Q_{\text{EC}}-values of the Superallowed \beta-Emitters {}^{10}C, {}^{34}Ar, {}^{38}Ca and {}^{46}V

-values of the Superallowed -Emitters C, Ar, Ca and V

T. Eronen tommi.eronen@phys.jyu.fi    D. Gorelov    J. Hakala Department of Physics, P.O. Box 35 (YFL), FI-40014 University of Jyväskylä, Finland    J. C. Hardy Cyclotron Institute, Texas A&M University, College Station, Texas 77843, USA    A. Jokinen    A. Kankainen    I. D. Moore    H. Penttilä    M. Reponen    J. Rissanen    A. Saastamoinen    J. Äystö Department of Physics, P.O. Box 35 (YFL), FI-40014 University of Jyväskylä, Finland
July 15, 2019
Abstract

The values of the superallowed -emitters C, Ar, Ca and V have been measured with a Penning-trap mass spectrometer to be 3648.12(8), 6061.83(8), 6612.12(7) and 7052.44(10) keV, respectively. All four values are substantially improved in precision over previous results.

pacs:
21.10.Dr, 23.40.Bw, 27.20.+n, 27.30.+t, 27.40.+z,
preprint: APS/123-QED

I Introduction

Superallowed decay between nuclear analog states plays an important role in several fundamental tests of the three-generation Standard Model. It tests the Conservation of the Vector Current (CVC), probes for the presence of scalar currents, and is a key contributor to the most demanding currently available test of the unitarity of the Cabibbo-Kobayashi-Maskawa (CKM) matrix Towner2010a (). For these and other reasons, it has been a subject of continuous and often intense study for six decades. The most important features of these superallowed transitions, and the ones that make them so attractive, are that their measured values are nearly independent of nuclear-structure ambiguities and that they depend uniquely on the vector (and scalar, if it exists) part of the weak interaction.

To date, the measured values for transitions from ten different nuclei are known to 0.1% precision, and three more are known to between 0.1% and 0.3%. An analysis of these values Hardy2009 () recently demonstrated that the vector coupling constant, , has the same value for all thirteen transitions to within 0.013%, thus confirming a key part of the CVC hypothesis; and it sets an upper limit on a possible scalar current at 0.2% of the vector current. With both these outcomes established, the results could then be used to extract a value for , the up-down element of the CKM matrix, with which the top-row unitarity test of that matrix yielded the result 0.9999(6) Towner2010a (). This is in remarkable agreement with the Standard Model, and the tight uncertainty significantly limits the scope for any new physics beyond the model. Further tightening of the uncertainty would, of course, increase the impact of this result even more.

Neglecting for now the possibility of any scalar current, we can relate the value for a superallowed transition directly to the vector coupling constant, by the following equation Hardy2009 ():

(1)

where is defined to be the “corrected” value and GeVs. There are four small correction terms: is the isospin-symmetry-breaking correction; is the transition-independent part of the radiative correction; and the terms and comprise the transition-dependent part of the radiative correction, the former being a function only of the maximum positron energy and the atomic number, , of the daughter nucleus, while the latter, like , depends in its evaluation on the details of nuclear structure. The two structure-dependent terms and , which appear in Eq. 1 as a difference, together contribute 1% to most values Towner2008 (). Even so, at the current level of experimental precision, their theoretical uncertainties contribute significantly to the final -value uncertainties.

Experiments can help to reduce these theoretical uncertainties. A method has recently been proposed Towner2010b (), by which the structure-dependent corrections can be validated. The calculated corrections change considerably from transition to transition, and the validation entails a comparison of these changes against the experimental changes from transition to transition in the uncorrected values. In essence, validation depends on whether the calculated corrections produce a result consistent with CVC. The effectiveness of this validation process depends directly on the experimental precision of the values.

The value that characterizes any -transition depends on three measured quantities: the total transition energy, ; the half-life, , of the parent state; and the branching ratio, , for the particular transition of interest. The -value is required to determine the statistical rate function, , while the half-life and branching ratio combine to yield the partial half-life, . It is important to recognize, though, that varies approximately with the fifth power of : If the fractional uncertainty in the measured  value is 1, the corresponding uncertainty in is 5. Thus, the precision required for -value measurements is substantially higher than that required for half-lives and branching ratios.

