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Halliday-Suranyi Approach to the Anharmonic Oscillator

Nabin Bhatta111[email protected] and Tatsu Takeuchi222[email protected] Center for Neutrino Physics, Department of Physics
Virginia Tech, Blacksburg VA 24061, USA
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.

\bodymatter

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 0+10+1 dimensions, namely, quantum mechanics (QM) with Hamiltonian

H^=12p^2+12m2q^2+14M3q^4.\hat{H}\,=\,\dfrac{1}{2}\hat{p}^{2}+\dfrac{1}{2}m^{2}\hat{q}^{2}+\dfrac{1}{4}M^{3}\hat{q}^{4}\;. (1)

Here, the operators q^\hat{q} and p^\hat{p} have mass dimensions 12-\frac{1}{2} and +12+\frac{1}{2}, respectively, and [q^,p^]=i[\hat{q},\hat{p}]=i, while mm and MM 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 H^\hat{H} by En(m,M)E_{n}(m,M), n=0,1,2,n=0,1,2,\cdots. We all know that when M=0M=0 we have

En(m,0)=m(n+12).E_{n}(m,0)\;=\;m\left(n+\frac{1}{2}\right)\;. (2)

Treating the harmonic oscillator part of H^\hat{H} as the unperturbed Hamiltonian and the quartic part of the potential as the perturbation, i.e.

H^0=12p^2+12m2q^2,V^=14M3q^4,\hat{H}_{0}\,=\,\dfrac{1}{2}\hat{p}^{2}+\dfrac{1}{2}m^{2}\hat{q}^{2}\;,\qquad\hat{V}\,=\,\dfrac{1}{4}M^{3}\hat{q}^{4}\;, (3)

Rayleigh-Schrödinger perturbation theory[4] gives the value of En(m,M)E_{n}(m,M) as a power series in λ=(M/m)3\lambda=(M/m)^{3} :

En(m,M)=m[c0(n)+λc1(n)+λ2c2(n)+λ3c3(n)+],E_{n}(m,M)\;=\;m\bigg{[}c_{0}(n)+\lambda\,c_{1}(n)+\lambda^{2}c_{2}(n)+\lambda^{3}c_{3}(n)+\cdots\bigg{]}\;, (4)

where

c0(n)\displaystyle c_{0}(n) =\displaystyle= n+12,\displaystyle n+\frac{1}{2}\;,\vphantom{\bigg{|}} (5)
c1(n)\displaystyle c_{1}(n) =\displaystyle= 3(2n2+2n+1)16,\displaystyle\dfrac{3(2n^{2}+2n+1)}{16}\;,\vphantom{\bigg{|}} (6)
c2(n)\displaystyle c_{2}(n) =\displaystyle= 34n3+51n2+59n+21128,\displaystyle-\dfrac{34n^{3}+51n^{2}+59n+21}{128}\;,\vphantom{\bigg{|}} (7)
c3(n)\displaystyle c_{3}(n) =\displaystyle= 3(125n4+250n3+472n2+347n+111)1024,\displaystyle\dfrac{3(125n^{4}+250n^{3}+472n^{2}+347n+111)}{1024}\;,\vphantom{\bigg{|}} (8)
\displaystyle\vdots (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 En(m,M)E_{n}(m,M). [15, 16, 17]

On the other hand, when m=0m=0 we can argue on dimensional grounds that

En(0,M)=MA0(n),E_{n}(0,M)\;=\;M\,A_{0}(n)\;, (10)

where A0(n)A_{0}(n) is a dimensionless function of nn, which scales as n4/3\sim n^{4/3} as nn\to\infty.[1, 2, 18] If we treat the quadratic part of the potential as the perturbation instead of the quartic part, that is:

H^0=12p^2+14M3q^4,V^=12m2q^2,\hat{H}_{0}\,=\,\dfrac{1}{2}\hat{p}^{2}+\dfrac{1}{4}M^{3}\hat{q}^{4}\;,\qquad\hat{V}\,=\,\dfrac{1}{2}m^{2}\hat{q}^{2}\;, (11)

then the m0m\neq 0 case is expandable in powers of λ2/3=(m/M)2\lambda^{-2/3}=(m/M)^{2} :

En(m,M)=M[A0(n)+A1(n)λ2/3+A2(n)λ4/3+].E_{n}(m,M)\;=\;M\bigg{[}A_{0}(n)+\dfrac{A_{1}(n)}{\lambda^{2/3}}+\dfrac{A_{2}(n)}{\lambda^{4/3}}+\cdots\bigg{]}\;. (12)

This strong-coupling expansion is convergent for λ1\lambda\gg 1.[14] However, the perturbative calculation of the coefficients Ak(n)A_{k}(n) is difficult due to the the unperturbed Hamiltonian H^0\hat{H}_{0} 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.

