Scholarly article on topic 'X-ray measurements in helium-like atoms increased discrepancy between experiment and theoretical QED'

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Academic research paper on topic "X-ray measurements in helium-like atoms increased discrepancy between experiment and theoretical QED"

New Journal of Physics

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Deutsche PhysikalischeGeseUschaft DPG IOP Institute Of PhySjCS

X-ray measurements in helium-like atoms increased discrepancy between experiment and theoretical QED

C T Chantler1, A T Payne1, J D Gillaspy2, L T Hudson2, L F Smale1, A Henins2, J A Kimpton3 and E Takacs4,5

1 School of Physics, The University of Melbourne, Australia

2 National Institute of Standards and Technology, 100 Bureau Drive, Gaithersburg, MD 20899, USA

3 Australian Synchrotron, Melbourne, Victoria 3000, Australia

4 Department of Physics and Astronomy, Clemson University, Clemson, SC 29634, USA

5 Experimental Physics Department, University of Debrecen, Bem ter 18/a, Debrecen, H-4026 Hungary

E-mail: chantler@unimelb.edu.au

Received 10 July 2014, revised 9 October 2014 Accepted for publication 28 October 2014 Published 15 December 2014 New Journal of Physics 16 (2014) 123037 doi:10.1088/1367-2630/16/12/123037

Abstract

A recent 15 parts per million (ppm) experiment on muonic hydrogen (p+w-) found a major discrepancy with quantum electrodynamics (QED) and independent nuclear size determinations. Here we find a significant discrepancy in a different type of exotic atom: a medium-Z nucleus with two electrons. Investigation of the data collected is able to discriminate between available QED formulations and reveals a pattern of discrepancy of almost six standard errors of experimental results from the most recent theoretical predictions, with a functional dependence proportional to Zn where n ^ 4. In both the muonic and highly charged systems, the sign of the discrepancy is the same, with the measured transition energy higher than predicted. Some consequences are possible or probable, and some are more speculative. This may give insight into effective nuclear radii, the Rydberg, the fine-structure constant, or unexpectedly large QED terms.

Keywords: helium-like quantum systems, relativistic atomic physics, x-ray spectroscopy, QED

Content from this work may be used under the terms of the Creative Commons Attribution 3.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.

New Journal of Physics 16 (2014) 123037

1367-2630/14/123037+15$33.00 © 2014 IOP Publishing Ltd and Deutsche Physikalische Gesellschaft

1. Introduction

In this article, we study the pattern of discrepancy between two-electron experiment and theory for x-ray transitions to core holes. Recent work has raised this area as one of the current anomalies in quantum electrodynamics (QED) computation. QED is one of the most important foundations of modern physics. The five-standard-deviation inconsistency between a 15 parts per million (ppm) measurement of a muonic hydrogen transition and theory [1] has led to four years of intensive research by many groups around the world. Leading theorists consider the discrepancy of 0.42 meV to be well outside possible causes within the Standard Model, claimed to have an uncertainty of no more than ±0.01 meV [2].

This puzzling situation has stimulated much theoretical activity, and it highlights the current difficulty in low-Z atomic spectroscopy that results from complexities of the nucleus. In precision measurements with atomic hydrogen [3], progress is stalled by uncertainties in nuclear form factors and nuclear polarization, both of which render the last few digits of available experimental accuracy underutilized. At high-Z, the strong enhancement of nuclear interactions also limits the degree to which available experimental measurements can be used to test QED [4]. For medium-Z, nuclear uncertainties do not limit the interpretation of atomic spectroscopy. The overall magnitude of the contribution from nuclear size and shape is small, and the uncertainty on the magnitude is smaller still; for the case of titanium, the uncertainty in the nuclear radius, even in early atomic structure calculations, is 0.012 fm [5], which is less than half that of the proton [5] and much less than the 0.42 fm discrepancy from the muonic hydrogen experiment.