We report here -value results for C, Ar, Ca and V with fractional uncertainties in the range (1-5), substantially better than any previous measurements for these transitions, and low enough that, with improvements in their half-lives and branching ratios, the uncertainties in these values could in principal be reduced to , a factor of five to ten below the uncertainties of the best-known cases today.

The superallowed decay of C is a particularly interesting case. If scalar currents exist, they would lead to a discrepancy between the values for the transitions in light nuclei and the average value for the heavier nuclei (see Fig. 7 in Ref. Hardy2009 ()). In particular, the decays of C and O are the most sensitive to the presence of a scalar current. Improved experimental precision for these two cases would have a significant impact on the search for a scalar current. If it were to be found, of course, that would constitute new physics beyond the standard model. Our C measurement reported here is the first step along this path.

Ii Experimental Method

Target Reaction Product(s)
B () 12 MeV B(,) C
B(,) B
KCl 35 MeV Cl(,2) Ar
Cl(,) Cl+Cl
Cl(,2) S
KCl 35 MeV K(,2) Ca
K(,) K+K
K(,2) Ar
Ti ( 20 MeV Ti(,) V
Table 1: The proton beam energies and target combinations used in these measurements. Where applicable, the percentage of isotopic enrichment is given in parenthesis. Only the Ti target was self supporting; all others were evaporated onto thin nickel foil. In all cases, the target thickness was a few mg/cm.

The targets, proton beam energies, and reactions we employed in these measurements are listed in Table 1.

The experiments were carried out with the JYFLTRAP Penning-trap mass spectrometer at the University of Jyväskylä, Finland Jokinen2006 (). The ions of interest were produced from fusion-evaporation reactions induced by protons from the K130 cyclotron, with the reaction products being collected and separated by the IGISOL technique Aysto2001 (), which is both universal and fast, enabling extraction of beams of any element within less than 100 ms. The recoiling nuclei are primarily slowed down in the target itself but are ultimately thermalized in a helium-filled stopping volume Huikari2004 (). The ions flow with helium out from the gas cell and into a sextupole ion guide Karvonen2008 (), after which they are electrostatically accelerated to an energy of 30 keV. These energetic ions are then separated with a 55 dipole magnet, which has a mass resolving power () of about 500, and injected into a radiofrequency quadrupole (RFQ) structure for ion-beam cooling and bunching Nieminen2001 (). Finally, each bunch is released to the JYFLTRAP Penning-trap setup where the ions’ masses are measured with the time-of-flight ion-cyclotron-resonance (TOF-ICR) technique Graff1980 ().

ii.1 Ion preparation

Figure 1: Quadrupole frequency scan of the purification trap. The trap was tuned in this case to have a mass resolving power of about 30,000, which is enough to separate isobars but not the isomeric states of Cl.

Ideally only one ion at a time is needed for a measurement, but in practice a few ions are usually used. However, the ions of interest typically comprise less than 1% of the mass-separated beam from IGISOL, so to have, for example, a few Ar ions in a bunch, we have to collect 2-3 orders-of-magnitude more ions — mostly Cl and S — in the RFQ buncher. Once a large enough bunch has been collected, it is sent to the first of the two Penning traps that comprise the JYFLTRAP setup. This first trap contains helium buffer gas and serves to purify the sample. In it, the ions of interest are spatially separated with the sideband cooling technique Savard1991 (). After separation, the ions are extracted towards the second Penning trap, their path to that trap being via an electrode, in which there is a narrow central channel 2-mm in diameter. Only the centered ions of interest can pass through this channel, while the other ions hit the electrode. The transmitted ions are then captured in the second, precision Penning trap, which is operated in vacuum. There, the TOF-ICR mass measurement could in principal be initiated.

However, in the case of close-lying isomeric states purity is not yet assured. As shown in Fig. 1 for the mass-34 measurements, the purification process in the first Penning trap is sufficent to make clean bunches of Ar, but it is not enough to separate Cl from Cl. The same problem occurs in the case of mass-38 as well. For these measurements we used the so-called Ramsey cleaning technique Eronen2008a (), in which a further purification is accomplished by use of a dipole rf electric field to drive the unwanted ions to large cyclotron orbits in the gas-free precision trap. The excitation pattern and duration are chosen so that, upon completion, ions in the unwanted state have a large orbit. The ions are then transferred back to the purification trap and, en route, the unwanted ions hit the electrode rather than passing through the narrow central channel. An example of a cleaning frequency scan is shown in Fig. 2.