H^0=14M3q^4,V^=12p^2+12m2q^2.\hat{H}_{0}\;=\;\frac{1}{4}M^{3}\hat{q}^{4}\;,\qquad\hat{V}\;=\;\frac{1}{2}\hat{p}^{2}+\dfrac{1}{2}m^{2}\hat{q}^{2}\;. (13)

However, this method requires the introduction of a spatial lattice to regulate the q^4\hat{q}^{4} 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 q^4\hat{q}^{4} operator can be rewritten as

14q^4\displaystyle\dfrac{1}{4}\,\hat{q}^{4} =\displaystyle= 1Ω4(12Ω2q^2)2\displaystyle\dfrac{1}{\Omega^{4}}\left(\dfrac{1}{2}\Omega^{2}\hat{q}^{2}\right)^{2}\vphantom{\Bigg{|}} (14)
=\displaystyle= 1Ω4{(p^22+12Ω2q^2)2Ω24(p^2q^2+q^2p^2)p^44},\displaystyle\dfrac{1}{\Omega^{4}}\left\{\left(\dfrac{\hat{p}^{2}}{2}+\dfrac{1}{2}\Omega^{2}\hat{q}^{2}\right)^{2}-\dfrac{\Omega^{2}}{4}\left(\hat{p}^{2}\hat{q}^{2}+\hat{q}^{2}\hat{p}^{2}\right)-\dfrac{\hat{p}^{4}}{4}\right\}\;,\vphantom{\Bigg{|}} (15)

where Ω\Omega is an arbitrary mass parameter. This allows us to separate H^\hat{H} into the unperturbed Hamiltonian H^0\hat{H}_{0} and the perturbation V^\hat{V} as follows:

H^\displaystyle\hat{H} =\displaystyle= 14M3q^4+(p^22+12m2q^2)\displaystyle\dfrac{1}{4}M^{3}\hat{q}^{4}+\left(\dfrac{\hat{p}^{2}}{2}+\dfrac{1}{2}m^{2}\hat{q}^{2}\right)\vphantom{\Bigg{|}} (16)
=\displaystyle= M3Ω4(p^22+12Ω2q^2)2H^0+(p^22+12m2q^2)M3Ω4{Ω24(p^2q^2+q^2p^2)+p^44}V^.\displaystyle\underbrace{\dfrac{M^{3}}{\Omega^{4}}\left(\dfrac{\hat{p}^{2}}{2}+\dfrac{1}{2}\Omega^{2}\hat{q}^{2}\right)^{2}}_{\displaystyle\hat{H}_{0}}+\underbrace{\left(\dfrac{\hat{p}^{2}}{2}+\dfrac{1}{2}m^{2}\hat{q}^{2}\right)-\dfrac{M^{3}}{\Omega^{4}}\left\{\dfrac{\Omega^{2}}{4}\left(\hat{p}^{2}\hat{q}^{2}+\hat{q}^{2}\hat{p}^{2}\right)+\dfrac{\hat{p}^{4}}{4}\right\}}_{\displaystyle\hat{V}}\;. (17)

Note that by the replacement

14M3q^4M3Ω4(p^22+12Ω2q^2)2\dfrac{1}{4}M^{3}\hat{q}^{4}\quad\to\quad\dfrac{M^{3}}{\Omega^{4}}\left(\dfrac{\hat{p}^{2}}{2}+\dfrac{1}{2}\Omega^{2}\hat{q}^{2}\right)^{2} (19)

we discretize the eigenvalues H^0\hat{H}_{0} with Ω\Omega acting as the regulator, without the introduction of a spatial lattice. The eigenvalues of H^0\hat{H}_{0} in units of MM are

En(0)(Z)=MZ2/3(n+12)2,n= 0,1,2,,E_{n}^{(0)}(Z)\;=\;\dfrac{M}{Z^{2/3}}\left(n+\dfrac{1}{2}\right)^{2}\;,\qquad n\;=\;0,1,2,\cdots\;, (20)

where Z=(Ω/M)3Z=(\Omega/M)^{3}. Denote the expansion of En(m,M)E_{n}(m,M) in powers of V^\hat{V} as

En(m,M)\displaystyle E_{n}(m,M) =\displaystyle= En(0)(Z)+En(1)(Z)+En(2)(Z)+En(3)(Z)+\displaystyle E_{n}^{(0)}(Z)+E_{n}^{(1)}(Z)+E_{n}^{(2)}(Z)+E_{n}^{(3)}(Z)+\cdots (21)

The convergence of this series is demonstrated in Ref. 22. The first few terms of this expansion are given by