Spectroscopy of highly charged ions and muonic atoms probes a relatively unexplored regime of physics, in which the peak of the radial wavefunction of the lepton is reduced by more than an order of magnitude. Effects associated with QED and the nucleus are greatly enhanced, due to the increased overlap of the nucleus with the wavefunction of the orbiting lepton. In the case of muonic hydrogen, the lepton orbital radius is reduced by the mass of the lepton, while in the case of highly charged ions, the lepton orbital radius is decreased by the increased nuclear charge. While hydrogenic (one electron) atomic systems are exotic and are critical challenges for theory and experiments, helium-like (He-like) atomic systems lie at one of the forefronts of QED research [6], because they display qualitatively new effects (including the 'two-electron Lamb shift') that are not present at any level in one-electron ions.

Crucial higher-order 1e-QED terms scale as a2(Za)6 and a (Za)7 for hydrogen, while similar 2e-QED terms scale as a2(Za)6 and a2(Za)7. Hence, an increase in Z results in a dramatic increase in the magnitude of higher-order contributions [7]. If the Z-expansions used for hydrogen remained valid, then a 1 ppm measurement in the middle of the periodic table would be equivalent to testing some higher-order terms in hydrogen to a few parts in 1015 [4]. Moreover, in the mid-Z range, some of the perturbative expansions fail, so nonperturbative methods are required. The mid-Z crossover range between neutral atoms and very high-Z, few-electron ions is the focus of this paper. Tests with atoms and muonic hydrogen have focused on the proton radius, while the real cause may lie elsewhere.

Precision measurements of x-ray energies require high resolution and must be undertaken using wavelength dispersive spectroscopy employing Bragg diffraction. Tests of QED in He-like systems often observe the diffraction profile of w(1s2(1S0) — 1s2p(1P1)), and less frequently the x(1s2(1S0) - 1s2p(3P2)), y(1s2(%) - 1s2p(3P1)) and z(1s2(%) - 1s2s(3S1)) transitions.

2. Inconsistency with the null hypothesis

Taken individually, recently measured He-like transition energies of titanium demonstrate significant deviation from the most recent comprehensive ab initio theoretical QED formulation [6], with significances of 2.9 s.e. for the w-line [8], 1.4 s.e. for the z-line, and 1.3 s.e. and 0.3 s.e. for the y- and x-lines, respectively [9]. All lie higher than the predictions of theory. The weighted mean of these four deviations from theory (see table 2) is nonzero by 3.2 s.e.

When all the assessed literature claiming absolute measurements for the four lines is taken together and the weighted mean is calculated for each value of Z > 15, then compared to the predictions in [6], the xf is found to be 3.5 (for no fit parameters), corresponding to a

probability of less than P = 1.2 x 10-5 that the data are adequately described by the predictions. This presents a challenging puzzle, as the uncertainty of the predictions is reported to be much smaller than even the most precise experiments, and the results of four independent calculations [6, 10-12] by leading groups agree with each other to within a fraction of the observed deviation from the experiments. Some 18 measurements are added for the x, y, and z transitions, including our recent data. The possibility that the experiments suffer from a common systematic error seems unlikely, given that this set includes 63 results distributed over 28 different experiments from at least 12 different groups, conducted over more than four decades. In addition, the independent measurements at each value of Z are in good agreement with their weighted means.

There are other measurements in the literature at lower values of Z, which are not directly comparable to [6] because that work is only tabulated down to Z = 12 and becomes increasingly uncertain as Z is reduced. In fact, the difference in the calculated energy of the ground level with respect to a competing calculation crosses over and changes sign around Z = 15.

3. Pattern of discrepancy

Our earlier work analyzed the strongest of the four lines and included data from the literature up through the end of 2011, and suggested a systematic discrepancy from theory with a functional dependence proportional to Z3 [8]. A later investigation demonstrated that the consideration of non integer exponents led to a minimum at Z3 5 [13], as shown in the lower curve in figure 1.

Quadrupling the number of spectral peaks does much more than increase the statistical significance of the deviation. It rules out a range of systematics relating to satellites and line shifts from adjacent peak overlap, for example, which may be unrecognized. The consistent pattern of discrepancy that results when all four lines are included also suggests that the problem lies primarily in the calculation of the ground level (common to all four lines), or that the error in most of the upper levels is of the same magnitude for each value of Z. This makes sense, in that the QED corrections to the ionization energy (as opposed to the total energy) scale in proportion to 1/n3 are proportional to the electron density at the nucleus (i.e., the matrix element of the delta function (equation 2, [11])).

