u}^{\prime\prime}}}}_{\text{e}}}{{{{\text{v}^{\prime}}}}_{\text{e}}}}}={\kappa _a}\left( {3\coth q\cosh q - \sinh q} \right)+{\kappa _b}\cosh q$$
(A24)
$${\kappa _1}=\frac{{{{{{\text{g}^{\prime}}}}_{\text{e}}}{{{{\text{v}^{\prime\prime}}}}_{\text{e}}} - {{{{\text{g}^{\prime\prime}}}}_{\text{e}}}{{{{\text{v}^{\prime}}}}_{\text{e}}}}}{{{{{{\text{u}^{\prime}}}}_{\text{e}}}{{{{\text{v}^{\prime\prime}}}}_{\text{e}}} - {{{{\text{u}^{\prime\prime}}}}_{\text{e}}}{{{{\text{v}^{\prime}}}}_{\text{e}}}}}= - {\kappa _a}\left( {3\coth q{{\cosh }^2}q - \frac{5}{4}\sinh 2q} \right)+\frac{1}{2}{\kappa _b}\left( {{{\cosh }^2}q+1} \right)$$
(A25)
$${\kappa _0}=\tanh \left( {\tfrac{1}{2}p} \right) - \frac{3}{2}{\kappa _a}\coth q - {\kappa _b}\left( {2{{\coth }^2}q - \frac{1}{2}} \right)$$
(A26)

where

$${\kappa _a}=\frac{1}{2}{{sech} ^2}\left( {\tfrac{1}{2}p} \right) - \frac{{\tanh \left( {\tfrac{1}{2}p} \right)}}{p}$$
(A27)
$${\kappa _b}= - \frac{1}{2}{{sech} ^2}\left( {\tfrac{1}{2}p} \right)\tanh \left( {\tfrac{1}{2}p} \right) - \frac{{{{{sech} }^2}\left( {\tfrac{1}{2}p} \right)}}{p}+\frac{{2\tanh \left( {\tfrac{1}{2}p} \right)}}{{{p^2}}}$$
(A28)

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.

$${\text{U}}\left( \rho \right)={{\text{U}}_0}+\frac{1}{{{y^2}}}{{\text{U}}_1} - \frac{x}{{{y^2}}}{{\text{U}}_2}$$
(B1)

where the auxiliary functions are

$$x=\cosh \alpha \left( {\rho - {\rho _0}} \right)$$
(B2)
$$y=\sinh \alpha \left( {\rho - {\rho _0}} \right)$$
(B3)

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

$$\mathop {\lim }\limits_{{\rho \to \infty }} {\text{U}}\left( \rho \right)={{\text{U}}_0}$$
(B4)

At the equilibrium point ρ = ρe, substituting (B2) and (B3) into (B1) yields

$${\text{U}}\left( {{\rho _\text{e} }} \right)={{\text{U}}_0}+\frac{1}{{y_{\text{e} }^{2}}}{{\text{U}}_1} - \frac{{{x_\text{e} }}}{{y_{\text{e} }^{2}}}{{\text{U}}_2}$$
(B5)

where

$${x_\text{e} }=\cosh \alpha \left( {{\rho _\text{e} } - {\rho _0}} \right)$$
(B6)
$${y_\text{e} }=\sinh \alpha \left( {{\rho _\text{e} } - {\rho _0}} \right)$$
(B7)

Inserting (B4) and (B5) into condition (29a) leads to

$$- {{\text{U}}_1}+{x_\text{e} }{{\text{U}}_2}=y_{\text{e} }^{2}{D_\text{e} }$$
(B8)

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)

$$\frac{{{\text{dU}}}}{{{\text{d}}\rho }}=\frac{{\partial {\text{U}}}}{{\partial x}}\frac{{dx}}{{{\text{d}}\rho }}+\frac{{\partial {\text{U}}}}{{\partial y}}\frac{{dy}}{{{\text{d}}\rho }}$$
(B9)