En(1)(Z)=MZ2/3(2n+14Z(1+X)10n2+10n+116),\displaystyle E_{n}^{(1)}(Z)\;=\;\dfrac{M}{Z^{2/3}}\bigg{(}\dfrac{2n+1}{4}Z(1\!+\!X)-\dfrac{10n^{2}+10n+1}{16}\bigg{)}\;, (22)
En(2)(Z)=MZ2/3[3(n4+2n32n23n3)27(2n3)(2n+5)\displaystyle E_{n}^{(2)}(Z)\;=\;-\dfrac{M}{Z^{2/3}}\Bigg{[}\dfrac{3(n^{4}+2n^{3}-2n^{2}-3n-3)}{2^{7}(2n-3)(2n+5)} (24)
n(n1)25(2n1)(Z(1X)2n12)2+(n+1)(n+2)25(2n+3)(Z(1X)2n+32)2],\displaystyle-\dfrac{n(n-1)}{2^{5}(2n-1)}\bigg{(}Z(1\!-\!X)-\dfrac{2n-1}{2}\bigg{)}^{2}+\dfrac{(n+1)(n+2)}{2^{5}(2n+3)}\bigg{(}Z(1\!-\!X)-\dfrac{2n+3}{2}\bigg{)}^{2}\Bigg{]}\;,\vphantom{\Bigg{|}}
En(3)(Z)=MZ2/3[\displaystyle E_{n}^{(3)}(Z)\;=\;\dfrac{M}{Z^{2/3}}\Bigg{[} (35)
(n+1)(n+2)4(2n+3)2(Z(1X)42n+38)2(2n+54Z(1+X)10n2+50n+6116)\displaystyle\dfrac{(n+1)(n+2)}{4(2n+3)^{2}}\bigg{(}\dfrac{Z(1-X)}{4}-\dfrac{2n+3}{8}\bigg{)}^{2}\bigg{(}\dfrac{2n+5}{4}Z(1\!+\!X)-\dfrac{10n^{2}+50n+61}{16}\bigg{)}\vphantom{\Bigg{|}}
+n(n1)4(2n1)2(Z(1X)42n18)2(2n34Z(1+X)10n230n+2116)\displaystyle+\dfrac{n(n-1)}{4(2n-1)^{2}}\bigg{(}\dfrac{Z(1-X)}{4}-\dfrac{2n-1}{8}\bigg{)}^{2}\bigg{(}\dfrac{2n-3}{4}Z(1\!+\!X)-\dfrac{10n^{2}-30n+21}{16}\bigg{)}\vphantom{\Bigg{|}}
+(n+1)(n+2)(n+3)(n+4)26(2n+5)(2n+3)(Z(1X)42n+38)(Z(1X)42n+78)\displaystyle+\dfrac{(n+1)(n+2)(n+3)(n+4)}{2^{6}(2n+5)(2n+3)}\bigg{(}\dfrac{Z(1-X)}{4}-\dfrac{2n+3}{8}\bigg{)}\bigg{(}\dfrac{Z(1-X)}{4}-\dfrac{2n+7}{8}\bigg{)}\vphantom{\Bigg{|}}
n(n1)(n+1)(n+2)25(2n+3)(2n1)(Z(1X)42n18)(Z(1X)42n+38)\displaystyle-\dfrac{n(n-1)(n+1)(n+2)}{2^{5}(2n+3)(2n-1)}\bigg{(}\dfrac{Z(1-X)}{4}-\dfrac{2n-1}{8}\bigg{)}\bigg{(}\dfrac{Z(1-X)}{4}-\dfrac{2n+3}{8}\bigg{)}\vphantom{\Bigg{|}}
+n(n1)(n2)(n3)26(2n1)(2n3)(Z(1X)42n58)(Z(1X)42n18)\displaystyle+\dfrac{n(n-1)(n-2)(n-3)}{2^{6}(2n-1)(2n-3)}\bigg{(}\dfrac{Z(1-X)}{4}-\dfrac{2n-5}{8}\bigg{)}\bigg{(}\dfrac{Z(1-X)}{4}-\dfrac{2n-1}{8}\bigg{)}\vphantom{\Bigg{|}}
+(n+1)(n+2)(n+3)(n+4)212(2n+5)2(2n+94Z(1+X)10n2+90n+20116)\displaystyle+\dfrac{(n+1)(n+2)(n+3)(n+4)}{2^{12}(2n+5)^{2}}\bigg{(}\dfrac{2n+9}{4}Z(1+X)-\dfrac{10n^{2}+90n+201}{16}\bigg{)}\vphantom{\Bigg{|}}
+n(n1)(n2)(n3)212(2n3)2(2n74Z(1+X)10n270n+12116)\displaystyle+\dfrac{n(n-1)(n-2)(n-3)}{2^{12}(2n-3)^{2}}\bigg{(}\dfrac{2n-7}{4}Z(1+X)-\dfrac{10n^{2}-70n+121}{16}\bigg{)}\vphantom{\Bigg{|}}
{(n+1)(n+2)4(2n+3)2(Z(1X)42n+38)2+(n+1)(n+2)(n+3)(n+4)212(2n+5)2\displaystyle-\Bigg{\{}\dfrac{(n+1)(n+2)}{4(2n+3)^{2}}\bigg{(}\dfrac{Z(1-X)}{4}-\dfrac{2n+3}{8}\bigg{)}^{2}+\dfrac{(n+1)(n+2)(n+3)(n+4)}{2^{12}(2n+5)^{2}}\vphantom{\Bigg{|}}
+n(n1)4(2n1)2(Z(1X)42n18)2+n(n1)(n2)(n3)212(2n3)2}\displaystyle\quad+\dfrac{n(n-1)}{4(2n-1)^{2}}\bigg{(}\dfrac{Z(1-X)}{4}-\dfrac{2n-1}{8}\bigg{)}^{2}+\dfrac{n(n-1)(n-2)(n-3)}{2^{12}(2n-3)^{2}}\Bigg{\}}\vphantom{\Bigg{|}}
×(2n+14Z(1+X)10n2+10n+116)],\displaystyle\quad\times\bigg{(}\dfrac{2n+1}{4}Z(1+X)-\dfrac{10n^{2}+10n+1}{16}\bigg{)}\Bigg{]}\;,\vphantom{\Bigg{|}}

where we have used the shorthand

X=m2Ω2=1(λZ)2/3.X\;=\;\dfrac{m^{2}}{\Omega^{2}}\;=\;\dfrac{1}{(\lambda Z)^{2/3}}\;. (36)

Collecting the powers of XX would lead to the strong coupling expansion of \erefSCexpansion. If we set n=0n=0 and X=0X=0 (i.e. m=0m=0) in the above expressions, we recover Eq. (2.6) of Ref. 22.

