Halliday-Suranyi Approach to the Anharmonic Oscillator
Abstract
In this contribution to Peter Suranyi Festschrift, we study the Halliday-Suranyi perturbation method for calculating the energy eigenvalues of the quartic anharmonic oscillator.
1 Introduction
The LHC’s non-discovery of new particles that were predicted by proposed solutions to the hierarchy problem suggests that our understanding of perturbative quantum field theory (QFT) is still limited. To better understand the behavior of QFT under perturbation theory, it is prudent to go back to the basics and study the simplest possible case, which would be interacting bosonic field theory in dimensions, namely, quantum mechanics (QM) with Hamiltonian
(1) |
Here, the operators and have mass dimensions and , respectively, and , while and both have mass dimension 1. This Hamiltonian has been studied by many authors since the dawn of QM, both for practical applications and also as a testbed for various approximation techniques. [1, 2, 3].
Let us denote the eigenvalues of by , . We all know that when we have
(2) |
Treating the harmonic oscillator part of as the unperturbed Hamiltonian and the quartic part of the potential as the perturbation, i.e.
(3) |
Rayleigh-Schrödinger perturbation theory[4] gives the value of as a power series in :
(4) |
where
(5) | |||||
(6) | |||||
(7) | |||||
(8) | |||||
(9) |
However, this is a divergent asymptotic series [5, 6, 7, 8, 9, 10, 11, 12, 13, 14] and must be Borel summed to recover the values of . [15, 16, 17]
On the other hand, when we can argue on dimensional grounds that
(10) |
where is a dimensionless function of , which scales as as .[1, 2, 18] If we treat the quadratic part of the potential as the perturbation instead of the quartic part, that is:
(11) |
then the case is expandable in powers of :
(12) |
This strong-coupling expansion is convergent for .[14] However, the perturbative calculation of the coefficients is difficult due to the the unperturbed Hamiltonian lacking in simple analytic expressions for its eigenvalues and eigenfunctions.[19] Bender et al. in Ref. 20 approach this problem by treating the quartic potential part as the unperturbed Hamiltonian and the harmonic oscillator part the perturbation, i.e.
(13) |
However, this method requires the introduction of a spatial lattice to regulate the operator, and this lattice spacing must be extrapolated to zero at the end of the calculation.
2 The Halliday-Suranyi Approach
In Refs. 21 and 22, Halliday and Suranyi introduce an interesting method for dealing with the quartic anharmonic oscillator. First, note that the operator can be rewritten as
(14) | |||||
(15) |
where is an arbitrary mass parameter. This allows us to separate into the unperturbed Hamiltonian and the perturbation as follows:
(16) | |||||
(17) |
Note that by the replacement
(19) |
we discretize the eigenvalues with acting as the regulator, without the introduction of a spatial lattice. The eigenvalues of in units of are
(20) |
where . Denote the expansion of in powers of as
(21) |
The convergence of this series is demonstrated in Ref. 22. The first few terms of this expansion are given by
(22) | |||||
(24) | |||||
(35) | |||||
where we have used the shorthand
(36) |
Collecting the powers of would lead to the strong coupling expansion of \erefSCexpansion. If we set and (i.e. ) in the above expressions, we recover Eq. (2.6) of Ref. 22.
3 Choice of the parameter
Note that though every term in the expansion of \erefHSexpansion depends on , the sum that the series converges to does not since the full Hamiltonian is independent of the arbitrary parameter used to separate into and . However, when the series is truncated after a finite number of terms, the dependence on will remain. This is illustrated for the case in \frefHSfig, in which the exact numerical results for , , are compared to the 0th, 1st, 2nd, and 3rd order approximations. From \frefHSfig, it is evident that for each there is an optimum value of for which the series converges quickly and the first few terms provide a very good approximation. By inspection, we expect this value to scale as
(37) |
The question is: what is the best procedure to fix so that the resulting approximation is good? Note that the problem is similar to the renormalization scale setting problem in perturbative QCD and, consequently, we borrow some of the language used in that field.[23]
3.1 Method 1 : Fastest Apparent Convergence


In Ref. 22, Halliday and Suranyi consider demanding that
(38) |
to fix at each order . This corresponds to the method of Fastest Apparent Convergence (FAC) used in pQCD.[23] For , we need to solve
(39) |
which, in general, has one real and two complex solutions. For the (i.e. ) case, the three solutions overlap and we have
(40) |
The value of at is
(41) | |||||
(42) |
Note that this expression scales as for large as it should.
Graphically, \erefFAC is equivalent to searching for values of at which the graphs for the 0th, and th order approximations cross:
(43) |
This is illustrated for the case in \frefFACfig. The six graphs shown are for the to states, and each shows the intersections of the graph (dotted) with the (dotdashed), (short-dashed), and (long-dashed) graphs. One problem with this approach is that there exist, in general, multiple real solutions to \erefZPcondition for . From these multiple real solutions, we choose the smallest for each . This gives us the crossing point closest to the vertical axis, which are the ones shown in \frefFACfig. The values of and at these points are graphed in \frefAP1 and \frefAP2, respectively. We can see from \frefAP1 that the values for never deviate away from the case \erefZPapprox, and from \frefAP2 that, for , the value is already within 1% of the actual value.