Deviations of the experiments from theory for all four lines are plotted as a function of Z (figures 2-5), and are statistically consistent with a single monomial, rising approximately as Z4. Theory predicts that the first-order QED corrections (vacuum polarization and self-energy) should scale as approximately Z4 as well. Specific Feynman diagrams involving virtual photons and electron correlation follow expansions of order Z4, Z6(1/Z), Z6(1/Z)2, and Z4(1/Z), for

Figure 1. A persistent discrepancy. Plot of x2 by monomial order for various data sets combining literature values with our experimental results. The dot-dash curve (magenta) includes only measurements of the w-line [13]. The red dotted line is Fit 'A', including all absolute w, x, y, and z transition measurements with claimed uncertainties above 10ppm. The solid blue line represents the x^ valley including [14]. The green dashed line includes both [14, 15].

Figure 2. Discrepancy of experimental data from the latest theory for two-electron systems. Difference of weighted mean results for w, x, y, and z transitions. The [red] dotted line is Fit 'A' (see text and table 2; Z4 dependence, x2 = 1-2). The [blue] solid line is Fit 'B' (including [14] and assuming Z dependence, with one s.e. shading -(68%) confidence interval around the fit to demonstrate consistency with the other fits within uncertainty, x2 = 1-3). The [green] dashed line is Fit 'C' including [14, 15], scaling as Z5. All are fitted across the range Z e [15, 92]. The error bar shown on each point is the s.e. Experimental results for the w, x, y, and z lines included in Fit 'A' are plotted as weighted means for each Z (table 1). Theoretical formulations presented, relative to Artemyev e? al [6] are Cheng [10], Drake [11], and Plante [12].

example. The current level of accuracy of the experiments does not warrant fitting a polynomial of more than one degree of freedom, so therefore we consider only the coefficient of a monomial of order n, where n is taken to be the constant value that minimizes the xr2 of the deviations of the weighted means at each value of Z from the theoretical predictions. The

Atomic Number, Z

Figure 3. Discrepancy of experimental data from the latest theory for two-electron systems for x (1s2p3P2 ^ 1s2 So), plotted across mid-Z (Z e [15, 40]), from Artemyev et al [6]. Lines as per figure 2. Experimental results for the x lines included in Fit 'A' are plotted for each Z. The result of our recent work is plotted as a black circle. Theoretical formulations presented, relative to Artemyev et al [6] are Cheng [10], Drake [11], and Plante [12]. None of these different advanced computations are consistent with the experimental data. Although the result is dominated by the statistical uncertainty for this transition, there is very good agreement with the imputed discrepancy. Experimental results plotted are [9, 16-21].

§ 0.8

? 0.6 0)

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Q 15 20 25 30 35 40

Atomic Number, Z

Figure 4. Discrepancy of experimental data from the latest theory for two-electron systems for y (1s2p3P1 ^ 1s2lS0), as per figure 3. Lines as per figure 2. Experimental results plotted are [9, 16-26].

y-line

♦ Schleinkoferl 9S2 0 Cheng2000 ........ Fit A

■ Deslattes 1 984 □ Drake 1 988 - Fit B

• Chantler2000 V Plantel 994 ---Fit C

Y Chantler2009

MacLaren 1 992

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X Widmannl 995

M Widmannl 996

Briand1989

- Briand 1 990 • Payne201 4 ■ _ ^ .........

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consideration of a high-order polynomial is self-evidently consistent with Feynman diagram expectation values and correlation orders. The null hypothesis (i.e., a constant offset discrepancy from theory with a zero amplitude) has the same number of fitting coefficients and appears improbable, so we are comparing like with like in the statistical evaluation.

