Category: Physics

  • The Path to Perturbation Theory

    “Almost no problems are exactly solvable”

    Carl Bender

    In physics, most problems—from the anharmonic oscillator to Quantum Electrodynamics (QED)— cannot be solved exactly. We rely on Perturbation Theory, expanding the solution in powers of a small coupling constant (often denoted λ or α).

    A classic example is the quantum anharmonic oscillator, where the Hamiltonian is

    \displaystyle H = \frac{p^2}{2m} + \frac{1}{2} m \omega^2 x^2 + \lambda x^4

    (with the quartic term treated as a small perturbation λ ≪ 1). Another famous case is QED, where the fine-structure constant α ≈ 1/137 serves as the small parameter for expanding processes involving electrons and photons.

    The challenge? These perturbative expansions are almost always asymptotic series with a null radius of convergence. The coefficients a_n typically grow factorially as n! (or even faster), making the series eventually diverge regardless of how small the coupling constant is.

    For instance, in the anharmonic oscillator, the perturbative corrections to the energy levels involve terms whose coefficients grow like n!, leading to a divergent series for any nonzero λ. Similarly, in QED, the perturbative series for quantities like the electron’s anomalous magnetic moment (g−2) is asymptotic: it gives spectacular agreement with experiment up to high orders, but diverges if pushed too far.

    This is where our journey pays off. By applying Borel resummation and Padé approximants to these divergent series, we can extract non-perturbative information and obtain remarkably accurate physical predictions. In quantum field theory, Borel summation helps recover meaningful results from perturbative expansions (for example, in certain Euclidean field theories or by handling contributions from instantons and renormalons). Padé approximants are routinely used to accelerate convergence and estimate the behavior of series in QCD and other models.

    In our upcoming posts, we will see how this mathematical framework becomes the essential language of modern theoretical physics.

  • Summation Techniques for Perturbation Theory

    After several months of exploring various summation and acceleration methods, it is time to synthesize these tools before we apply them to one of their most important domains: Perturbation Theory.

    When a power series \displaystyle \sum_{n=0}^\infty a_n z^{n} has a small or even zero radius of convergence, or converges too slowly to be numerically useful, we require more than standard arithmetic. Here is a recap of the methods we have covered and how they bridge the gap between formal series and numerical values.


    Summation Methods: Taming Divergence

    • Borel and Borel–Écalle: By using the Borel transform, we transform factorially growing coefficients into a convergent series in the Borel plane. The Borel–Écalle framework further allows us to handle singularities via resurgence theory, providing a unique “resummed” value even for non-Borel-summable series.
    • Euler and Zeta summation: These methods assign finite values to divergent sums by analytic continuation. While Euler summation is ideal for alternating series, Zeta summation provides a powerful way to handle the infinite sums that frequently appear in quantum vacuum energy calculations.
    • Generic summation: Beyond these classical approaches, we have also explored the idea of generic summation, which provides a unifying framework for assigning values to divergent or slowly convergent series.

    Acceleration Techniques: Enhancing Convergence

    • Shanks Transformation and Padé Approximants: These nonlinear transformations (often related to continued fractions) excel at capturing the behavior of functions beyond their radius of convergence, particularly when poles are present.
    • Richardson Extrapolation: A fundamental tool for numerical analysis that cancels out the leading error terms, allowing us to estimate the limit of a sequence Sn with much higher precision from only a few terms.

    An important consistency check underlies all these techniques: whenever different summation or acceleration methods apply to the same series, they agree on a common value. This convergence of independent approaches is not accidental, it reflects the fact that these methods capture an underlying analytic object beyond the formal series itself. When they work, they do not merely assign a value: they reveal a coherent extension of the function that the original divergent expansion was hinting at.

  • Anharmonic oscillator II

    Remember that the perturbative series for the anharmonic oscillator is

    Anharmonic oscillator I

    \displaystyle E_0(\epsilon) = \frac{1}{2} + \frac{3}{4}\epsilon - \frac{21}{8}\epsilon^2 + \frac{333}{16}\epsilon^3 + \mathcal{O}(\epsilon^4)

    We used Padé approximants to compute the ground state energy E_0(\epsilon). Now we aim to calculate E_0(\epsilon) using Borel summation. The (formal) Borel sum is given by

    \displaystyle \int_{0}^{\infty} e^{-t} \sum_{n=0}^\infty \frac{a_n}{n!} (\epsilon t)^n \, dt.