Figure 2: Dipole frequency scan in the precision trap for bunches containing both Cl and Cl. With an excitation time-pattern of 10/20/10 ms (on/off/on) a mass resolving power was obtained. The two states of Cl are cleanly separated.

Even with ions that did not require such high-precision cleaning, we chose to transfer them back from the precision trap to the purification trap. There the mono-isomeric ion sample was recooled and recentered with the sideband cooling technique Savard1991 (). Only after this second purification step was the ion bunch sent to the precision trap for the TOF-ICR mass measurement. We found that this additional cooling step significantly improved the quality of the measured TOF-ICR resonances and thus improved our precision. The full ion preparation cycle is illustrated in Fig. 3.

Figure 3: The measurement cycle.

ii.2 TOF-ICR measurement

In these measurements the time-of-flight ion-cyclotron resonance (TOF-ICR) technique Graff1980 () has been applied not only in conventional square-wave mode Konig1995 () but also in time-separated (Ramsey-type) mode George2007a (); Kretzschmar2007 (). The measurement procedure starts with a phase-locked dipole rf electric field used to increase slightly the magnetron orbit radius of the ions Blaum2003 (). In measurements reported in this work, this excitation was applied for a single magnetron period of about 5.5 ms and with an amplitude of about 50 mV.

Following the dipole magnetron excitation, a quadrupole excitation was switched on to couple the two radial trap eigenmotions. The frequency of this quadrupole excitation was scanned over a range that included the sum of the two eigenfrequencies , which is also the cyclotron frequency of ions in the absence of any trapping electric fields: viz.

(2)

where and are the frequencies of the two radial motions, commonly called the trap-modified cyclotron and magnetron frequencies, respectively; is the charge-to-mass ratio of the ions and is the magnetic field. The duration we could use for the excitation was limited not only by the half-life of the ions of interest, but also by ion-motion damping effects caused by residual gas present in the precision trap. These effects are much stronger with lighter ions. The excitation durations we used were between 200 ms and 400 ms.

After completion of the quadrupole excitation, the ions were released from the trap in the direction of a microchannel plate (MCP) detector. As ions travel through a region with high magnetic field gradient, their radial energy converts to axial velocity, so ions starting with more radial energy will gain more speed and thus arrive earlier at the detector than the ions that have not been resonantly excited. Since the energy content of the trap-modified cyclotron motion () is of the order of several eV and the energy of the magnetron motion () is only a few eV, the resonantly excited ions can have as much as a factor of two shorter time-of-flight to the MCP detector than non-excited ions. Figure 4 shows a sample TOF-ICR curve for Ar, in which the measured ion time-of-flight is plotted as a function of the quadrupole-excitation frequency over a 30 Hz range. In this case, the ion-motion excitation was accomplished by use of Ramsey’s method of time-separated oscillatory fields.

Figure 4 also shows a fit to the experimental data. For the mass-34 measurement illustrated in the figure, and also for the mass-38 and mass-46 measurements, we took the shape of the Ramsey-type resonance from Ref. George2007a (). For the mass-10 measurements we could not use the Ramsey procedure (see Sec. III.1 for more details) and had to revert to the conventional resonance procedure, for which we took the shape of the resonance curve from Ref. Konig1995 (). Very recently, the effects of ion-motion damping due to collisions with rest gas atoms have been incorporated into the function describing the Ramsey resonance shape George2010 (). Part of our data was checked with both fitting functions. No significant shifts were seen in the results so, for the analysis presented here, we used the function corresponding to the ideal lineshape.

Figure 4: (color online) A TOF-ICR curve measured for Ar ions. An excitation time pattern of 25/150/25 ms (on/off/on) was used. The black circles (with error bars smaller than the points) are time-of-flight averages for each frequency. The (blue) pixels represent the number of detected ions: the darker the pixel the more ions it represents. The solid (red) line is the fit to the experimental data. Note that the averages include some non-resonant background as well as the resonant Ar ions, which accounts for why the averages do not go through the densest concentration of pixels. See Sec. III.2 for more details.

ii.3 value determination

The value is the total decay energy of the transition. It can be expressed as the difference between the mass of the parent atom and that of the daughter :

(3)