To check the possibility that one or more experimental approaches might have a recurring systematic error, we have performed a variety of robustness tests by systematically deleting all of the data from one or more types of experimental arrangements (those with the most data, with

z-line

1.0 0.8 0.6 0.4 0.2 0.0 -0.2 -0.4

Amaro201 2 4 ■ Chantler2000 MacLaren1992 Widmannl 995 4 T Widmannl 996 Payne201 4

Fit A Fit B Fit C

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Figure 5. Discrepancy of experimental data from the latest theory for two-electron systems for z (1s2s3Si ^ 1s2'So), as per figure 3. Lines as per figure 2. Experimental results plotted are [9, 14, 17, 19-21].

the smallest error bars, etc) and refit. The data set composed of our results and results prior to 2012 is robust against this test. We also grouped these data by subset of the photon source, and we found robust evidence for a strong Z-dependent deviation from theory. For example, looking at only electron beam ion trap (EBIT) data, since that subset is believed to suffer less from systematic corrections, we find a Z3 2 dependence of discrepancy, based on the w-line only, with a x? = 1-06. Inclusion of EBIT data from the literature on x, y, and z yields the same optimized

dependence of discrepancy (Z3 2) and a significance of 4.6 (i.e., a 4.6 standard error discrepancy from theory). Furthermore, the evidence suggests that the measurements in the literature up through 2011 reasonably accurately estimated their errors, and can be treated as statistically independent.

We now consider the effect of two recent measurements in argon [14, 15], which appear to fall into a different category from earlier data. These two measurements claim an uncertainty at the level of nearly one ppm, about an order of magnitude better than the best measurements performed at any other value of Z, and hence bring with them the possibility of significantly skewing the results of a global fit.

The primary conclusion of a Z-dependent discrepancy remains unchanged whether or not these two recent data points are included in the analysis. The statistical consistency of the global deviation fit, however, can be significantly affected. To investigate this, we present the results of three different fits to subsets of the data: Fit 'A', including [8, 9, 16-37], Fit 'B,' including [14], and Fit 'C,' including [14, 15].

We obtain a discrepancy given by Fit 'A,' AE = (2.8 X 10-7 ± 4.9 X 10-8)Z4 eV, X^ = 1.2. The uncertainty of the fit coefficient represents a 5.74 s.e. deviation from zero.

Such a discrepancy would occur in a normal distribution, with a probability of only 5 X 10-9 (5.74 s.e.). This fit represents some 61 spectral lines, and lies within one s.e. of the result based on the w-line only. This fit is presented in figures 2-5, presenting individual data points for the x, y, and z lines, respectively, indicating the common pattern with increasing atomic number. All data are plotted against the theoretical predictions of Artemyev et al [6], which has been the benchmark standard for He-like QED theory for a number of years. Three of the most highly

referenced theoretical predictions from 1988 [11], 1994 [12], 2000 [38], and the current standard of 2005 [6] are clustered together, indicating the advance and convergence of scholarship.

Amaro et al [14] do not report the w-transition because the state-population mechanisms of the ECRIS source (Electron Cyclotron Resonance Ion Source) rendered it relatively weak. Their reported z-transition is discrepant from theory, with the same sign as our results. Including [14] in the overall fit yields two results with the same goodness-of-fit: (1) AE = (4.2 X 10-8 ± 7.4 X 10-9)Z4 5 eV, x2 = 1.3, a 5.7 s.e. deviation of the coefficient from zero; and (2) Fit 'B' (figures 2-5), with AE = (2.3 X 10-7 ± 4.0 X 10-8)Z4 eV, x2 = 1.3, also a 5.7 s.e. deviation from zero. The deep valley of the x? surface (figure 1, 'w-line' or Fits 'A' or 'B') argues strongly for a discrepancy and that a power law with n ^ 4 (to within an uncertainty of about ± 0.5) is the best fit. The x? remains consistent with unity, arguing for a self-consistent data set. The consistent patterns of discrepancy can be seen in the plots. The power law dependence is robust and significant in all variations. Fits (1) and (2) ('B') lie within 1 s.e. of Fit 'A'.