3 Choice of the parameter ZZ

Note that though every term in the expansion of \erefHSexpansion depends on Z=(Ω/M)3Z=(\Omega/M)^{3}, the sum that the series converges to does not since the full Hamiltonian H^\hat{H} is independent of the arbitrary parameter Ω\Omega used to separate H^\hat{H} into H^0\hat{H}_{0} and V^\hat{V}. However, when the series is truncated after a finite number of terms, the dependence on ZZ will remain. This is illustrated for the m=0m=0 case in \frefHSfig, in which the exact numerical results for A0(n)A_{0}(n), n=0,1,,5n=0,1,\cdots,5, are compared to the 0th, 1st, 2nd, and 3rd order approximations. From \frefHSfig, it is evident that for each nn there is an optimum value of ZZ 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

Zn+1.Z\;\sim\;n+1\;. (37)

The question is: what is the best procedure to fix ZZ 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]

Refer to caption

Figure 1: The Halliday-Suranyi expansion for the m=0m=0 case compared with the exact result for the states n=0n=0 through n=5n=5. Dotted line: 0th order, dot-dashed line: 1st order, short-dashed line: 2nd order, long-dashed line: 3rd order, solid horizontal line: exact value. We can see that the optimum value of ZZ for state nn is Zn+1Z\sim n+1.

3.1 Method 1 : Fastest Apparent Convergence

Refer to caption
Refer to caption
Figure 2: (a) Mimimim values of ZZ that solve \erefZPcondition for the X=0X=0 case, and (b) approximate over exact values of En(0,M)E_{n}(0,M) at those ZZ. Results are shown for k=1k=1 (diamonds, dotdashed), k=2k=2 (squares, short-dashed), and k=3k=3 (circles, long-dashed). The three lines are overlapping in (a) and difficult to distinguish.

In Ref. 22, Halliday and Suranyi consider demanding that

En(m,M)En(0)(Z)+En(1)(Z)+En(2)(Z)++En(k)(Z)=0E_{n}(m,M)\;\approx\;E_{n}^{(0)}(Z)+\underbrace{E_{n}^{(1)}(Z)+E_{n}^{(2)}(Z)+\cdots+E_{n}^{(k)}(Z)}_{\displaystyle=0} (38)

to fix ZZ at each order kk. This corresponds to the method of Fastest Apparent Convergence (FAC) used in pQCD.[23] For k=1k=1, we need to solve

En(1)(Z)= 0Z+m2M2Z1/35(n2+n+110)4(n+12)= 0,E_{n}^{(1)}(Z)\,=\,0\quad\to\quad Z+\frac{m^{2}}{M^{2}}Z^{1/3}-\dfrac{5\left(n^{2}+n+\frac{1}{10}\right)}{4\left(n+\frac{1}{2}\right)}\,=\,0\;, (39)

which, in general, has one real and two complex solutions. For the m=0m=0 (i.e. X=0X=0) case, the three solutions overlap and we have

Z=Zn,FAC(1)5(n2+n+110)4(n+12)n154(n+12).Z\;=\;Z_{n,\text{FAC}}^{(1)}\;\equiv\;\dfrac{5\left(n^{2}+n+\frac{1}{10}\right)}{4\left(n+\frac{1}{2}\right)}\;\xrightarrow{n\gg 1}\;\frac{5}{4}\bigg{(}n+\frac{1}{2}\bigg{)}\;. (40)

The value of En(0)(Z)E_{n}^{(0)}(Z) at Z=Zn,FAC(1)Z=Z_{n,\text{FAC}}^{(1)} is

En(0)(Zn,FAC(1))\displaystyle E_{n}^{(0)}(Z_{n,\text{FAC}}^{(1)}) =\displaystyle= M(45)2/3[(n+12)4(n2+n+110)]2/3\displaystyle M\bigg{(}\dfrac{4}{5}\bigg{)}^{2/3}\bigg{[}\dfrac{(n+\frac{1}{2})^{4}}{(n^{2}+n+\frac{1}{10})}\bigg{]}^{2/3}\vphantom{\Bigg{|}} (41)
n1\displaystyle\xrightarrow{n\gg 1} M(45)2/3(n+12)4/3= 0.862M(n+12)4/3.\displaystyle M\bigg{(}\dfrac{4}{5}\bigg{)}^{2/3}\bigg{(}n+\frac{1}{2}\bigg{)}^{4/3}=\;0.862\,M\bigg{(}n+\frac{1}{2}\bigg{)}^{4/3}\;. (42)

Note that this expression scales as n4/3\sim n^{4/3} for large nn as it should.

Graphically, \erefFAC is equivalent to searching for values of ZZ at which the graphs for the 0th, and kkth order approximations cross:

En(0)(Z)=j=0kEn(j)(Z).E_{n}^{(0)}(Z)\;=\;\sum_{j=0}^{k}E_{n}^{(j)}(Z)\;. (43)

Refer to caption

Figure 3: Blowups of \frefHSfig showing the crossing points of the 0th order (dotted) with the 1st (dot-dashed), 2nd (short-dashed), and 3rd (long-dashed) order approximations. The 2nd and 3rd order lines can have multiple crossings with the 0th order line. Here, we show the crossings with the smallest values of ZZ.

