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Journal ArticleDOI

Concerning the time dependence of the decay rate of 137Cs.

TL;DR: It is found that the PTB measurements of the decay rate of (137)Cs show no evidence of an annual oscillation, in agreement with the recent report by Bellotti et al., and is consistent with the finding that different nuclides have different sensitivities to whatever external influences are responsible for the observed periodic variations.
About: This article is published in Applied Radiation and Isotopes.The article was published on 2013-04-01 and is currently open access. It has received 26 citations till now. The article focuses on the topics: Nuclide.

Summary (1 min read)

2. Analysis of PTB measurements

  • For present purposes, the authors have found it convenient to adopt sections of 500 measurements.
  • This spectrogram exhibits a strong annual oscillation from 2003 to 2005.
  • The plot derived from 133Ba data is shown in Fig.

3. Discussion

  • The authors next review in more detail previous reports concerning the decay rate of 137Cs.
  • Thermal expansion of the lucite, which has an expansion coefficient of 7:1 10 5 cm=cm=1C (10.02, 2012), would have been the same for the two standards, and hence expansion due to temperature would not be a likely source of any seasonal variations.
  • It is well known that the output of the detector is relatively insensitive to changes in the detector bias voltage, since the voltage is high enough to prevent recombination of the electron/ion pairs generated, but too low to cause electron multiplication.
  • Notably, the decay rate of 226Ra shows strong evidence of an annual oscillation in the earlier dataset but weaker evidence for such an oscillation in the later dataset (Fig. 4).

4. Conclusions

  • The authors purpose here has been to present new data, for 133Ba and 137Cs, which were measured on the same detector system for the same time period, where one isotope (133Ba) exhibited a clear annual periodicity and the other (137Cs) did not.
  • This result, in addition to the results of decay experiments listed in Table 1, indicates that the failure to observe the annual (or other) periodicity in one isotope does not exclude that possibility in others.
  • More specifically, the results presented in Table 1 in support of time-varying nuclear decay rates cumulatively represent over 60 years of data collection, in comparison to the 0.5 years of data from Bellotti et al. (2012).
  • Clearly, a new series of experiments with a variety of nuclides and a variety of detectors would help to determine definitively whether the amplitudes and phases of annual oscillations are steady or variable and, if variable, the characteristics of the variability.

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Citations
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Journal ArticleDOI
TL;DR: There is no indication of a natural impediment against sub-permille accuracy in half-life determinations, renormalisation of activity to a distant reference date, application of nuclear dating for archaeology, geo- and cosmochronology, nor in establishing the SI unit becquerel and seeking international equivalence of activity standards.

46 citations


Cites background or methods from "Concerning the time dependence of t..."

  • ...Authors of both convictions expressed the need for collecting evidence for different radionuclides measured with different detection techniques [7,11,13,18,23]....

    [...]

  • ...Evidence has been collected to demonstrate instabilities in the decay of other radionuclides [10,11] and by means of time-frequency analysis periodicity at shorter and longer term than 1 year have been claimed [11–13]....

    [...]

Journal ArticleDOI
TL;DR: The most stable activity measurements of alpha decaying sources set an upper limit between 0.0006% and 0.006% to the amplitude of annual oscillations in the decay rate.
Abstract: Claims that proximity to the Sun causes variation of decay constants at permille level have been investigated for alpha decaying nuclides. Repeated decay rate measurements of Po-209, Ra-226, Th-228, U-230, and Am-241 sources were performed over periods of 200 d up to two decades at various nuclear metrology institutes around the globe. Residuals from the exponential decay curves were inspected for annual oscillations. Systematic deviations from a purely exponential decay curve differ in amplitude and phase from one data set to another and appear attributable to instabilities in the instrumentation and measurement conditions. The most stable activity measurements of alpha decaying sources set an upper limit between 0.0006% and 0.006% to the amplitude of annual oscillations in the decay rate. There are no apparent indications for systematic oscillations at a level of weeks or months. Oscillations in phase with Earth's orbital distance to the sun could not be observed within 10(-5)-10(-6) range precision.