In terms of the measured cyclotron frequencies for the singly-charged ions of the parent and daughter, and respectively [see Eq. (2)], the value can be written as

(4)

where is the electron rest mass and arises from the atomic-electron binding-energy difference between the parent and daughter atoms. The latter contributes at most about 3 eV for the cases we report on here, since we studied only singly-charged ions.

ii.4 Control of systematic errors

The values reported in this work were all measured as parent-daughter doublets, both with the same value of . Thus we can apply Eq. (4) to our results. Furthermore, we obtained the cyclotron frequency ratio by interleaving scans of the two ion species, about 30 s for one, then 30 s for the other, with the alternation repeated for a number of hours. The temporal drift of the magnetic field is of the order of  min Rahaman2007a (), so any shifts between one 30-s scan and the next would have made a negligible contribution to the frequency ratio.

We analyzed the data by splitting the alternating parent- and daughter-ion scans into approximately 30-minute intervals, each consisting of about 30 pairs of scans. The 30 scan-pairs were not merged to form just one resonance curve for each ion species but several, the data being split according to the number of ions recorded per bunch. This allowed us to test for possible shifts in the resonance frequency due to multiple ions being stored in the trap Kellerbauer2003 (). (Our procedures will be described more fully for each measured value in Sec. III.) The time-of-flight resonance results obtained for each 30-minute interval were then fitted separately for both ion species to get a frequency ratio. The final frequency ratio for a particular doublet was obtained from the weighted average of its interval results.

Figure 5: A series of fitted cyclotron frequencies for Ar and Cl ions (lower panel). Each frequency point includes the results of 30 interleaved scans. The top panel shows the deviation of the corresponding frequency ratios, from the average frequency ratio.

As an example of the quality of results, Fig. 5 shows the individual cyclotron frequencies obtained for the Ar-Cl pair, together with the deviations of the frequency ratios from the average value. It can be seen that, although the magnetic field fluctuates, the cyclotron-frequency ratios were consistent over an eight-hour period on one day, and a five-hour period a day later.

We have also considered other possible sources of systematic error. Tiny differences between the measured and the actual cyclotron frequency could result from a slight misalignment of the electric- and magnetic-field axes, and from distortion in the quadrupole electric field Gabrielse2009 (). Because the ion-pairs in our measurements are doublets, the effect on the frequency ratio would be negligibly small compared to the statistical uncertainty. Mass-dependent shifts Elomaa2009b () are negligible as well, also because we are working with doublets having the same mass number. Previous measurements with JYFLTRAP have successfully reproduced accurately known isomeric excitation energies or values Rahaman2008a (); Eronen2009a () down to a relative precision of .

In the measurements reported here, by far the largest contribution to each final uncertainty is the statistical component, which originates from counting statistics and the fitting procedure.

Iii Results and Analysis

The values of the superallowed emitters C, Ar, Ca and V were all measured during a 9-day period of beam time in May 2010, only a month before the IGISOL and JYFLTRAP facilities were shut down in preparation for being moved to a different target location. Our four different frequency-ratio measurements are described individually in the following sections.

iii.1 C

The value for C proved to be the most difficult one we have measured so far. Mass-10 being the lightest mass ever measured with JYFLTRAP, we carefully tuned the setup before the on-line experiment began, using stable B and C ions from an off-line ion source. We found that the buffer-gas pressure of the purification Penning trap had to be significantly reduced since the cooling effect of the helium gas is much stronger for light ions. Even so, damping of the TOF-ICR resonance was rather pronounced and thus we could only use short excitation times. An additional difficulty was that the transmission of the RFQ was rather poor. Nevertheless, in the end enough ions could be delivered to the Penning trap for a successful measurement.

Unlike our experience with heavier ions (), a rather strong dipole component in the quadrupole field was apparent, as evidenced by a clear resonance observed at frequency , about 170 Hz away from the sideband. This prevented our using Ramsey excitation, since the two resonance patterns overlapped. Instead, we used a conventional TOF-ICR resonance technique with a 200 ms excitation time.

Figure 6: values obtained for each set of 30 scans. All the data were analyzed to account for multiple stored ions. In the data denoted by “A” the maximum number of ions per accepted bunch was 5, while those denoted “B” included a maximum of 3. We obtained the final value by taking the unweighted average of “A” and “B” and applying an error bar derived by taking the larger uncertainty of the two and adding the difference between “A” and “B” in quadrature.