This is illustrated for the X=0X=0 case in \frefFACfig. The six graphs shown are for the n=0n=0 to n=5n=5 states, and each shows the intersections of the k=0k=0 graph (dotted) with the k=1k=1 (dotdashed), k=2k=2 (short-dashed), and k=3k=3 (long-dashed) graphs. One problem with this approach is that there exist, in general, multiple real solutions to \erefZPcondition for k2k\geq 2. From these multiple real solutions, we choose the smallest ZZ for each kk. This gives us the crossing point closest to the vertical axis, which are the ones shown in \frefFACfig. The values of ZZ and En(0)(Z)E_{n}^{(0)}(Z) at these points are graphed in \frefAP1 and \frefAP2, respectively. We can see from \frefAP1 that the ZZ values for k2k\geq 2 never deviate away from the k=1k=1 case \erefZPapprox, and from \frefAP2 that, for n2n\geq 2, the k=1k=1 value is already within 1% of the actual value.

3.2 Method 2 : Principle of Minimum Sensitivity

Another method for choosing ZZ would be to require

ddZ[j=0kEn(j)(Z)]= 0.\dfrac{d}{dZ}\bigg{[}\sum_{j=0}^{k}E_{n}^{(j)}(Z)\bigg{]}\;=\;0\;. (44)

This corresponds to the Principle of Minimum Sensitivity (PMS) used in pQCD.[23] For the k=1k=1 case, PMS is equivalent to minimizing the expectation value of H^=H^0+V^\hat{H}=\hat{H}_{0}+\hat{V} using the harmonic oscillator eigenfunctions as the variational trial functions.[24] Indeed, En(0)(Z)E_{n}^{(0)}(Z) and En(1)(Z)E_{n}^{(1)}(Z) are respectively the expectation values of H^0\hat{H}_{0} and V^\hat{V} for the nnth eigenstate of H^0\hat{H}_{0}. Imposing \erefPMScondition for k=1k=1, we find

ddZ[En(0)(Z)+En(1)(Z)]\displaystyle\dfrac{d}{dZ}\Big{[}E_{n}^{(0)}(Z)+E_{n}^{(1)}(Z)\Big{]} =\displaystyle= 0\displaystyle 0 (45)
\displaystyle\downarrow (46)
Zm2M2Z1/33(n2+n+12)2(n+12)\displaystyle Z-\frac{m^{2}}{M^{2}}Z^{1/3}-\dfrac{3\left(n^{2}+n+\frac{1}{2}\right)}{2\left(n+\frac{1}{2}\right)} =\displaystyle= 0,\displaystyle 0\;, (47)

which, in general, has one real and two complex solutions. For the m=0m=0 (i.e. X=0X=0) case, we find

Z=Zn,PMS(1)3(n2+n+12)2(n+12)n132(n+12),Z\;=\;Z_{n,\text{PMS}}^{(1)}\;\equiv\;\dfrac{3\left(n^{2}+n+\frac{1}{2}\right)}{2\left(n+\frac{1}{2}\right)}\;\xrightarrow{n\gg 1}\;\dfrac{3}{2}\bigg{(}n+\frac{1}{2}\bigg{)}\;, (48)

and the approximate value at Z=Zn,PMS(1)Z=Z_{n,\text{PMS}}^{(1)} is [24]

En(0)(Zn,PMS(1))+En(1)(Zn,PMS(1))\displaystyle E_{n}^{(0)}(Z_{n,\text{PMS}}^{(1)})+E_{n}^{(1)}(Z_{n,\text{PMS}}^{(1)}) (49)
=\displaystyle= M34/327/3[(n+12)2(n2+n+12)]1/3\displaystyle M\,\dfrac{3^{4/3}}{2^{7/3}}\bigg{[}\bigg{(}n+\frac{1}{2}\bigg{)}^{2}\bigg{(}n^{2}+n+\frac{1}{2}\bigg{)}\bigg{]}^{1/3}\vphantom{\Bigg{|}} (50)
n1\displaystyle\xrightarrow{n\gg 1} M34/327/3(n+12)4/3= 0.859M(n+12)4/3,\displaystyle M\,\dfrac{3^{4/3}}{2^{7/3}}\bigg{(}n+\frac{1}{2}\bigg{)}^{4/3}\;=\;0.859\,M\bigg{(}n+\frac{1}{2}\bigg{)}^{4/3}\;, (51)

which is numerically similar to \erefZPapprox. For k2k\geq 2, PMS does not correspond to any variational calculation.

Refer to caption


Figure 4: The Principle of Minimum Sensitivity (PMS) applied to the states n=0n=0 through n=5n=5. The diamonds, squared, and circles respectively show the points at which the 1st (dot-dashed), 2nd (short-dashed), and 3rd (long-dashed) order approximations are flat. The 2nd order graph has two flat points, with the left point giving a local minimum, and the right point a local maximum. The 3rd order graph has three flat points, with the left-most and right-most points giving local minima, and the middle point a local maximum. However, the right local minimum always undershoots the exact value for all nn, and dips into the negative for n2n\geq 2.

Graphically, \erefPMScondition looks for the values of ZZ for which the slope of the kkth order approximation is flat. This is illustrated for the X=0X=0 case in \frefPMSfig, in which the six graphs shown are for the n=0n=0 to n=5n=5 states. For k=1k=1, there is a unique flat location as we saw above. For k=2k=2, 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 k=3k=3, 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, n=0n=0, the right local minimum is closer to the exact result than the left local minimum, but undershoots it. For n2n\geq 2, 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 En(0,M)E_{n}(0,M).

Refer to caption
Refer to caption
Figure 5: (a) Mimimim values of ZZ that solve \erefPMScondition for the X=0X=0 case, and (b) approximate over exact values of En(0,M)E_{n}(0,M) at those ZZ. Results are shown for k=1k=1 (diamonds, dotdashed), k=2k=2 (squares, short-dashed), and k=3k=3 (circles, long-dashed).