There has been much confusion about the status of experiments at Z = 18. Our current Fit 'A' predicts a deviation from theory of +0.029(5) eV at Z =18, while [14] found +0.012(9) eV (±0.0077 eV without inclusion in quadrature of claimed theoretical uncertainty). This [14] is within two s.e. of both our predicted result and the previous theory, despite its low claimed uncertainty of 2.5 ppm (though, of course, in a different experimental regime). This measurement is a high-precision result using a powerful ion source (ECRIS), a new methodology, and discussion of a range of systematics [39]. The paper reports a z-transition, so it could not be discussed in terms of an earlier analysis of the w line consistency, but it can now be discussed in relation to a common trend found in the four lines. The inclusion or exclusion of

[14] does not significantly impact the primary or numerical conclusions, nor does it impact the magnitude (number of standard errors) of the discrepancy. Specifically, with or without this data point, the discrepancy is 5.7 s.e. The point also lies within the normal distribution of measured points relative to either Fit 'A' or Fit 'B'.

Including a second recent measurement [15] in the overall fit yields Fit 'C', which is also plotted in the figures, AE = (5.4 X 10-9 ± 1.1 X 10-9)Z5 eV, x2 = 1.9. This remains a 4.8 s.e. deviation from current theory, within about one s.e. of Fit 'B'. It [15] does skew the optimal order, but the significance is only marginally weakened and the clear pattern of discrepancy from theory remains manifest under all permutations. This result is still inconsistent with theory, with a probability of only 8 X 10-7 (4.8 s.e. using normal distributions). According to [14], the authors of [15] neglected at least one potentially large 5 ppm shift, especially compared to their claimed uncertainty of 1.5 ppm. Further, this accuracy implies that their published correction for over 60 ppm of line curvature has been corrected to an accuracy of approximately 1 ppm.

Table 1 lists all of the weighted means of the data included in our analysis. Fit 'A' included all data cited except [14, 15]; Fit 'B' included [14]; and Fit 'C' included [14, 15]. For completeness, table 2 lists all 63 experimental results considered herein. From [29], we include only the subset of their data that they designate as arising from 'direct measurements' of the satellite correction normalization ratios (Z < 28); if we include their higher-Z results in our analysis, it does not significantly change our conclusions, but it does entangle the measurement with complex theoretical modelling untested in this regime. For the measurement of Bruhns

Table 1. Experimental weighted mean values used in this work.

Z Discrepancy (eV) g (eV)

16 0.011624 0.0285

18 'Fit A' -0.01471 0.0198

18 'Fit B' 0.008 68 0.0072

18 'Fit C' 0.00209 0.0041

19 0.165 49 0.119

20 0.04957 0.186

21 0.128 42 0.151

22 0.13563 0.0415

23 0.00034 0.0736

24 0.373 93 0.316

26 0.23567 0.1089

27 -0.46935 0.632

32 0.423 17 0.1171

36 0.477 94 0.1298

54 1.1570 1.080

92 10.8261 29.04

st-i ti

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o- - -T>.

10 20 30 40 50 60

measurement number (increasing with Z)

Figure 6. Deviation from Fit 'A' of the data, published up through [15], in units of the published experimental error bars. The measurement number is given in table 2.

et al [33], we use their claimed absolute uncertainty (rather than their uncertainty relative to calculated values for calibration lines in other ions) for direct comparison with our present results and with other claimed absolute measurements. The consistency of the pattern of discrepancy is remarkable—the discrepancies lie on one side of theory—and this consistency across multiple spectral lines leads to the apparent universality of the fit.

The very recent result [15] stands apart, in part by virtue of its extremely small claimed uncertainty (figure 6). This datum would become consistent with the overall data set if the reported uncertainty were some three to six times the claimed value. Without such an expanded uncertainty, the probability that this point is consistent with the fit of the other points is P < 10-9, based upon the 6.1 s.e. discrepancy.

Table 2. Experimental data used in analysis.

