It is inferred that magnesian non-porphyritic chondrules in the CB (Bencubbin-type) carbonaceous chondrites formed in an impact generated plume of gas and melt at 4562.49 ± 0.21 Ma (Bollard et al., 2015) and could be suitable for the absolute age normalization of relative chronometers. Here xenon isotopic compositions of neutron irradiated chondrules from the CB chondrites Gujba and Hammadah al Hamra (HH) 237 have been analyzed in an attempt to determine closure time of their I-Xe isotope systematics. One of the HH 237 chondrules, #1, yielded a well-defined I-Xe isochron that corresponds to a closure time of 0.29 ± 0.16 Ma after the Shallowater aubrite standard. Release profiles and diffusion properties of radiogenic Xe and Xe, extracted from this chondrule by step-wise pyrolysis, indicate presence of two iodine host phases with distinct activation energies of 73 and 120 kcal/mol. In spite of the activation energy differences, the I-Xe isotope systematics of these two phases closed simultaneously, suggesting rapid heating and cooling (possibly quenching) of the CB chondrules. The release profiles of U-fission Xe and I-derived Xe correlate in the high temperature host phase supporting simultaneous closure of I-Xe and Pb-Pb systematics. The absolute I-Xe age of Shallowater standard is derived from the observed correlation between I-Xe and Pb-Pb ages in a number of samples. It is re-evaluated here using Pb-Pb ages adjusted for an updated U/U ratio of 137.794 and meteorite specific U-isotope ratios. With the addition of the new data for HH 237 chondrule #1, the re-evaluated absolute I-Xe age of Shallowater is 4562.4 ± 0.2 Ma. The absolute I-Xe age of the HH 237 chondrule #1 is 4562.1 ± 0.3 Ma, in good agreement with U-corrected Pb-Pb ages of the Gujba chondrules (Bollard et al., 2015) and HH 237 silicates (Krot et al., 2005). All I-Xe data used here, and in previous estimates of the absolute age of Shallowater, are calculated using 15.7 ± 0.6 Ma value for I half-life. The slopes of I-Xe - Pb-Pb correlation lines plotted for different sets of samples for Shallowater normalization are always ≤1. Assuming uranium half-life values are correct; this restricts the half-life of I to ≤15.7 Ma.
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http://dx.doi.org/10.1016/j.gca.2016.01.012 | DOI Listing |
Appl Radiat Isot
October 2024
Department of Physics, Kyungpook National University, Daegu, 41566, South Korea.
For the first time, charge distribution studies have been carried out in the epi-cadmium neutron induced fission of U by measuring the fractional cumulative yields (FCY) and independent yields (IY) of various fission products. An off-line γ-ray spectrometric technique was used for the measurements. The average energy of the epi-cadmium neutron spectrum is 1.
View Article and Find Full Text PDFAppl Radiat Isot
July 2024
Department of Physics, Kyungpook National University, Daegu, 41566, South Korea.
Studies on charge distribution have been carried out in the epi-cadmium neutron induced fission of Pu for the first time. Experimentally fractional cumulative yields (FCY) and independent yields (IY) of various fission products have been measured by using an off-line γ-ray spectrometric technique. From the FCY values, the charge distribution parameters such as the isobaric width parameter (σ), most probable charge (Z) and the charge polarization (ΔΖ) as a function of fragment mass were obtained.
View Article and Find Full Text PDFPhys Rev Lett
August 2021
School of Physics, University of New South Wales, Sydney 2052, