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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: An experiment designed to address the question of whether a flux of reactor-generated electron antineutrinos can alter the rates of weak nuclear interaction induced decays of 54Mn, 22Na, and 60Co is conducted.

7 citations

Journal ArticleDOI
TL;DR: In this article, the authors analyzed data from eight HPGe gamma ray detectors at the NC State University PULSTAR Reactor for evidence of periodic variations, with particular attention to annual variations.
Abstract: Measurements of Ra-226 activity from eight HPGe gamma ray detectors at the NC State University PULSTAR Reactor were analyzed for evidence of periodic variations, with particular attention to annual variations. All measurements were made using the same reference source, and data sets were of varying length taken over the time period from September 1996 through August 2014. Clear evidence of annual variations was observed in data from four of the detectors. Short time periodograms from the data sets suggest temporal variability of both the amplitude and frequency of these variations. The annual variations in two of the data sets show peak values near the first of February, while surprisingly, the annual variations in the other two are roughly out of phase with the first two. Three of the four detectors exhibited annual variations over approximately the same time period. A joint statistic constructed by combining spectra from these three shows peaks approximating the frequencies of solar r-mode oscillations with $ u_R = 11.74$ cpy, $m=1$, and $l=3,5,6.$ The fact that similar variations were not present in all detectors covering similar time periods rules out variations in activity as the cause, and points to differing sensitivities to unspecified environmental parameters instead. In addition to seasonal variations, the modulation of environmental parameters by solar processes remains a possible explanation of periodogram features, but without requiring new physics.

6 citations

Journal ArticleDOI
TL;DR: In this paper, the decay rate of 60Co, 44Ti and 137Cs sources was measured by two independent NaI(Tl) detector setups, and no correlation between the two strongest observed Solar flares in September 2017 and the decay rates was found.

6 citations

23 Apr 2022
TL;DR: In this article , a model for mixing in decay configuration was proposed based on the zero threshold energy for neutrino absorption in beta emitters, and the model for con-guration mixing between two distinct beta disintegration modes β ν -disintegration (electron from neutrinos interaction) and the β − − − disintegration was proposed.
Abstract: Background: Decay constants of unstable nuclei and particles are quantum constants. Recent controversy on the existence (versus non-existence) of variability in the observation of decay rate can be settled by considering mixing in decay configuration. Purpose: Variability in decay rate was investigated based on the available information of beta decay rate data, solar neutrino flux, and energy distribution. Method: Full systematic analysis of the oscillatory behavior was carried out. Based on the zero threshold energy for neutrino absorption in beta emitters, a model for configuration mixing between two distinct beta disintegration modes β ν -disintegration (electron from neutrino interaction) and the β − -disintegration (electron from natural decay) was proposed. Results: The phenomenon of variability in beta decay rate was related to the possible exothermic neutrino absorption by unstable nuclei which, in principle, should include the whole range of flux energies involving flux with energy below the 71 Ga threshold at 0.23 MeV. These two disintegration modes occur independently and model for their apparent mixing rate was proposed. Conclusions: The configuration mixing between the two modes cause depletion of radioactive nuclei which is subject to change with seasonal solar neutrino variability. Ability to detect this variability was found to be dependent on the Q-value of the β ν disintegration and detection instrument setup. Value of neutrino cross section weighted by the ratio between β ν and β − detection efficiencies was found to be in the range 10 − 44 to 10 − 36 cm 2 . For experiments that uses the end point to determine the neutrino mass, interference due to mixing should be taken into account.

5 citations

Journal ArticleDOI
TL;DR: In this paper, the generalized Lombargle periodogram was applied to the decay rate of radionuclei at the Bronson Methodist Hospital to find a sinusoidal modulation at any frequency, including annual modulation or at frequencies associated with solar rotation.
Abstract: We apply the generalized Lomb–Scargle periodogram to the $${^{123}\text {I}}$$ and $${^{99\mathrm{m}}\text {Tc}}$$ decay rate measurements based on data taken at the Bronson Methodist Hospital. The aim of this exercise was to carry out an independent search for sinusoidal modulation for these radionuclei (to complement the analysis in Borrello et al.) at frequencies for which other radionuclei have shown periodicities. We do not find such a modulation at any frequencies, including annual modulation or at frequencies associated with solar rotation. Our analysis codes and datasets have been made publicly available.

4 citations

References
More filters
Journal ArticleDOI
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

Journal ArticleDOI
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

Journal ArticleDOI
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

Journal ArticleDOI
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

Journal ArticleDOI
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.