41 citations

Journal ArticleDOI
TL;DR: The hypothesis that seasonal changes in proximity to the Sun cause variation of decay constants at permille level has been tested for radionuclides disintegrating through electron capture and beta plus decay as mentioned in this paper.
Abstract: The hypothesis that seasonal changes in proximity to the Sun cause variation of decay constants at permille level has been tested for radionuclides disintegrating through electron capture and beta plus decay. Activity measurements of 22Na, 54Mn, 55Fe, 57Co, 65Zn, 82+85Sr, 90Sr, 109Cd, 124Sb, 133Ba, 152Eu, and 207Bi sources were repeated over periods from 200 d up to more than four decades at 14 laboratories across the globe. Residuals from the exponential nuclear decay curves were inspected for annual oscillations. Systematic deviations from a purely exponential decay curve differ from one data set to another and appear attributable to instabilities in the instrumentation and measurement conditions. Oscillations in phase with Earth's orbital distance to the sun could not be observed within 10−4–10−5 range precision. The most stable activity measurements of β + and EC decaying sources set an upper limit of 0.006% or less to the amplitude of annual oscillations in the decay rate. There are no apparent indications for systematic oscillations at a level of weeks or months.

35 citations

Journal ArticleDOI
TL;DR: In this article, the results of time-series analyses of data, kindly provided by the Physikalisch-Technische Bundesanstalt, concerning the beta-decays of Ag108, Ba133, Cs137, Eu152 and Eu154, Kr85, Ra226, and Sr90 were presented.

35 citations

Journal ArticleDOI
TL;DR: The most stable activity measurements of beta-decaying sources set an upper limit of 0.003-0.007% to the amplitude of annual oscillations in the decay rate as mentioned in this paper.
Abstract: Claims that proximity to the Sun causes variations of decay constants at the permille level have been investigated for beta-minus decaying nuclides. Repeated activity measurements of H-3, C-14, Co-60, Kr-85, Sr-90, Sb-124, Cs-134, Cs-137, and Eu-154 sources were performed over periods of 259 d up to 5 decades at various nuclear metrology institutes. Residuals from the exponential decay curves were inspected for annual oscillations. Systematic deviations from a purely exponential decay curve differ in amplitude and phase from one data set to another and appear attributable to instabilities in the instrumentation and measurement conditions. Oscillations in phase with Earth's orbital distance to the Sun could not be observed within 10(-4)-10(-5) range precision. The most stable activity measurements of beta-decaying sources set an upper limit of 0.003%-0.007% to the amplitude of annual oscillations in the decay rate. There are no apparent indications for systematic oscillations at a level of weeks or months.

32 citations


Cites background from "Concerning the time dependence of t..."

  • ...Parkhomov [7] and Jenkins et al [6] collected additional experimental evidence of time-dependent decay rates for β− emitters 3H, 36Cl, 56Mn, 60Co, 85Kr, 90Sr, 133Ba, 137Cs, and 239Pu as well as for β+ and electron capture decaying nuclides....

    [...]

  • ...Since it was considered less likely that α decay was affected by (mildly varying) external conditions, it was argued by Jenkins et al [6] and Parkhomov [7] that the oscillations in the 226Ra decay rates could be caused by solar influences on the β− emitters in the decay chain....

    [...]

References
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TL;DR: This paper studies the reliability and efficiency of detection with the most commonly used technique, the periodogram, in the case where the observation times are unevenly spaced to retain the simple statistical behavior of the evenly spaced case.
Abstract: Detection of a periodic signal hidden in noise is frequently a goal in astronomical data analysis This paper does not introduce a new detection technique, but instead studies the reliability and efficiency of detection with the most commonly used technique, the periodogram, in the case where the observation times are unevenly spaced This choice was made because, of the methods in current use, it appears to have the simplest statistical behavior A modification of the classical definition of the periodogram is necessary in order to retain the simple statistical behavior of the evenly spaced case With this modification, periodogram analysis and least-squares fitting of sine waves to the data are exactly equivalent Certain difficulties with the use of the periodogram are less important than commonly believed in the case of detection of strictly periodic signals In addition, the standard method for mitigating these difficulties (tapering) can be used just as well if the sampling is uneven An analysis of the statistical significance of signal detections is presented, with examples

