Total Absorption Spectroscopy Study of (92)Rb Decay: A Major Contributor to Reactor Antineutrino Spectrum Shape.

The antineutrino spectra measured in recent experiments at reactors are inconsistent with calculations based on the conversion of integral beta spectra recorded at the ILL reactor. (92)Rb makes the dominant contribution to the reactor antineutrino spectrum in the 5-8 MeV range but its decay properties are in question. We have studied (92)Rb decay with total absorption spectroscopy. Previously unobserved beta feeding was seen in the 4.5-5.5 region and the GS to GS feeding was found to be 87.5(25)%. The impact on the reactor antineutrino spectra calculated with the summation method is shown and discussed.

Enhanced γ-Ray Emission from Neutron Unbound States Populated in ß Decay.

Total absorption spectroscopy is used to investigate the ß-decay intensity to states above the neutron separation energy followed by γ-ray emission in (87,88)Br and (94)Rb. Accurate results are obtained thanks to a careful control of systematic errors. An unexpectedly large γ intensity is observed in all three cases extending well beyond the excitation energy region where neutron penetration is hindered by low neutron energy. The γ branching as a function of excitation energy is compared to Hauser-Feshbach model calculations. For (87)Br and (88)Br the γ branching reaches 57% and 20%, respectively, and could be explained as a nuclear structure effect. Some of the states populated in the daughter can only decay through the emission of a large orbital angular momentum neutron with a strongly reduced barrier penetrability. In the case of neutron-rich (94)Rb the observed 4.5% branching is much larger than the calculations performed with standard nuclear statistical model parameters, even after proper correction for fluctuation effects on individual transition widths. The difference can be reconciled by introducing an enhancement of 1 order of magnitude in the photon strength to neutron strength ratio. An increase in the photon strength function of such magnitude for very neutron-rich nuclei, if it proves to be correct, leads to a similar increase in the (n,γ) cross section that would have an impact on r process abundance calculations.

Ultra-high resolution mass separator--application to detection of nuclear weapons tests.

A Penning trap-based purification process having a resolution of about 1 ppm is reported. In this context, we present for the first time a production method for the most complicated and crucially important nuclear weapons test signature, (133m)Xe. These pure xenon samples are required by the Comprehensive Nuclear-Test-Ban Treaty Organization to standardize and calibrate the worldwide network of xenon detectors.

Smallest known Q value of any nuclear decay: the rare beta;{-} decay of ;{115}In(9/2;{+}) --> ;{115}Sn(3/2;{+}).

The ground-state-to-ground-state Q_{beta;{-}} value of ;{115}In was determined to 497.68(17) keV using a high-precision Penning trap facility at the University of Jyväskylä, Finland. From this, a Q_{beta;{-}} value of 0.35(17) keV was obtained for the rare beta;{-} decay to the first excited state of ;{115}Sn at 497.334(22) keV. The partial half-life was determined to 4.1(6) x 10;{20} yr using ultra low-background gamma-ray spectrometry in an underground laboratory. Theoretical modeling of this 2nd-forbidden unique beta;{-} transition was also undertaken and resulted in Q_{beta;{-}} = 57_{-12};{+19} eV using the measured half-life. The discrepancy between theory and experiment could be attributed to atomic effects enhanced by the low Q value. The present study implies that this transition has the lowest Q value of any known nuclear beta decay.

Quenching of the SnSbTe cycle in the rp process.

The nuclides 104-108Sn, 106-110Sb, 108,109Te, and 111I at the expected endpoint of the astrophysical rp process have been produced in 58Ni+natNi fusion-evaporation reactions at IGISOL and their mass values were precisely measured with the JYFLTRAP Penning trap mass spectrometer. For 106Sb, 108Sb, and 110Sb these are the first direct experimental mass results obtained. The related one-proton separation energies have been derived and the value for 106Sb, Sp=424(8) keV, shows that the branching into the closed SnSbTe cycle in the astrophysical rp process is weaker than expected.

Accurate Q value for the 112Sn double-beta decay and its implication for the search of the neutrino mass.

The Q value of the ;{112}Sn double-beta decay was determined by using a Penning trap mass spectrometer. The new atomic-mass difference between ;{112}Sn and ;{112}Cd of 1919.82(16) keV is 25 times more precise than the previous value of 1919(4) keV. This result removes the possibility of enhanced resonance capture of the neutrinoless double-EC decay to the excited 0;{+} state at 1871.00(19) keV in ;{112}Cd.

QEC values of the superallowed beta emitters 34Cl and 38Km.

The superallowed beta-decay Q(EC) values of (34)Cl and (38)K(m) have been measured with an online Penning trap to be 5491.662(47) keV and 6044.223(41) keV, respectively. The new values are more precise than the previous high-precision reaction-based values but are consistent with them and establish that there are no significant systematic differences between the two types of measurements.