Differentiating (B2) and (B3) gives

$$\frac{{{\text{d}}x}}{{{\text{d}}\rho }}=\alpha \sinh \alpha \left( {\rho - {\rho _0}} \right) \equiv \alpha y$$
(B10)
$$\frac{{{\text{d}}y}}{{{\text{d}}\rho }}=\alpha \cosh \alpha \left( {\rho - {\rho _0}} \right) \equiv \alpha x$$
(B11)

Substituting (B10) and (B11) into (B9) yields the differential operator used to generate successive derivatives of the potential

$$\frac{{\text{d}}}{{{\text{d}}\rho }}=\alpha \left( {y\frac{\partial }{{\partial x}}+x\frac{\partial }{{\partial y}}} \right)$$
(B12)

Applying this operator to (B1) produces the first derivative

$${{\text{U}^{\prime}}}\left( \rho \right)=\frac{{\text{d}}}{{{\text{d}}\rho }}{\text{U}} \equiv \alpha \left( { - \frac{{2x}}{{{y^3}}}{{\text{U}}_1}+\frac{{2{x^2} - {y^2}}}{{{y^3}}}{{\text{U}}_2}} \right)$$
(B13)

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

$${{\text{U}^{\prime}}}\left( \rho \right)=\alpha \left( { - \frac{{2x}}{{{y^3}}}{{\text{U}}_1}+\frac{{{x^2}+1}}{{{y^3}}}{{\text{U}}_2}} \right)$$
(B14)

Evaluating at ρ = ρe (where x = xe, y = ye), and applying condition (29b), results in

$$- 2{x_\text{e} }{{\text{U}}_1}+\left( {2x_{\text{e} }^{2} - y_{\text{e} }^{2}} \right){{\text{U}}_2}=0$$
(B15)

Solving the linear system formed by (B8) and (B15) yields

$${{\text{U}}_1}=\left( {x_{\text{e} }^{2}+1} \right){D_\text{e} }$$
(B16)
$${{\text{U}}_2}=2{x_\text{e} }{D_\text{e} }$$
(B17)

Next, applying operator (B12) to (B14) gives the second derivative

$${{\text{U}^{\prime\prime}}}\left( \rho \right)={\alpha ^2}\left( {\frac{{4{x^2}+2}}{{{y^4}}}{{\text{U}}_1} - \frac{{{x^3}+5x}}{{{y^4}}}{{\text{U}}_2}} \right)$$
(B18)

At equilibrium ρ = ρe, using (B16), (B17), (B18) with condition (29c) produces

$${{\text{U}^{\prime\prime}}}\left( {{\rho _\text{e} }} \right)=2{\alpha ^2}{D_\text{e} }$$
(B19)
$$\alpha ={\text{\varvec{\uppi}}}c{\omega _{\text{e}}}\sqrt {\frac{{2\mu }}{{{D_{\text{e}}}}}}$$
(B20)

Proceeding similarly, the third derivative at equilibrium is obtained as

$${{\text{U}^{\prime\prime\prime}}}\left( {{\rho _\text{e} }} \right)= - 6{\alpha ^3}{D_\text{e} }\frac{{{x_\text{e} }}}{{{y_\text{e} }}} \equiv - 6{\alpha ^3}{D_\text{e} }\coth \alpha \left( {{\rho _\text{e} } - {\rho _0}} \right)$$
(B21)

Combining (B19), (B21), and condition (29d), and solving gives

$${\rho _0}={\rho _\text{e} } - \frac{1}{\alpha }\ln \sqrt {\left| {\frac{{1+\tfrac{{{\alpha _\text{e} }{\omega _\text{e} }}}{{6{\text{B}}_{{\text{e}}}^{{\text{2}}}}}+\alpha {\rho _\text{e} }}}{{1+\tfrac{{{\alpha _\text{e} }{\omega _\text{e} }}}{{6{\text{B}}_{{\text{e}}}^{{\text{2}}}}} - \alpha {\rho _\text{e} }}}} \right|}$$
(B22)

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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  • Received: 17 November 2025

  • Accepted: 16 April 2026

  • Published: 25 April 2026

  • DOI: https://doi.org/10.1038/s41598-026-49748-w

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Keywords

  • Magnetization
  • Ro-vibrational energy
  • Partition function
  • Diatomic molecules
  • Schrödinger equation
  • Fractional parameters
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