The values of ZZ chosen in this way are plotted in \frefPMS1, and the resulting approximate values normalized to the exact value are shown in \frefPMS2. At k=3k=3, the approximate values are within 1% of the exact value for all nn considered.

3.3 Method 3 : Perturbative Variational Method

The problem with \erefZPcondition and \erefPMScondition is that they do not uniquely determine ZZ for k2k\geq 2, 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 H^\hat{H} in powers of V^\hat{V} as

|n=|n(0)+|n(1)+|n(2)+|n(3)+,|n\rangle\;=\;|n^{(0)}\rangle+|n^{(1)}\rangle+|n^{(2)}\rangle+|n^{(3)}\rangle+\cdots\;, (52)

where |n(k)|n^{(k)}\rangle includes all terms proportional to kk powers of V^\hat{V}. We have commented in the previous subsection that

Hn(0)n(0)|H^|n(0)n(0)|n(0)\displaystyle\langle H\rangle_{n}^{(0)}\;\equiv\;\dfrac{\langle n^{(0)}|\hat{H}|n^{(0)}\rangle}{\langle n^{(0)}|n^{(0)}\rangle} =\displaystyle= n(0)|(H^0+V^)|n(0)\displaystyle\langle n^{(0)}|\Big{(}\hat{H}_{0}+\hat{V}\Big{)}|n^{(0)}\rangle\vphantom{\bigg{|}} (53)
=\displaystyle= n(0)|H^0|n(0)En(0)+n(0)|V^|n(0)En(1),\displaystyle\underbrace{\langle n^{(0)}|\hat{H}_{0}|n^{(0)}\rangle}_{\displaystyle E_{n}^{(0)}}+\underbrace{\langle n^{(0)}|\hat{V}|n^{(0)}\rangle}_{\displaystyle E_{n}^{(1)}}\;, (54)

so the PMS condition, \erefPMScondition, applied to the k=1k=1 case minimizes Hn(0)\langle H\rangle_{n}^{(0)} using |n(0)|n^{(0)}\rangle as the trial function. Now, consider the expectation value of H^\hat{H} for the state |n0+|n(1)|n^{0}\rangle+|n^{(1)}\rangle :

Hn(1)(n(0)|+n(1)|)(H^0+V^)(|n0+|n(1))(n(0)|+n(1)|)(|n0+|n(1)).\langle H\rangle_{n}^{(1)}\;\equiv\;\dfrac{\big{(}\langle n^{(0)}|+\langle n^{(1)}|\big{)}\big{(}\hat{H}_{0}+\hat{V}\big{)}\big{(}|n^{0}\rangle+|n^{(1)}\rangle\big{)}}{\big{(}\langle n^{(0)}|+\langle n^{(1)}|\big{)}\big{(}|n^{0}\rangle+|n^{(1)}\rangle\big{)}}\;. (55)

Minimizing Hn(1)\langle H\rangle_{n}^{(1)} by varying |n0+|n(1)|n^{0}\rangle+|n^{(1)}\rangle should improve the approximations for the n=0n=0 (ground state, even parity) and the n=1n=1 (1st excited state, odd parity) cases without ever going below the exact values.

The numerator and denominator of \erefH1def are

(n(0)|+n(1)|)(H^0+V^)(|n0+|n(1))\displaystyle\big{(}\langle n^{(0)}|+\langle n^{(1)}|\big{)}\big{(}\hat{H}_{0}+\hat{V}\big{)}\big{(}|n^{0}\rangle+|n^{(1)}\rangle\big{)} (56)
=\displaystyle= n(0)|H^0|n(0)En(0)+n(0)|V^|n(0)En(1)+n(0)|H^0|n(1)+n(1)|H^0|n(0)0\displaystyle\underbrace{\langle n^{(0)}|\hat{H}_{0}|n^{(0)}\rangle}_{\displaystyle E_{n}^{(0)}}+\underbrace{\langle n^{(0)}|\hat{V}|n^{(0)}\rangle}_{\displaystyle E_{n}^{(1)}}+\underbrace{\langle n^{(0)}|\hat{H}_{0}|n^{(1)}\rangle+\langle n^{(1)}|\hat{H}_{0}|n^{(0)}\rangle}_{\displaystyle 0} (59)
+n(0)|V^|n(1)+n(1)|V^|n(0)2En(2)\displaystyle+\underbrace{\langle n^{(0)}|\hat{V}|n^{(1)}\rangle+\langle n^{(1)}|\hat{V}|n^{(0)}\rangle}_{\displaystyle 2E_{n}^{(2)}}
+n(1)|H^0|n(1)En(2)+En(0)n(1)|n(1)+n(1)|V^|n(1)En(3)+En(1)n(1)|n(1)\displaystyle+\underbrace{\langle n^{(1)}|\hat{H}_{0}|n^{(1)}\rangle}_{\displaystyle-E_{n}^{(2)}+E_{n}^{(0)}\langle n^{(1)}|n^{(1)}\rangle}+\underbrace{\langle n^{(1)}|\hat{V}|n^{(1)}\rangle}_{\displaystyle E_{n}^{(3)}+E_{n}^{(1)}\langle n^{(1)}|n^{(1)}\rangle}
=\displaystyle= (En(0)+En(1))(1+n(1)|n(1))+En(2)+En(3),\displaystyle\big{(}E_{n}^{(0)}+E_{n}^{(1)}\big{)}\big{(}1+\langle n^{(1)}|n^{(1)}\rangle\big{)}+E_{n}^{(2)}+E_{n}^{(3)}\;,\vphantom{\bigg{|}} (60)
(n(0)|+n(1)|)(|n0+|n(1))\displaystyle\big{(}\langle n^{(0)}|+\langle n^{(1)}|\big{)}\big{(}|n^{0}\rangle+|n^{(1)}\rangle\big{)} (61)
=\displaystyle= n(0)|n(0)1+n(0)|n(1)+n(1)|n(0)0+n(1)|n(1)\displaystyle\underbrace{\langle n^{(0)}|n^{(0)}\rangle}_{\displaystyle 1}+\underbrace{\langle n^{(0)}|n^{(1)}\rangle+\langle n^{(1)}|n^{(0)}\rangle}_{\displaystyle 0}+\langle n^{(1)}|n^{(1)}\rangle\vphantom{\bigg{|}} (62)
=\displaystyle= 1+n(1)|n(1).\displaystyle 1+\langle n^{(1)}|n^{(1)}\rangle\;.\vphantom{\bigg{|}} (63)