Mass measurements and implications for the energy of the high-spin isomer in 94Ag.

Nuclides in the vicinity of 94Ag have been studied with the Penning trap mass spectrometer JYFLTRAP at the Ion-Guide Isotope Separator On-Line. The masses of the two-proton-decay daughter 92Rh and the beta-decay daughter 94Pd of the high-spin isomer in 94Ag have been measured, and the masses of 93Pd and 94Ag have been deduced. When combined with the data from the one-proton- or two-proton-decay experiments, the results lead to contradictory mass excess values for the high-spin isomer in 94Ag, -46 370(170) or -44 970(100) keV, corresponding to excitation energies of 6960(400) or 8360(370) keV, respectively.

Evolution of the N=50 shell gap energy towards 78Ni.

Atomic masses of the neutron-rich isotopes (76-80)Zn, (78-83)Ga, (80-85)Ge, (81-87)As, and (84-89)Se have been measured with high precision using the Penning trap mass spectrometer JYFLTRAP at the IGISOL facility. The masses of (82,83)Ga, (83-85)Ge, (84-87)As, and 89Se were measured for the first time. These new data represent a major improvement in the knowledge of the masses in this neutron-rich region. Two-neutron separation energies provide evidence for the reduction of the N=50 shell gap energy towards germanium (Z=32) and a subsequent increase at gallium (Z=31). The data are compared with a number of theoretical models. An indication of the persistent rigidity of the shell gap towards nickel (Z=28) is obtained.

QEC values of the superallowed beta emitters 50Mn and 54Co.

Using a new fast cleaning procedure to prepare isomerically pure ion samples, we have measured the beta-decay Q(EC) values of the superallowed beta emitters 5(0)Mn and (54)Co to be 7634.48(7) and 8244.54(10) keV, respectively, results which differ significantly from the previously accepted values. The corrected Ft values derived from our results strongly support new isospin-symmetry-breaking corrections that lead to a higher value of the up-down quark mixing element V(ud) and improved confirmation of the unitarity of the Cabibbo-Kobayashi-Maskawa matrix.

Biological markers of alcohol consumption and effect of calcitonin in nonalcoholic men: a prospective, double-blind study.

The objective of this study was to study the ability of biological markers of alcohol consumption in differentiating subjects below weekly consumption of 400 or 600 g of absolute ethanol from those above, and to study the effect of intranasal calcitonin on alcohol drinking. A prospective 12-week double-blind study that used anonymous data collection with drinking diaries was done. The drug that was studied (calcitonin or placebo) was used during study weeks 5-8. This study was performed at the research unit of a university hospital. The subjects consisted of 59-nine men aged 26 to 57 years who considered themselves as regular but modest drinkers and were recruited by advertisements. The measurements were obtained from monthly questionnaires and daily anonymous diaries for alcohol drinking data, and biological markers of alcohol consumption (aspartate aminotransferase, alanine aminotransferase, gamma-glutamyl transpeptidase, beta hexosaminidase, and carbohydrate deficient transferrin). The results indicated intranasal calcitonin with a dose of 200 IU three times a week had no effect on alcohol use. All biological markers studied had only a modest ability to differentiate those with weekly alcohol consumption of 400 or 600 g or over from those below these limits. The areas under receiver operating characteristic (ROC) curve with the limit 400 g/week were 0.71 for aspartate aminotransferase, 0.61 for alanine aminotransferase, 0.74 for gamma-glutamyl transpeptidase, 0.68 for beta-hexosaminidase, and 0.78 for carbohydrate deficient transferrin. Respective numbers for the 600-g limit were more uniform. As evaluated by ROC analysis, carbohydrate deficient transferrin was the best biological marker to find men with weekly alcohol consumption over 400 g. Intranasal salmon calcitonin had no affect on alcohol drinking.

Low particulate type IV phosphodiesterase activity in hypothyroid rat atria.

Rats were made hypothyroid by adding propylthiouracil (PTU) to their drinking water. Some of the PTU-treated rats were given thyroid hormone injections for 5 days. Both soluble and particulate cAMP-phosphodiesterase activities of adipose and ventricular tissues were increased by 25-60% in hypothyroidism. In left atria, soluble cAMP-phosphodiesterase activity was not significantly altered in hypothyroidism, while total particulate cAMP-phosphodiesterase activity was lowered by 30%. This lowering was due to diminished isoenzyme IV activity, as studied with the isoenzyme-specific inhibitors rolipram and SK&F 94836. In conclusion, the present results show decreased particulate type IV cAMP-phosphodiesterase activity in hypothyroid rat atria. This may explain the increased responsiveness to isoproterenol in hypothyroid atria.