Measurement # Z Element Line (eV) Energy (eV) a (eV) Discrepancy Reference

1 16 S w 2461.2735 0.4886 0.6443 [28]

2 16 S w 2460.6874 0.1465 0.0582 [29]

3 16 S w 2461.8000 3.0000 1.1708 [30]

4 16 S w 2460.6410 0.0320 0.0118 [31]

5 16 S w 2460.6700 0.0900 0.0408 [23]

6 16 S y 2447.0500 0.1100 -0.0939 [23]

7 18 Ar w 3139.6000 0.2500 0.0179 [32]

8 18 Ar w 3139.5830 0.0630 0.0009 [33]

9 18 Ar w 3139.5517 0.0366 -0.0304 [16]

10 18 Ar w 3140.1000 0.7000 0.5179 [27]

11 18 Ar w 3139.5810 0.0050 -0.0011 [15]

12 18 Ar w 3138.9000 0.9000 -0.6821 [34]

13 18 Ar x 3126.2830 0.0363 -0.0066 [16]

14 18 Ar y 3123.5208 0.0362 -0.0136 [16]

15 18 Ar z 3104.1480 0.0077 -0.0003 [14]

16 19 K w 3511.4048 0.4972 0.9432 [28]

17 19 K w 3510.5796 0.1229 0.1180 [35]

18 20 Ca w 3902.4273 0.1860 0.0496 [29]

19 21 Sc w 4315.5408 0.1510 0.1284 [35]

20 22 Ti w 4750.1702 0.9100 0.5261 [28]

21 22 Ti w 4749.7335 0.1662 0.0894 [35]

22 22 Ti w 4749.8520 0.0720 0.2079 [8]

23 22 Ti x 4733.8335 0.1311 0.0327 [9]

24 22 Ti y 4727.0667 0.1000 0.1294 [9]

25 22 Ti z 4702.0782 0.0723 0.1036 [9]

26 23 V w 5204.3904 1.0923 -0.7749 [28]

27 23 V w 5205.5922 0.5464 0.4269 [29]

28 23 V w 5205.2644 0.2082 0.0991 [35]

29 23 V w 5205.1000 0.1400 -0.0653 [17]

30 23 V x 5189.1200 0.2200 0.3822 [17]

31 23 V y 5180.2200 0.1700 -0.1064 [17]

32 23 V z 5153.8200 0.1400 -0.0762 [17]

33 24 Cr w 5682.6562 0.5209 0.5878 [29]

34 24 Cr w 5682.3176 0.3978 0.2492 [35]

35 26 Fe w 6700.7617 0.3621 0.3270 [29]

36 26 Fe w 6700.7254 0.2010 0.2907 [35]

37 26 Fe w 6700.9000 0.2680 0.4653 [18]

38 26 Fe w 6700.4025 0.3172 -0.0322 [36]

39 26 Fe x 6682.7000 0.2673 0.3661 [18]

40 26 Fe y 6667.5000 0.2667 -0.0786 [18]

41 27 Co w 7241.6439 0.6323 -0.4694 [29]

42 32 Ge w 10 280.3573 0.2715 0.1398 [22]

43 32 Ge w 10 280.7000 0.2200 0.4825 [19]

44 32 Ge x 10259.5155 0.3693 0.6416 [19]

45 32 Ge y 10220.9316 0.2275 0.1320 [22]

46 32 Ge y 10221.7911 0.3475 0.9915 [19]

Table 2. (Continued.)

Measurement # Z Element Line (eV) Energy (eV) tf (eV) : Discrepancy Reference

47 32 Ge z 10181.3324 0.5192 0.9456 [19]

48 36 Kr w 13 113.8000 1.2000 -0.6705 [55]

49 36 Kr w 13115.4500 0.3000 0.9795 [26]

50 36 Kr w 13 114.7800 0.7100 0.3095 [20]

51 36 Kr w 13 114.6800 0.3600 0.2095 [21]

52 36 Kr x 13 091.5300 0.8200 0.6643 [20]

53 36 Kr x 13 091.1700 0.3700 0.3043 [21]

54 36 Kr y 13 026.8000 0.3000 0.6835 [26]

55 36 Kr y 13 026.3000 0.7100 0.1835 [20]

