The high-n form of the radiation-damped S-matrix
نویسنده
چکیده
There now exist two different formalisms for the high-n form of the radiationdamped S-matrix. These two formalisms give nearly identical results for all physical systems and either may be used in calculations. However, there is some uncertainty as to which is the more exact form. It is shown that Bell and Seaton made four approximations that prevented them from deriving the correct form due to Hickman. A corrected derivation is given in this letter. It is shown that the poles of a two-channel S-matrix have an unphysical high-n form when using the formalism of Bell and Seaton, but behave nicely using the formalism of Hickman. Also, two statements about Robicheaux et al (1995) in a recent paper by Pradhan and Zhang are corrected. For over a decade, there have been questions raised about the correct form for the closecoupling equations when one electron is in a Rydberg state outside of a core that can decay radiatively. The first formalism was introduced by Hickman (1984) using very plausible heuristic arguments; this formalism consists of replacing the real core energy, Ec, in the close-coupling equations with a complex energy, Ec− iR/2, where R is the radiative decay rate of the core. The second formalism was introduced by Bell and Seaton (1985) based on the general radiation damping formalism of Davies and Seaton (1969); this formalism consists of replacing the real principal quantum number, ν, in the multichannel quantum defect theory (MQDT) with a complex principal quantum number, ν + iRν3/2z2, where z is the residual charge of the ion. Seaton (1984) gave an intuitive derivation of the Bell and Seaton result because in Bell and Seaton this simple result was obtained after a tour de force derivation involving ∼ 200 equations. Although Hickman’s formalism was much more physically plausible, the Bell and Seaton formalism was preferred in calculations because it had been derived from first principles (only LaGattuta and Hahn (1985) attempted model calculations using Hickman’s formalism); it appeared that Hickman’s formalism was a good approximation of that by Bell and Seaton. A recent paper by Pradhan and Zhang (1997) is an example illustrating the controversy in that the work of Hickman is not even mentioned. This issue was reopened by Robicheaux et al (1995). Using a very powerful and flexible formalism for describing general radiation damping, we were able to derive the form for the close-coupling equations using five equations (section VIB). Strikingly, the final form consisted of replacing the real core energy, Ec, in the close-coupling equations with a complex energy Ec − iR/2 (i.e. identical to the formalism of Hickman). As both formalisms have now been derived from first principles, a natural question is which is the more exact formalism and which is the approximation? Is Bell and Seaton’s formalism a good approximation to Hickman’s more exact formalism (or vice versa)? 0953-4075/98/040109+07$19.50 c © 1998 IOP Publishing Ltd L109 L110 Letter to the Editor There are four arguments for supposing that Hickman’s formalism is more exact and that Bell and Seaton’s formalism is approximate: (i) Hickman’s formalism is more physically appealing and can be trivially generalized to cases where the asymptotic potential is not 1/r; (ii) the derivation of Hickman’s formalism is much simpler and therefore there is less opportunity for inadvertent approximations; (iii) the poles of the S-matrix have a more intuitively correct form using Hickman’s formalism. (Arguments (i) and (iii) depend on personal taste and argument, (ii) rests on the assumption that Robicheaux et al are less likely to make mistakes than Bell and Seaton; thus these arguments are not very compelling by themselves.) (iv) It is possible to identify four approximations in Bell and Seaton’s derivation; removing these four approximations, but otherwise following Bell and Seaton’s derivation, results in a final formula that is identical to that of Hickman. Together, these four arguments make it overwhelmingly likely that Bell and Seaton’s formalism is a good approximation of Hickman’s more exact formalism. In the derivation that follows, I will use the notation of Bell and Seaton unless stated otherwise. Equations taken from this paper will be denoted with a BS. Bell and Seaton used the general radiation damping formalism of Davies and Seaton which was shown to be formally equivalent to that used by Robicheaux et al (see section VC). Thus the differences between Hickman and Bell and Seaton must arise in an approximate implementation. The final form of Bell and Seaton rests on a derivation given in their section 6 for a two-channel case; this derivation will be examined in detail. Assume that channel α is open and channel γ is closed and that the core state for