Several checks of the data were done in order to ensure that the measurements yielded correct results despite the strong dipole component. In addition to measuring the value between C and B, we also measured the well known mass of stable C Audi2003 (), using C as the reference ion. Also, parameters like dipole-magnetron-excitation amplitude and ion-transfer time between the two traps were varied to check that there was no shift in the measured frequency ratio when the ions occupied a different fraction of the trap volume.

In all, we obtained seven sets of data for the C value and three for the C mass. The data were analyzed using count-rate class analysis Kellerbauer2003 () to account for the effects of multiple stored ions in the trap. Moreover, to double-check our results, the class division was done in two different ways. In the first analysis, we subdivided the data into three classes according to how many ions were in each bunch, 1-2, 3 or 4-5. In the second analysis only two classes were retained, those with 1 ion/bunch and those with 2-3 ions/bunch. As can be seen from Fig. 6, the results from each group of 30 interleaved scans changed from one analysis to the other but the two average frequency ratios were consistent with one another. Our final frequency ratio and value appear in Table 2, and the latter is compared with previous measurements of the value derived from (,) threshold measurements Barker1984 (); Barker1998 () in Fig. 7.

The value given in Table 2 is, of course, for the ground-state-to-ground-state transition. The superallowed transition feeds the state in B, which is at 1740.07(2) keV Hardy2009 (), so our result for the transition populating the ground state corresponds to a value for the superallowed transition of 1908.05(8) keV.

Ion A Ion B Frequency ratio or (keV)
Mass 10:
C B 1.000 391 157(9) 13648.12(8)
Mass 34:
Ar Cl 1.000 191 551 8(27) 16061.82(9)
Ar Cl 1.000 186 923 2(33) 15915.37(10)
Cl Cl 1.000 004 630(8) 11146.52(26)
Ar S 1.000 365 151(6) 11553.51(19)
Mass 38:
Ca K 1.000 186 955 0(28) 16612.15(10)
Ca K 1.000 190 632 6(27) 16742.19(10)
K K 1.000 003 681 5(38) 11130.21(14)
Ca Ar 1.000 357 913 2(32) 12656.36(11)
Mass 46:
V Ti 1.000 164 760 8(23) 17052.44(10)
Table 2: The obtained frequency ratios and the derived values or energy differences for ions having =10, 34, 38 and 46.

Our control measurement of the C-to-C mass difference yielded a frequency ratio of CC  =  1.083  616  728(5). This corresponds to a mass excess for C of 3125.04(6) keV, which is in perfect agreement with the high-precision literature value of 3125.011(1) keV Audi2003 (). This further confirms that our C value does not suffer from any significant systematic error.

iii.2 Ar

To determine the value for Ar, we measured its frequency ratio, not only compared with Cl but also with the high-spin () isomer Cl and with its grand-daughter S. The two states in Cl are only 146 keV apart, but were easily separated as we have done before Eronen2009a () using the Ramsey cleaning method. The cyclotron frequencies were measured using a Ramsey-type excitation with the pattern 25/150/25 ms (on/off/on). This short excitation time was used because of the residual-gas impurities present in the precision trap. When we used longer times, we observed significant charge-exchange losses for all ion species. The effect of these losses is also evident in Fig. 4, where some ions are seen to appear at 170 s time-of-flight regardless of the excitation frequency. This accounts for why the average time-of-flight points do not go through the darkest concentration of pixels in the figure: the contaminants, which appear at 170 s and are probably singly charged O molecules, serve to pull the average up a bit.

To take this constant time-of-flight background into account, we added two additional fit parameters: a constant time of flight for the background, and the ratio of the number of background counts to that of the resonant ions. Despite the presence of contaminating ions, no systematic shifts of the fitted frequencies were observed as we increased the number of stored ions in the trap.

Figure 7: Comparison of our value measurements, labelled JYFLTRAP, with previous measurements. For each transition, our result is plotted at 0 on the abscissa, and the other results are plotted as differences . The references from the top down are Barker1984 (); Barker1998 (); Hardy1974b (); Herfurth2001 (); Herfurth2002 (); Ringle2007 (); George2007 (); Squier1976 (); Savard2005 (); Eronen2006 (); Faestermann2009 () respectively.
Method (keV)
Ar—Cl direct 6061.82(9)
via Cl 6061.89(28)
via S 6061.85(20)111The mass difference between Cl and S [5491.662(47) keV] was taken from Ref. Eronen2009a ().
FINAL 6061.83(8)
Table 3: values for the Ar-to-Cl superallowed transition obtained via three different reference ions. The input data are taken from Table 2 and from Refs. Snover1971 (); Eronen2009a ().