56 36 Kr y 13 026.2900 0.3600 0.1735 [21]

57 36 Kr z 12 979.7200 0.6600 0.4544 [20]

58 36 Kr z 12979.6300 0.4100 0.3644 [21]

59 54 Xe w 30 629.1000 3.5000 -0.9512 [24]

60 54 Xe w 30 631.2000 1.2000 1.1488 [37]

61 54 Xe y 30209.6000 3.5000 3.3348 [24]

62 92 U w 100 626.0000 35.0000 15.1100 [25]

63 92 U y 96 171.0000 52.0000 1.3700 [25]

The body of experimental literature, arising from many different groups across a range of elements and using quite different experimental excitation and detection methods, is consistent with the approximately Z4 deviation that we report here. Other authors have considered experimental measurements of QED to deviate from the theories of past work, or have raised questions about specific values of Z [1, 35, 40, 41], but these conjectures have sometimes been reversed in subsequent reports [17, 21], reflecting the scarcity of all-Z data and large uncertainties at the time. Here, both by increasing the accuracy of our own measurement and by performing a meta-analysis of the global data set, we postulate and present statistically strong and systematically consistent evidence for a functional dependence that may relate to specific correlation and Feynman diagrams.

The titanium measurements are the first set of He-like ions in which a highly significant discrepancy has withstood comparison across multiple spectral lines. Previously, investigations typically have either had insufficient signal-to-noise, too narrow a spectral bandpass, or inadequate calibration accuracy needed to show such a pattern of internal consistency. By including extensive data sets from the earlier literature, we minimize the possibility of a specific experimental systematic. By observing and including several lines, we limit the possibility of any asymmetry or line blends from impurities shifting one line in any particular direction.

4. Harmonizing theory and experiment

At present, QED treatment of low-Z and high-Z few-electron systems is undertaken with significantly different starting points and mathematical techniques. This work bridges the two regimes in order to stimulate the development of an improved universal computational methodology. Establishing this is desirable from a fundamental perspective, and crucial for the

¿¿H Lamb Shift

uu xyz— lines Z4 fit at Ti2C+

Figure 7. Comparison of the current status of two key discrepancies of QED-sensitive measurements from accepted energy determinations, divided by the magnitude of the energy measured. The scales in different types of experiments are quite different. The error bar shown on each point is the standard error of the measurement. The label gives the ratio of the discrepancy to the uncertainty. The muonic hydrogen Lamb shift energy [48] is compared to the result using the CODATA rms proton charge radius [49]. The He-like wxyz-transition discrepancy is determined as the transition energy difference of our results from the theory of Artemyev [6], as a fraction of that theoretical energy at Z = 22.

reliability of a wide range of practical applications. These include new classes of calibration standards based upon hydrogenic and He-like energy levels [14, 42] and the multiplicity of novel laser techniques in high-field and high-energy-density applications [43]. These experimental probes of the quantum vacuum provide the foundations for the determination of current values of the constants of nature, including the Rydberg constant [44] and the fine-structure constant [45]. Finally, this work calls into question the degree to which such atomic physics understanding has converged, and points, like the muonic hydrogen work, to further critical inquiry.

One interpretation of the fact that the same universal fit seems to be consistent for the patterns of discrepancy for w, x, y, and z transitions is that the discrepancy could lie in the computation of the 1s2 ground-state energies and Lamb shift. (The QED corrections to the ionization energy scale in proportion to 1/n3 is proportional to the electron density at the nucleus (e.g., [11])). The evidence is at least suggestive of a common or similar discrepancy for z (1s2s 3S1 ^ 1s2 :S0) and w (1s2p 1P1 ^ 1s2 :S0), but there are few measurements of the z transition that meet the accuracy required.

In this case, we could once again have the possibility of a form factor, effective radius, or some such similar interaction, as has been proposed for the muonic hydrogen discrepancy. Indeed, a comparison of the magnitude of the muonic hydrogen discrepancy with the current status for He-like medium-Z systems is intriguing (figure 7). However, extensive theoretical investigation of that anomaly has thus far found no explanation based upon the effective radius, polarization of the nucleus, or shape.