Therefore,

Hn(1)=En(0)+En(1)+En(2)+En(3)1+n(1)|n(1).\langle H\rangle_{n}^{(1)}\;=\;E_{n}^{(0)}+E_{n}^{(1)}+\dfrac{E_{n}^{(2)}+E_{n}^{(3)}}{1+\langle n^{(1)}|n^{(1)}\rangle}\;. (64)

We see that Hn(1)\langle H\rangle_{n}^{(1)} can be considered the 3rd-order perturbative energy j=03En(j)\sum_{j=0}^{3}E_{n}^{(j)} corrected by a class of higher order terms which have been resummed into the factor (1+n(1)|n(1))1(1+\langle n^{(1)}|n^{(1)}\rangle)^{-1}. This is similar in spirit to Renormalization Group resummation, or the Brodsky-Lepage-Mackenzie method used in pQCD.[23] The correction renders Hn(1)\langle H\rangle_{n}^{(1)} positive definite, and avoids the problem j=03En(j)\sum_{j=0}^{3}E_{n}^{(j)} has of becoming negative around the right local minimum for n2n\geq 2.

Refer to caption

Figure 6: Stationary points of Hn(0)=En(0)+En(1)\langle H\rangle_{n}^{(0)}=E_{n}^{(0)}+E_{n}^{(1)} (squares) and Hn(1)\langle H\rangle_{n}^{(1)} (circles) for n=0n=0 through n=5n=5. The graphs shown are those for Hn(0)\langle H\rangle_{n}^{(0)} (dot-dashed), Hn(1)\langle H\rangle_{n}^{(1)} (dashed), and j=03En(j)\sum_{j=0}^{3}E_{n}^{(j)} (dotted). Solid horizontal lines indicate the exact values. The stationary points of Hn(0)\langle H\rangle_{n}^{(0)} are the same as the k=1k=1 PMS points in \frefPMSfig. The right local minimum of j=03En(j)\sum_{j=0}^{3}E_{n}^{(j)} has been lifted above the exact values for n=0n=0 and 11, and from the negative into the positive for n2n\geq 2.

To calculate Hn(1)\langle H\rangle_{n}^{(1)} we need, in addition to \erefHSterms,

n(1)|n(1)\displaystyle\langle n^{(1)}|n^{(1)}\rangle (65)
=\displaystyle= (n+1)(n+2)4(2n+3)2(Z(1X)42n+38)2+(n+1)(n+2)(n+3)(n+4)212(2n+5)2\displaystyle\dfrac{(n+1)(n+2)}{4(2n+3)^{2}}\bigg{(}\dfrac{Z(1-X)}{4}-\dfrac{2n+3}{8}\bigg{)}^{2}+\dfrac{(n+1)(n+2)(n+3)(n+4)}{2^{12}(2n+5)^{2}}\vphantom{\Bigg{|}} (67)
+n(n1)4(2n1)2(Z(1X)42n18)2+n(n1)(n2)(n3)212(2n3)2.\displaystyle+\dfrac{n(n-1)}{4(2n-1)^{2}}\bigg{(}\dfrac{Z(1-X)}{4}-\dfrac{2n-1}{8}\bigg{)}^{2}+\dfrac{n(n-1)(n-2)(n-3)}{2^{12}(2n-3)^{2}}\vphantom{\Bigg{|}}\;.

The graphs of Hn(0)\langle H\rangle_{n}^{(0)} and Hn(1)\langle H\rangle_{n}^{(1)} as well as their stationary points are shown for the X=0X=0 case in \frefVARfig for n=0n=0 through n=5n=5. Comparing the ZZ-dependence of Hn(1)\langle H\rangle_{n}^{(1)} (dashed line) and j=03En(j)\sum_{j=0}^{3}E_{n}^{(j)} (dotted line), we can see that they both have three stationary points: two local minima and one local maximum.