The frequency ratios and values we obtained from these measurements are compiled in Table 2 and the final derived values are in Table 3. Our value for the excitation energy of the Cl isomer, 146.52(26) keV, agrees well with our previous JYFLTRAP value, 146.29(10) keV, which we reported in 2009 Eronen2009a (), and with a more precise value, 146.36(3) keV, obtained Snover1971 () from its decay ray. Furthermore, the three Ar-Cl values, derived via three different paths, are in remarkable agreement with one another. Our final result for the value of this superallowed transition is 6061.83(8) keV.

This value is compared with previous measurements of the Ar value Hardy1974b (); Herfurth2001 (); Herfurth2002 () in Fig. 7. The earliest of these results Hardy1974b () was from a (,) -value measurement; the later two Herfurth2001 (); Herfurth2002 () were Penning-trap measurements from ISOLTRAP. Only one of these results—the most recent value from ISOLTRAPHerfurth2002 ()—has an uncertainty comparable to ours, although even its uncertainty is five times larger than ours. However, our result disagrees by three of the latter’s standard deviations. We have no definitive explanation for this discrepancy but there is an important difference between the two measurements: ours obtained the Ar value directly by a measurement of the frequency ratio of the daughter to the parent ions. The ISOLTRAP measurement used K as its reference ion. Thus, to get the Ar value, the mass of the daughter Cl also had to be linked to K. This link via K – 5 mass units away – may well have been the source of error.

iii.3 Ca

Our measurement of the Ca value was conducted in the same way as the measurement just described for Ar. The daughter nucleus in this case, K, has a low-lying isomeric state just like Cl has, although it is the isomeric state in K that has spin and parity of and the ground state that is . These states are only 130 keV apart but were easily separated with the Ramsey cleaning method. As with the Ar measurement, we obtained the value for Ca, not only by a direct daughter-parent frequency ratio, but also via the high-spin ground state of K and via the granddaughter nucleus Ar. Charge-exchange background was evident in the Ar frequency measurement but not for the other ion species. We used a Ramsey excitation pattern of 25/350/25 ms (on/off/on) for all measurements except for one set of data connecting Ca to Ar. In that case, we used a shorter excitation pattern, 25/150/25 ms, in order to confirm that there was no change in the results as the number of contaminant ions increased.

Our measured frequency ratios and values appear in Table 2 and the final derived values are in Table 4. Our measured value for the excitation energy of the K isomer, 130.21(14) keV, agrees well with our previous JYFLTRAP value, 130.13(6) keV, and with the previously accepted value of 130.4(3) keV Endt1990 (), which is the least precise. Furthermore, the three Ca-K values, derived via three different paths, are in excellent agreement with one another. Our final result for the value of this superallowed transition is 6612.12(7) keV.

Method (keV)
Ca—K direct 6612.15(10)
via K 6611.99(16)
via Ar 6612.14(12)111The mass difference between K and Ar [6044.223(41) keV] was taken from Ref. Eronen2009a ().
FINAL 6612.12(7)
Table 4: values for the Ca-to-K superallowed transition obtained via three different reference ions. The input data are taken from Table 2 and from Ref. Eronen2009a ().

This value is compared in Fig. 7 with the two previous determinations of the Ca value, both based on Penning-trap mass measurements, one from the LEBIT trap Ringle2007 () and the other from ISOLTRAP George2007 (). These two values, which are quite recent, and the new measured result we report here all agree within error bars. Our value, though, is about six times more precise than that in Ref. Ringle2007 () and ten times more precise than Ref. George2007 ().

iii.4 V

We have already measured the value for the superallowed decay of V once before at JYFLTRAP, in 2006 Eronen2006 (). Our motivation for remeasuring it now was to improve the precision of the result. Since 2006 we have introduced a number of improvements to our system, most notably the rapid alternation of parent-daughter frequency scans and the use of Ramsey excitation. The excitation pattern used for this measurement was 25/350/25 ms (on/off/on). The resonances we obtained were clean and showed no evidence of any charge-exchange products. The frequency ratio and corresponding value are presented in Table 2.