channel γ decays to that for channel α with a rate R. Let χ = ( χαα χαγ χγα χγγ ) (6.5 BS) be the unphysical S-matrix obtained by allowing both channels to be open. The complex quantum defect is defined in equation (6.12 BS) to be χγγ = exp[2π iμγ ]; μγ has real and imaginary parts μγ = p + iq (equation (6.13 BS)) where p and q are real and q > 0. Without radiation damping, the physical S-matrix has poles at νn = n−μγ (equation (6.14 BS)) or energies En = −z2/2ν2 n (equation (6.15 BS)) relative to the γ threshold. The important parameter for describing radiation damping in this two-channel case is T = ∑ n (Pγ (ν)|Pγ (νn)) ( E − En + 2 iR )−1 t (νn)/t (ν) (6.50 BS) where Pγ (ν) is the radial wavefunction in channel γ (equation (A.2.3 BS)), (Pγ (ν)|Pγ (νn) is a radial overlap integral (equation (A.2.1 BS)) and t (ν) is a complex normalization factor (equation (6.9 BS)). There are no approximations in these equations. Bell and Seaton use four approximations to evaluate the expression for T . These approximations are not necessary for obtaining a final result. Approximation (i). Bell and Seaton use an approximate expression for the radial overlap: (Pγ (ν)|Pγ (νn)) ' sinπ(ν − νn) ν − νn (A.2.12 BS) instead of the exact expression (Pγ (ν)|Pγ (νn)) = z 2 Eν − En (ννn) −3/2 sinπ(ν − νn) π (1) obtained from equations (A.2.8 BS)–(A.2.11 BS) and where Eν = −z2/2ν2 (equation (A.2.5 BS)). (Pγ (ν) is replaced by its complex conjugate if ν is complex (equation (A.2.12 Letter to the Editor L111 BS)).) The approximate expression (A.2.12 BS) arises by using the large-n approximation Eν − Eν ′ ' −z2(ν ′ − ν)/ν3. Approximation (ii). Bell and Seaton use the approximation for the ratio of t’s: t (νn)/t (ν) ' exp[iπ(ν − νn)] (6.53 BS) instead of the exact expression t (νn)/t (ν) = (ν/νn) exp[iπ(ν − νn)]. (6.51 BS) The approximate expression (6.53 BS) arises by using the large-n approximation ν/νn ' 1. Approximation (iii). Bell and Seaton use an approximate expression for energy differences for real ν: Eν − En ' (z/ν)(ν − νn) (6.54 BS) instead of the exact expression Eν − En = z/2ν n − z/2ν. (2) The approximate expression (6.54 BS) arises from the large-n approximation δE/δν ' z2/ν3. Approximation (iv). Bell and Seaton use an approximate expression for complex energy differences: Eν − En + 2 iR ' (z/ν)[ν − νn + i1(ν)] (6.55 BS) instead of the exact expression Eν − En + 2 iR = z/2ν n − z/2(ν + i1). (3) The approximate expression (6.55 BS) again arises from the large-n approximation δE/δν ' z2/ν3. In what follows, I will use a parameter not defined by Bell and Seaton: ν̄ = ν + i1 (4) or equivalently Eν − En + 2 iR = z/2ν n − z/2ν̄ ≡ Eν̄ − En. (5) Exact derivation. The derivation of Bell and Seaton section 6.5.2 (evaluation of T ) can proceed but now using the exact expressions. First substitute in equation (6.50 BS) for the ratio of the t’s using the exact expression (6.51 BS), T = ∑ n (Pγ (ν)|Pγ (νn))(Eν̄ − En)−1(ν/νn)3/2 exp[iπ(ν − νn)] (6) where Eν̄ = Eν + iR/2 has been used. Use the exact overlap expression (1) to eliminate (Eν̄ − En)−1: T = −π ∑ n (Pγ (ν)|Pγ (νn))(P ∗ γ (νn)|Pγ (ν̄)) √ ν̄3ν3/z4 exp[iπ(ν − νn)] sinπ(νn − ν̄) . (7) Because the ratio exp[iπ(ν − νn)] sinπ(νn − ν̄) = − exp[iπ(ν + μγ )] sinπ(ν̄ + μγ ) (8) L112 Letter to the Editor is independent of n, the only terms that depend on n are in the overlaps. Using closure gives T = π(Pγ (ν)|Pγ (ν̄)) √ ν̄3ν3/z4 exp[iπ(ν + μγ )] sinπ(ν̄ + μγ ) . (9) (Note that closure is not exact because only the bound states are summed over but the continuum is not integrated over; the error is of the same size as in the Bell and Seaton closure derivation. The size of this error is roughly δμ2/n, where δμ is the difference between the quantum defect of the autoionizing state and the final state; δμ will typically be much less than 0.01 for ions thus making this a very good approximation.) Now again use the exact expression for the overlap, equation (1), to obtain T = (Eν − Eν̄)−1 sinπ(ν − ν̄) sinπ(ν̄ + μγ ) exp[iπ(ν + μγ )]. (10) Using Eν−Eν̄ = −iR/2 and multiplying the numerator and denominator by exp[iπ(μγ−ν̄)] gives T = 2i R (e2iπ(ν−ν̄) − 1)eγ /(eγ − e−2iπν̄). (11) Now use the definition of χγγ = exp[2π iμγ ], equation (6.12 BS), and define the parameter g(ν) = exp[2iπ(ν − ν̄)] (12) to obtain T = 2i R [g(ν)− 1]χγγ /[χγγ − g(ν) e−2iπν]. (6.65 BS) This expression for T is the same as in Bell and Seaton except they used the approximate expression g(ν) ' exp(πνR/z). (6.66 BS) This approximate form for g is obtained from the exact expression, equation (12), by expanding ν− ν̄ to lowest order in R. Equations (6.67)–(6.71) of Bell and Seaton are exact as long as the exact value of g(ν) is used instead of the approximate expression (6.66 BS). In particular, the physical S-matrix is given by Sαα = χαα − χαγ [χγγ − g(ν) e−2iπν]−1χγα (6.71 BS) which is equivalent to Sαα = χαα − χαγ [χγγ − e−2iπν̄]−1χγα (13) when using the exact form for g(ν), equation (12). This is equivalent to substituting Ec−iR/2 for the core energy in the close-coupling expansion. (Note that this form of the Smatrix does give an unphysical discontinuity at threshold proportional to exp(−πZ√2/R); for the example below the size of the discontinuity is e−7025 ∼ 10−3051 which is negligibly small for most applications.) This derivation shows that if the four high-n approximations are eliminated from the derivation in Bell and Seaton, then the formalism of Davies and Seaton is equivalent to that of Hickman for a Rydberg electron attached to a radiating core. The main reason Bell and Seaton’s original derivation did not reproduce Hickman’s formalism is that at high n the spacing of successive resonances becomes much smaller than the radiative decay rate of the core, R. Thus the small change in energy Eν → Eν+ iR/2 becomes a substantial change in principal quantum number ν → ν̄. Removing approximation (iv) is the key to showing that Letter to the Editor L113 the formalism of Davies and Seaton is equivalent to that of Hickman. The reason for the difference also shows why the two formalisms give nearly identical results for all physical systems. Most autoionizing resonances have widths much smaller than the Rydberg spacing z2/ν3. As n increases Bell and Seaton’s formalism differs increasingly from Hickman’s. But before this approximation breaks down, the radiative rate becomes much larger than the autoionization rate; for this case, the branching ratio for autoionization is very small so order of magnitude errors are irrelevant in practice (for example, the difference between branching ratios of 10−3 and 10−5 is physically irrelevant). Recently, Pradhan and Zhang (1997) made several comments regarding the accuracy of Bell and Seaton’s results and several purported assertions in Robicheaux et al (1995). Pradhan and Zhang assert that we stated reservations about the precision and utility of Bell and Seaton’s formalism. This is incorrect. There are no statements in Robicheaux et al that are in any way related to judgements about the utility of Bell and Seaton’s formalism. Bell and Seaton’s formalism is a very good approximation to the more exact formalism by Hickman (in all known cases); however, because it is such a good approximation, agreement with experiment does not indicate that the formalism is exact because no experiments to date can distinguish between Bell and Seaton’s approximate formalism and Hickman’s more exact treatment. Pradhan and Zhang also state ‘This contradicts the assertions of Robicheaux et al (1995), made without reporting any calculations, that the BS theory leads to ‘strange poles in the S-matrix’.’ This is also incorrect. The direct quote ‘strange poles in the S-matrix’ which they attribute to Robicheaux et al is not in this paper; in fact, the issue of poles in the S-matrix is not addressed at all. Therefore, it is not surprising that we have not reported any calculations supporting these non-existent assertions. While Robicheaux et al did not make this assertion, it is nevertheless true that the approximate form of the S-matrix due to Bell and Seaton has a strange sequence of poles when ν3R/z2 1. The more exact form by Hickman has a physically reasonable sequence of poles. Figure 1. The poles of the S-matrix using the exact form due to Hickman (squares) and the approximate form due to Bell and Seaton (pluses). The energy where the Rydberg spacing equals R/2 is marked with a vertical line. The boxed region is expanded in figure 2. L114 Letter to the Editor To demonstrate this, examine the position of the poles for the two-channel case above. Using Hickman’s formalism, the poles are at ν̄ = n−μγ = n− p− iq; this gives poles at E n = − z2 2(n− p − iq)2 − iR 2 ' − z 2 2(n− p)2 − iz2q (n− p)3 − iR 2 . (14) This equation makes physical sense since the imaginary part is simply minus the sum of the autoionization and radiative decay rates; these different decay paths are distinguishable. In contrast, using Bell and Seaton’s formalism, the poles are at exp(−2iπν + πνR/z) = exp(2iπμγ ) (15) where ν = z/√−2EBS n . This transcendental equation has no simple solution except for ν3R/z2 1, where the EBS n ' EH n . Figure 2. Same as figure 1. The boxed region is expanded in figure 3. Note the change in scale for the real part of the energy. Figure 3. Same as figure 1. Note that the decay rates of the very high-n states using Bell and Seaton’s formalism are less than the radiative decay rate of the core. Only a fraction of the states has been plotted for clarity. Note the change in scale for the real part of the energy. Letter to the Editor L115 The results of a model calculation are plotted in figures 1–3 for p = 0.03, q = 0.01, R = 10−5 au and z = 5. The poles of the S-matrix