    Using the first three coefficients of the perturbative series, the truncated Borel transform is approximated by

    \displaystyle \mathcal{B}E_0(t) \approx \frac{1}{2} + \frac{3}{4} t - \frac{21}{16} t^2,

    so the truncated Borel sum writes

    \displaystyle E_0(\epsilon) \approx \int_0^\infty e^{-t} \left(\frac{1}{2} + \frac{3}{4} \epsilon t - \frac{21}{16} \epsilon^2 t^2 \right) dt = \frac{1}{2} + \frac{3}{4} \epsilon - \frac{21}{8} \epsilon^2.

    since

    \displaystyle \int_0^\infty \frac{1}{2} e^{-t} \, dt = \frac{1}{2}
    \displaystyle \int_0^\infty e^{-t} \cdot \frac{3}{4} \epsilon \, t \, dt = \frac{3}{4} \epsilon
    \displaystyle \int_0^\infty e^{-t} \cdot \left( -\frac{21}{16} \epsilon^2 t^2 \right) dt = -\frac{21}{8} \epsilon^2

    This doesn’t really seem like progress, since the first terms of the Borel sum are identical to those of the perturbative expansion. The perturbative expansion E_0(\epsilon) = \sum_{n=0}^\infty a_n \epsilon^n above has coefficients that grow factorially. Bender and Wu showed that for large n,

    \displaystyle a_n \sim -r\, (-1)^n \left(\frac{3}{2}\right)^n \Gamma\!\left(n+\tfrac12\right), \qquad r>0.

    Since

    \displaystyle \Gamma\!\left(n+\tfrac12\right) \sim n!\, n^{-1/2},
    formule avec n! en rouge et gras

    thus the series diverges for all \epsilon \neq 0.

    Borel summation improves convergence by dividing out this factorial growth.

    In summary, even with just a few terms, Borel summation correctly recovers the perturbative results for the anharmonic oscillator then It turns the divergent series into a well-defined and useful result.

  • Anharmonic oscillator I

    We would like to illustrate the use of Padé approximants in the context of the anharmonic oscillator. A harmonic oscillator is an oscillating system that experiences a restoring force. Anharmonicity is the deviation of a system from being a harmonic oscillator. The anharmonic oscillator is described by the following differential equation:

    \displaystyle \left(-\frac{d^2}{dx^2} + x^2 + x^4\right) \phi(x) = E_n \phi(x)

    This differential equation is very hard to solve exactly. In order to obtain an approximate solution, we can use perturbation theory. By inserting a small dimensionless parameter \epsilon, the equation becomes:

    \displaystyle \left(-\frac{d^2}{dx^2} + x^2 + \epsilon x^4\right) \phi(x) = E_n(\epsilon) \phi(x)

    If we are interested in the energy levels, the basic idea is to write E_n(\epsilon) as a geometric series. For the ground state E_0 we write:

    \displaystyle E_0(\epsilon) = \sum_{n=0}^{\infty} E_{0,n} \epsilon^n

    The solution is a divergent perturbation series (C.M. Bender and T.T. Wu, Phys. Rev. 184, 1969):

    \displaystyle E_0(\epsilon) = \frac{1}{2} + \frac{3}{4}\epsilon - \frac{21}{8}\epsilon^2 + \frac{333}{16}\epsilon^3 + \mathcal{O}(\epsilon^4)

    Let’s calculate the P(1,1) approximant of E_0 using the techniques presented in post Computing Padé approximants:

    \displaystyle P(1,1) = \frac{A_0 + A_1 \epsilon}{1 + B_1 \epsilon} = C_0 + C_1 \epsilon + C_2 \epsilon^2

    Solving the linear systems for computing Padé approximants sequentially leads to:

    \displaystyle C_1 B_1 = - C_2 \implies B_1 = -\frac{C_2}{C_1}
    \displaystyle \frac{3}{4} B_1 = \frac{21}{8} \implies B_1 = \frac{84}{24} = \frac{7}{2}
    \displaystyle \begin{pmatrix} C_0 & 0 \\ C_1 & C_0 \\ \end{pmatrix} \begin{pmatrix} 1 \\ B_1 \end{pmatrix} = \begin{pmatrix} A_0 \\ A_1 \end{pmatrix}
    \displaystyle \begin{pmatrix} \frac{1}{2} & 0 \\ \frac{3}{4} & \frac{1}{2} \\ \end{pmatrix} \begin{pmatrix} 1 \\ \frac{7}{2} \end{pmatrix} = \begin{pmatrix} \frac{1}{2} \\ \frac{3}{4} + \frac{7}{4} \end{pmatrix}
    \displaystyle P(1,1)_{E_0} = \frac{\frac{1}{2} + \left(\frac{3}{4} + \frac{7}{4}\right)\epsilon}{1 + \frac{7}{2}\epsilon}

    Setting \epsilon = 1 (to recover the initial differential equation) we have:

    \displaystyle P(1,1)_{E_0} = \frac{\frac{1}{2} + \frac{3}{4} + \frac{7}{4}}{1 + \frac{7}{2}} = 0.6666

    The P(4,4)_{E_0} = 1.3838 and the exact solution is 1.3924.

    The relative error (definition here) of the approximant P(4,4)_{E_0} is:

    \displaystyle \text{Relative error} = \frac{1.3838 - 1.3924}{1.3924} = -0.0062

    It’s therefore interesting to note that in order to solve a very difficult differential equation, we can use perturbation theory. In the case of the anharmonic oscillator, the perturbative series is divergent. Using Padé approximants, we can make use of a divergent perturbative series and approximate the exact answer arbitrarily.