6,761 citations

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N. R. Lomb1
TL;DR: In this article, the statistical properties of least-squares frequency analysis of unequally spaced data are examined and it is shown that the reduction in the sum of squares at a particular frequency is a X22 variable.
Abstract: The statistical properties of least-squares frequency analysis of unequally spaced data are examined. It is shown that, in the least-squares spectrum of gaussian noise, the reduction in the sum of squares at a particular frequency is aX22 variable. The reductions at different frequencies are not independent, as there is a correlation between the height of the spectrum at any two frequencies,f1 andf2, which is equal to the mean height of the spectrum due to a sinusoidal signal of frequencyf1, at the frequencyf2. These correlations reduce the distortion in the spectrum of a signal affected by noise. Some numerical illustrations of the properties of least-squares frequency spectra are also given.

4,950 citations

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TL;DR: An analysis of the free radical decay as a function of time and temperature shows the contribution of at least three types of radicals, whose half-lifes, radiochemical yields and activation energies are given.

1,039 citations

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J. P. Cravens1, K. Abe2, T. Iida2, K. Ishihara2  +147 moreInstitutions (34)
TL;DR: The results of the second phase of the Super-Kamiokande solar neutrino measurement are presented and compared to the first phase in this paper, showing no evidence of systematic tendencies between the first and second phases.
Abstract: The results of the second phase of the Super-Kamiokande solar neutrino measurement are presented and compared to the first phase. The solar neutrino flux spectrum and time variation as well as oscillation results are statistically consistent with the first phase and do not show spectral distortion. The time-dependent flux measurement of the combined first and second phases coincides with the full period of solar cycle 23 and shows no correlation with solar activity. The measured {sup 8}B total flux is (2.38{+-}0.05(stat.){sub -0.15}{sup +0.16}(sys.))x10{sup 6} cm{sup -2} s{sup -1} and the day-night difference is found to be (-6.3{+-}4.2(stat.){+-}3.7(sys.))%. There is no evidence of systematic tendencies between the first and second phases.

439 citations

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TL;DR: The results of the Troitsk ν -mass experiment on the search for the neutrino rest mass in the tritium beta-decay are presented in this article.

295 citations

Frequently Asked Questions (9)
Q1. What are the contributions in "Concerning the time dependence of the decay rate of 137 cs" ?

In this paper, the authors present new data for 133Ba and 137Cs, which were measured on the same detector system for the same time period, for which no annual oscillatory behavior was observed. 

This result, in addition to the results of decay experiments listed in Table 1, indicates that the failure to observe the annual ( or other ) periodicity in one isotope does not exclude that possibility in others. In light of Table 1, the authors can state in general that their studies to date suggest the following: ( a ) not all nuclides exhibit variability in decay constants ; ( b ) among nuclides that do exhibit this variability, the patterns of variability ( e. g., amplitude and phase of any oscillation ) are not all the same ; and ( c ) for nuclides that do exhibit variability, the patterns themselves may vary over time. 

The authors have also analyzed the PTB measurements in terms of ‘‘phasegrams,’’ which are analogous to spectrograms, displaying the power as a function of time and phase for an assumed annual oscillation. 

One of the significant factors leading to the selection of ionization chambers in these types of measurements is their inherent stability with respect to systematic and environmental effects. 

The rod was placed in the neutron irradiator for 5 min, activated, and then was placed in the counting bed and counted for fifteen minutes. 

The 137Cs standard set referenced above, which was used to determine system stability and calibration, consisted of nineindividual sources of 0:5 mCi each. 

Over a six month period of initial set-up and calibration, as reported in Cohn et al. (1969), the standard deviation of the 137Cs counts was 0.54%, implying good stability, and the background over the same period was 2:32 10470:56% counts/min over a 2:5 MeV spectrum window. 

Based on the care and thorough effort in the design, construction and calibration of the counting system in the Ellis experiment, aimed at reducing possible background and systematic variations, it seems probable that the observed differences in the fluctuations in the measured decay rates are intrinsic to the 56Mn and 137Cs decays themselves. 

This counting system was utilized in conjunction with a broad beam neutron irradiator (Cohn et al., 1972), for the in vivo NAA experiments described in Ellis (1990), as mentioned above.