If the 1s orbital is responsible, it does not prove an error of one-electron QED, which has been attested in experiments for one-loop terms. It could relate to an interplay between the 1 s electrons and their correlation energies. The former can be represented by Z4 terms; the latter by

Z or Z5. The various theoretical predictions consider their missing terms to be of different form and power law dependence. What this means is a matter of future work, rather than speculation. We do not impute a failure of two-loop terms, but rather suggest that a cause may lie in two-photon diagrams, or something far more intriguing.

In medium-Z ion transitions, a prior estimate of 0.1 eV was made for the magnitude of missing correlation effects to the QED contributions [6]. This may result in approximately 20ppm of uncertainty or a miscalculation of atomic transition energies [46]. A recent discussion has highlighted the importance of further investigation of the experimental discrepancies [47]. In the latter development, specific uncalculated terms of order Z3 are predicted. Theory predicts that the first-order QED corrections (vacuum polarization and self-energy) should scale as approximately Z4. Higher-order Feynman diagrams generally include log terms or additional powers of Za2. Correlation terms, especially for two-electron systems, generally involve shielding or coupling, which scales as powers of (1/Z), so the order of the polynomial n ^ 4 is a reasonable hypothesis.

Interestingly (G W F Drake, private communication), the leading term not included correctly by the unified method is of order a4Z4, in harmony with the Z4 scaling that we find for the discrepancy. This can be understood as follows. The second-order relativistic corrections are of leading orders a4Z6 and a4Z5 (in units of Ry). Both of these are fully accounted for by the unified method. The leading term not accounted for is therefore of order a4Z4, which is the next term in the 1/Z expansion of the higher-order relativistic corrections. The a4Z4 scaling of the uncertainty due to the combined effects of relativity and QED is stated explicitly on p 607 of [11], along with an estimate of the uncertainty from this source.

5. Conclusions and outlook to the future

Over the past several decades, techniques based on the refinement of the understanding of Bragg diffraction, coupled with the development of new methods of producing highly charged ions, have facilitated the measurement of the x-ray spectra of highly charged ions to an accuracy of approximately 10 ppm. Bragg-based measurements at the 1 ppm level raise numerous systematic errors (corrections due to n ^ 3 satellites, depth penetration of wavefields, detector registration, and curvature) that have not been adequately addressed in published results to date, and others of less well-defined magnitude in the case of highly charged ions excited by electron collisions (quantum interference shifts) [50, 51].

The quest for high-accuracy absolute spectroscopy in the low-Z ultraviolet-visible regime has advanced technology and provided powerful new tools for research and applications, yielding Nobel Prizes to Hansch [3] and to Wieman, Cornell, and Ketterle [52]. The work of Hansch in particular has pushed the uncertainty of the 1S-2S hydrogen transition energy to 4.2 parts in 1015 [53]. Core transitions in medium-Z systems cannot be addressed by conventional lasers, so new techniques need to be developed, as discussed here. Efforts in medium-Z systems are limited by available calibration techniques (typically to 15 ppm or so), but with lower fractional accuracy, they can probe similar physics due to the enhancement of contributions [54] (figure 7). A recent paper has provided evidence for a functional discrepancy of measurements of the He-like w line from advanced QED theory [8]. Here we find that this discrepancy also appears in a series of transitions (x, y, z, in addition to w), strengthening the significance of our original finding and allowing the possible origin of the discrepancy in the upper or lower levels

to be investigated. Of course, experimental limitations can be responsible for any discrepancy, but the pattern and independence of the result with data from different sources and groups helps to minimize this possibility. Work from our (and other) groups reported at recent conferences suggests that the trend of discrepancy with theory may be larger (or smaller) than presented here. We encourage more independent research in theory and experiment, and especially recommend blind protocols for analysis.

Our result can be directly related to Z4 or Z6(1/Z) expansion terms, for example, or to combinations with multiple terms. In other words, this is suggestive evidence that specific Feynman diagrams involving virtual photons and electron correlation are not fully accounted for. Of course, additional physics with a similar dependence may be present.

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