3.2 Method 2 : Principle of Minimum Sensitivity
Another method for choosing would be to require
(44) |
This corresponds to the Principle of Minimum Sensitivity (PMS) used in pQCD.[23] For the case, PMS is equivalent to minimizing the expectation value of using the harmonic oscillator eigenfunctions as the variational trial functions.[24] Indeed, and are respectively the expectation values of and for the th eigenstate of . Imposing \erefPMScondition for , we find
(45) | |||||
(46) | |||||
(47) |
which, in general, has one real and two complex solutions. For the (i.e. ) case, we find
(48) |
and the approximate value at is [24]
(49) | |||||
(50) | |||||
(51) |
which is numerically similar to \erefZPapprox. For , PMS does not correspond to any variational calculation.
Graphically, \erefPMScondition looks for the values of for which the slope of the th order approximation is flat. This is illustrated for the case in \frefPMSfig, in which the six graphs shown are for the to states. For , there is a unique flat location as we saw above. For , there are two flat locations in which the one on the left is a local minimum while the one of the right is a local maximum. Though we cannot tell which one should be choosen beforehand, comparison with the exact results suggests we should choose the local minimum point on the left.
For , there are three flat locations, where the two outer points are local minima, while the one in the middle is a local maximum. For all the cases considered, the left local minimum is closer to the exact result than the central local maximum. For the ground state, , the right local minimum is closer to the exact result than the left local minimum, but undershoots it. For , though we cannot tell from \frefPMSfig, the right local minimum dips into the negative. Thus, we choose the left local minimum as our approximation for .


The values of chosen in this way are plotted in \frefPMS1, and the resulting approximate values normalized to the exact value are shown in \frefPMS2. At , the approximate values are within 1% of the exact value for all considered.
3.3 Method 3 : Perturbative Variational Method
The problem with \erefZPcondition and \erefPMScondition is that they do not uniquely determine for , and choosing the smallest real solution was somewhat arbitrary and there is no guarantee that this choice would be optimal. To remedy this problem, let us consider the following. Denote the perturbative expansion of the eigenstates of in powers of as
(52) |
where includes all terms proportional to powers of . We have commented in the previous subsection that
(53) | |||||
(54) |
so the PMS condition, \erefPMScondition, applied to the case minimizes using as the trial function. Now, consider the expectation value of for the state :
(55) |
Minimizing by varying should improve the approximations for the (ground state, even parity) and the (1st excited state, odd parity) cases without ever going below the exact values.
The numerator and denominator of \erefH1def are
(56) | |||||
(59) | |||||
(60) | |||||
(61) | |||||
(62) | |||||
(63) |
Therefore,
(64) |
We see that can be considered the 3rd-order perturbative energy corrected by a class of higher order terms which have been resummed into the factor . This is similar in spirit to Renormalization Group resummation, or the Brodsky-Lepage-Mackenzie method used in pQCD.[23] The correction renders positive definite, and avoids the problem has of becoming negative around the right local minimum for .
To calculate we need, in addition to \erefHSterms,
(65) | |||||
(67) | |||||
The graphs of and as well as their stationary points are shown for the case in \frefVARfig for through . Comparing the -dependence of (dashed line) and (dotted line), we can see that they both have three stationary points: two local minima and one local maximum.
For the (ground state, even parity) and (1st exited state, odd parity) cases, the global minimum of will provide the best approximation without undershooting the exact values. Indeed, comparing the graphs of (dashed line) and (dotted line) for these cases in \frefVARfig, we can see that the right local minimum has been lifted to just above the exact value. These global minima of and compared to the exact values are
(68) |
which are amazingly accurate (better than 0.1%) for a 3rd order perturbative calculation without any small expansion parameter.
For the cases, the global minimum of does not have any special meaning. Indeed, for the case we can see from \frefVARfig that the global minimum of is a poor approximation. Nevertheless, for all cases the right local minimum is now positive, and the spread of in the range between the two local minima are greatly reduced compared to that of . This is shown in \frefEHspread. For , the function is flat enough between the two local minima, so it does not matter what value of is chosen in that range.
As we continue this procedure to higher orders, we conjecture that will become flatter for a wider range of with increasing . For instance, the next function to consider in the sequence is
(69) | |||||
(71) | |||||
which we expect to have three local minima and two local maxima. The “wiggles” in between these extrema should be smaller than those of .
4 Discussion
We have studied the -value selection problem in the Halliday-Suranyi approach to the quartic anharmonic oscillator.[21, 22] We have analyzed the pure quartic potential case () and found that the FAC and PMS methods lead to fractional errors that decrease monotonically with increasing . This is in stark contrast to usual perturbation theory in which the energies of the higher excited states are more difficult to calculate.
The method can be improved by replacing the st order energy with the expectation value of for the th order state . This expectation value is positive definite, and for the (ground state) and (1st excited state) cases bounded from below by the exact energies. At the resulting approximations for the and energies are better than 0.1%. The dependence on the value of is also greatly reduced compared to , facilitating the choice of .
While this result is quite interesting in itself, the more important question is whether analogous techniques can be applied to dimensional QFT. Suggestions exist in the literature[24] but the details need to be worked out.
Acknowledgements
TT thanks P. Suranyi for his friendship over the years and L. C. R. Wijewardhana for inviting him to contribute to Peter Suranyi Festschrift. Helpful discussions with D. Minic and C. H. Tze are gratefully acknowledged. TT and NB are supported in part by the U.S. Department of Energy (DE-SC0020262, Task C).
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