For the n=0n=0 (ground state, even parity) and n=1n=1 (1st exited state, odd parity) cases, the global minimum of Hn(1)\langle H\rangle_{n}^{(1)} will provide the best approximation without undershooting the exact values. Indeed, comparing the graphs of Hn(1)\langle H\rangle_{n}^{(1)} (dashed line) and j=03En(j)\sum_{j=0}^{3}E_{n}^{(j)} (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 H0(1)\langle H\rangle_{0}^{(1)} and H1(1)\langle H\rangle_{1}^{(1)} compared to the exact values are

H0,min(1)E0,exact= 1.00076,H1,min(1)E1,exact= 1.00066,\displaystyle\dfrac{\langle H\rangle_{0,\text{min}}^{(1)}}{E_{0,\text{exact}}}\,=\,1.00076\;,\qquad\dfrac{\langle H\rangle_{1,\text{min}}^{(1)}}{E_{1,\text{exact}}}\,=\,1.00066\;,\vphantom{\Bigg{|}} (68)

which are amazingly accurate (better than 0.1%) for a 3rd order perturbative calculation without any small expansion parameter.

Refer to caption

Figure 7: The spread of Hn(1)\langle H\rangle_{n}^{(1)} (circles, dashed) and j=03En(j)\sum_{j=0}^{3}E_{n}^{(j)} (squares, dotted) between their respective local minima.

For the n2n\geq 2 cases, the global minimum of Hn(1)\langle H\rangle_{n}^{(1)} does not have any special meaning. Indeed, for the n=2n=2 case we can see from \frefVARfig that the global minimum of H2(1)\langle H\rangle_{2}^{(1)} is a poor approximation. Nevertheless, for all n2n\geq 2 cases the right local minimum is now positive, and the spread of Hn(1)\langle H\rangle_{n}^{(1)} in the range between the two local minima are greatly reduced compared to that of j=03En(j)\sum_{j=0}^{3}E_{n}^{(j)}. This is shown in \frefEHspread. For n3n\geq 3, the function Hn(1)\langle H\rangle_{n}^{(1)} is flat enough between the two local minima, so it does not matter what value of ZZ is chosen in that range.

As we continue this procedure to higher orders, we conjecture that Hn(k)\langle H\rangle_{n}^{(k)} will become flatter for a wider range of ZZ with increasing kk. For instance, the next function to consider in the sequence is

Hn(2)\displaystyle\langle H\rangle_{n}^{(2)} \displaystyle\equiv (n(0)|+n(1)|+n(2)|)(H^0+V^)(|n0+|n(1)+|n(2))(n(0)|+n(1)|+n(2)|)(|n0+|n(1)+|n(2))\displaystyle\dfrac{\big{(}\langle n^{(0)}|+\langle n^{(1)}|+\langle n^{(2)}|\big{)}\big{(}\hat{H}_{0}+\hat{V}\big{)}\big{(}|n^{0}\rangle+|n^{(1)}\rangle+|n^{(2)}\rangle\big{)}}{\big{(}\langle n^{(0)}|+\langle n^{(1)}|+\langle n^{(2)}|\big{)}\big{(}|n^{0}\rangle+|n^{(1)}\rangle+|n^{(2)}\rangle\big{)}}\vphantom{\Bigg{|}} (69)
=\displaystyle= En(0)+En(1)+En(2)1+n(1)|n(2)+n(2)|n(1))1+n(1)|n(2)+n(2)|n(1)+n(2)|n(2)\displaystyle E_{n}^{(0)}+E_{n}^{(1)}+E_{n}^{(2)}\dfrac{1+\langle n^{(1)}|n^{(2)}\rangle+\langle n^{(2)}|n^{(1)}\rangle)}{1+\langle n^{(1)}|n^{(2)}\rangle+\langle n^{(2)}|n^{(1)}\rangle+\langle n^{(2)}|n^{(2)}\rangle}\vphantom{\Bigg{|}} (71)
+En(3)+En(4)+En(5)1+n(1)|n(2)+n(2)|n(1)+n(2)|n(2),\displaystyle+\;\dfrac{E_{n}^{(3)}+E_{n}^{(4)}+E_{n}^{(5)}}{1+\langle n^{(1)}|n^{(2)}\rangle+\langle n^{(2)}|n^{(1)}\rangle+\langle n^{(2)}|n^{(2)}\rangle}\;,\vphantom{\Bigg{|}}

which we expect to have three local minima and two local maxima. The “wiggles” in Hn(2)\langle H\rangle_{n}^{(2)} between these extrema should be smaller than those of Hn(1)\langle H\rangle_{n}^{(1)}.

4 Discussion

We have studied the ZZ-value selection problem in the Halliday-Suranyi approach to the quartic anharmonic oscillator.[21, 22] We have analyzed the pure quartic potential case (m=0m=0) and found that the FAC and PMS methods lead to fractional errors that decrease monotonically with increasing nn. 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 (2k+1)(2k+1)st order energy j=02k+1En(j)\sum_{j=0}^{2k+1}E_{n}^{(j)} with the expectation value of H^=H^0+V^\hat{H}=\hat{H}_{0}+\hat{V} for the kkth order state j=0k|n(j)\sum_{j=0}^{k}|n^{(j)}\rangle. This expectation value is positive definite, and for the n=0n=0 (ground state) and n=1n=1 (1st excited state) cases bounded from below by the exact energies. At k=1k=1 the resulting approximations for the n=0n=0 and n=1n=1 energies are better than 0.1%. The dependence on the value of ZZ is also greatly reduced compared to j=02k+1En(j)\sum_{j=0}^{2k+1}E_{n}^{(j)}, facilitating the choice of ZZ.

While this result is quite interesting in itself, the more important question is whether analogous techniques can be applied to d+1d+1 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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