Our new value is compared with the four previous measurements of the V value Squier1976 (); Savard2005 (); Eronen2006 (); Faestermann2009 () in Fig. 7. Our new result agrees with our previous one Eronen2006 () but has an uncertainty smaller by a factor of three. In fact, our new result also agrees with the other three measurements, one of which is from the CPT Penning trap Savard2005 (), another is from a (He,) reaction value Faestermann2009 (), and the third is from a (,) threshold measurement Squier1976 (). All three have uncertainties at least a factor of three greater than our new result.

Iv Conclusions

Our four new -value results for superallowed transitions are collected in Table 5, where they are compared with the equivalent values that appeared in the most recent survey of superallowed nuclear decay Hardy2009 (). In all cases, our new results have reduced the uncertainties considerably, although in the case of Ar the reduction is constrained by the inconsistency between our result and one of the previous measurements Herfurth2002 () (see Fig. 7). That inconsistency leads to a normalized of 7 for the average and, following the procedures used in Ref. Hardy2009 (), we increase the uncertainty on the average by a scale factor equal to the square root of the normalized .

values (keV)
Parent Daughter this work surveyHardy2009 () average
C B() 1908.05(8) 1907.87(11) 1907.99(7)
Ar Cl 6061.83(8) 6062.98(48)  6061.86(21)
Ca K 6612.12(7) 6611.75(41) 6612.11(7)
V Ti  7052.44(10) 7052.40(16) 7052.45(9)
Table 5: The four values for superallowed transitions that were obtained in this work. Also shown are the equivalent values quoted in the most recent survey of data Hardy2009 () and the new weighted averages including our measurements.

Although our improvement in -value precision for these four cases is significant, our results do not in themselves reduce the uncertainty in the corresponding values. For each case, the uncertainty in its value is dominated by another property of the transition: For C, Ar and Ca, it is the branching ratio that dominates, while for V it is the half-life. What our results do is to provide values with fractional uncertainties that are comfortably below what is likely to be achieved in the near future for branching ratios or half-lives. Thus, whatever experimental improvements can be achieved in reducing the branching-ratio uncertainties for the decays of C, Ar and Ca, that reduction will translate directly into reduced -value uncertainties; and the same argument applies to the half-life of V.

To give one example, the branching ratio for the superallowed transition from Ar is currently known to a fractional uncertainty of and its half-life to Hardy2009 (). The fractional uncertainty we report here for its value is , which corresponds to a fractional uncertainty on the statistical rate function of , a factor of six better than the half-life and a factor of 35 better than the branching ratio. Because Ar has a rather favorable decay scheme, it should be possible with currently available techniques to reduce the branching-ratio uncertainty to or even below that. This would lead to an -value for Ar at essentially that same precision. Then it would become possible for the first time to compare at the 0.1% level a mirror pair of superallowed transitions, ArCl and ClS, a comparison that would help to distinguish among the various models used to calculate the isospin-symmetry-breaking correction to superallowed decays Towner2010b ().

It is also interesting to note that our measurement has slightly increased the value for the C superallowed decay. If we take the average value listed in Table 5 and include a new half-life measurement for C Barker2009 () together with the data listed in the 2009 survey Hardy2009 (), we obtain an value for the C superallowed transition of s. This is slightly outside error bars from the average of all values, 3072.08(79) s, obtained in the 2009 survey. If this discrepancy were to be confirmed by an improved branching-ratio value for C and by a similarly high value for the O decay, it could signal the appearance of a scalar current (see Ref. Hardy2009 ()). With this motivation, it is our plan in future to measure the -value of the superallowed transition from O. Obviously, an improved value for the C branching ratio would also be very welcome.

Acknowledgements.
This work has been supported by the EU 6th Frame- work programme “Integrating Infrastructure Initiative- Transnational Access” Contract No. 506065 (EURONS) and by the Academy of Finland under the Finnish Centre of Excellence Programme 2006-2011 (Nuclear and Accelerator Based Physics Programme at JYFL). JCH was supported by the U. S. Department of Energy under Grant DE-FG03-93ER40773 and by the Robert A. Welch Foundation under Grant no. A-1397.