are plotted in the complex energy plane with squares for the poles from the more exact equation (14) and with pluses using the approximate form from equation (15). The vertical line marks the energy where the Rydberg spacing equals R/2. It is clear that over a huge range of n, the results are nearly identical. Note that the branching ratio for autoionization has dropped to ∼10−3 before the two results begin to disagree. But clearly the poles of the S-matrix using Bell and Seaton’s approximate form have a strange behaviour at high n. The widths of the resonances are going to 0 and therefore becoming smaller than the radiative decay rate of the core state. This is certainly unphysical behaviour. In conclusion, we have shown that a more accurate derivation using Davies and Seaton’s formalism corrects the final result of Bell and Seaton so that it agrees exactly with Hickman’s formalism for a Rydberg electron outside of a core that can decay radiatively. The original derivation of Bell and Seaton must be considered an approximation to the more exact formalism by Hickman. However, it must be stressed that Bell and Seaton’s formalism accurately reproduces Hickman’s formalism until the Rydberg spacing becomes much smaller than the radiative decay rate of the core. Thus, the approximate results of Bell and Seaton will probably be accurate enough for all practical calculations because the physically important range for dielectronic recombination is when the Rydberg spacing is larger than the radiative decay rate of the core. I thank Drs Badnell, Gorczyca, Pindzola, Pradhan and Seaton for reading an early version of this manuscript. Also, I am grateful to Dr Seaton for pointing out weak steps in the original derivation. This work was supported by the US Department of Energy under grant number DE-FC02-91ER75678.
منابع مشابه
Hydrodynamic damped pitch motion of tension leg platforms
Because of fluctuation in leg tension, pitch motion is very effective fatigue and life safety of leg elements in tension leg structures (TLSs). In this paper an exact solution for pitch vibration of a TLS interacting with ocean wave is presented. The legs of TLP are considered as elastic springs. The flow is assumed to be irrotational and single-valued velocity potentials are defined. The effec...
متن کاملDamped DQE Model Updating of a Three-Story Frame Using Experimental Data
In this paper, following a two-stage methodology, the differential quadrature element (DQE) model of a three-story frame structure is updated for the vibration analysis. In the first stage, the mass and stiffness matrices are updated using the experimental natural frequencies. Then, having the updated mass and stiffness matrices, the structural damping matrix is updated to minimize the error be...
متن کاملA matrix LSQR algorithm for solving constrained linear operator equations
In this work, an iterative method based on a matrix form of LSQR algorithm is constructed for solving the linear operator equation $mathcal{A}(X)=B$ and the minimum Frobenius norm residual problem $||mathcal{A}(X)-B||_F$ where $Xin mathcal{S}:={Xin textsf{R}^{ntimes n}~|~X=mathcal{G}(X)}$, $mathcal{F}$ is the linear operator from $textsf{R}^{ntimes n}$ onto $textsf{R}^{rtimes s}$, $ma...
متن کاملOn study of X-ray absorption and properties of dispersion of W, MoS2 and B4C particles in high density polyethylene
Shielding radiation from both x-rays and gamma-rays is important for personnel in medical fields e.g. interventional radiology, nuclear power stations, and other inspection facilities where radiation is involved. Lead is known for its effective shielding property against these high energy radiations, however heaviness and toxicity are its main drawback. In this study effectiveness of non-lead p...
متن کاملOn the solving matrix equations by using the spectral representation
The purpose of this paper is to solve two types of Lyapunov equations and quadratic matrix equations by using the spectral representation. We focus on solving Lyapunov equations $AX+XA^*=C$ and $AX+XA^{T}=-bb^{T}$ for $A, X in mathbb{C}^{n times n}$ and $b in mathbb{C} ^{n times s}$ with $s < n$, which $X$ is unknown matrix. Also, we suggest the new method for solving quadratic matri...
متن کاملThe (R,S)-symmetric and (R,S)-skew symmetric solutions of the pair of matrix equations A1XB1 = C1 and A2XB2 = C2
Let $Rin textbf{C}^{mtimes m}$ and $Sin textbf{C}^{ntimes n}$ be nontrivial involution matrices; i.e., $R=R^{-1}neq pm~I$ and $S=S^{-1}neq pm~I$. An $mtimes n$ complex matrix $A$ is said to be an $(R, S)$-symmetric ($(R, S)$-skew symmetric) matrix if $RAS =A$ ($ RAS =-A$). The $(R, S)$-symmetric and $(R, S)$-skew symmetric matrices have a number of special properties and widely used in eng...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
عنوان ژورنال:
دوره شماره
صفحات -
تاریخ انتشار 1998