References

  • (1) I.S. Towner and J.C. Hardy, Rep. Prog. Phys. 73, 046301 (2010).
  • (2) J. C. Hardy and I. S. Towner, Phys. Rev. C 79, 055502 (2009).
  • (3) I.S. Towner and J.C. Hardy, Phys. Rev. C 77, 025501 (2008).
  • (4) I.S. Towner and J.C. Hardy, Phys. Rev. C 82, 065501 (2010)
  • (5) A. Jokinen et al., Int. J. Mass Spectrom. 251, 204 (2006).
  • (6) J. Äystö, Nucl. Phys. A 693, 477 (2001).
  • (7) J. Huikari et al., Nucl. Instrum. Methods Phys. Res., Sect. B 222, 632 (2004).
  • (8) P. Karvonen et al., Nucl. Instrum. Methods Phys. Res., Sect. B 266, 4794 (2008).
  • (9) A. Nieminen et al., Nucl. Instrum. Methods Phys. Res., Sect. A 469, 244 (2001).
  • (10) G. Gräff, H. Kalinowsky, and J. Traut, Z. Phys. A 297, 35 (1980).
  • (11) G. Savard et al., Phys. Lett. A 158, 247 (1991).
  • (12) T. Eronen et al., Nucl. Instrum. Methods Phys. Res., Sect. B 266, 4527 (2008).
  • (13) M. König et al., Int. J. Mass Spectrom. 142, 95 (1995).
  • (14) S. George et al., Int. J. Mass Spectrom. 264, 110 (2007).
  • (15) M. Kretzschmar, Int. J. Mass Spectrom. 264, 122 (2007).
  • (16) K. Blaum et al., J. Phys. B: At., Mol. Opt. Phys. 36, 921 (2003).
  • (17) S. George et al., Int. J. Mass Spectrom. 299, 102 (2010).
  • (18) S. Rahaman et al., Eur. Phys. J. A 34, 5 (2007).
  • (19) A. Kellerbauer et al., Eur. Phys. J. D 22, 53 (2003).
  • (20) G. Gabrielse, Int. J. Mass Spectrom. 279, 107 (2009).
  • (21) V.-V. Elomaa et al., Nucl. Instrum. Methods Phys. Res., Sect. A 612, 97 (2009).
  • (22) S. Rahaman et al., Phys. Lett. B 662, 111 (2008).
  • (23) T. Eronen et al., Phys. Rev. Lett. 103, 252501 (2009).
  • (24) P. H. Barker and S. M. Ferguson, Phys. Rev. C 38, 1936 (1988).
  • (25) S. C. Baker, M. J. Brown, and P. H. Barker, Phys. Rev. C 40, 940 (1989).
  • (26) G. Audi et al., Nucl. Phys. A729, 327 (2003).
  • (27) P. H. Barker and R. E. White, Phys. Rev. C 29, 1530 (1984).
  • (28) P. H. Barker and P. A. Amundsen, Phys. Rev. C 58, 2571 (1998).
  • (29) K. A. Snover et al., Phys. Rev. C 4, 398 (1971).
  • (30) J. C. Hardy et al., Phys. Rev. C 9, 252 (1974).
  • (31) F. Herfurth et al., Nucl. Instrum. Methods Phys. Res., Sect. A 469, 254 (2001).
  • (32) F. Herfurth et al., Eur. Phys. J. A 15, 17 (2002).
  • (33) P.M. Endt, Nucl. Phys. A 521, 1 (1990).
  • (34) R. Ringle et al., Int. J. Mass Spectrom. 262, 33 (2007).
  • (35) S. George et al., Phys. Rev. Lett. 98, 162501 (2007).
  • (36) G.T.A. Squier, W.E. Burcham, S.D. Hoath, J.M. Freeman, P.H. Barker and R.J. Petty, Phys. Lett. 65B, 122 (1976).
  • (37) G. Savard et al., Phys. Rev. Lett. 95, 102501 (2005).
  • (38) T. Eronen et al., Phys. Rev. Lett. 97, 232501 (2006).
  • (39) T. Faestermann, R. Hertenberger, H.-F. Wirth, R. Krücken, M. Mahgoub and P. Maier-Komor, Eur. Phys. J. A, 42, 339 (2009).
  • (40) P.H. Barker, K.K.H. Leung and A.P. Byrne, Phys. Rev. C 79, 024311 (2009).
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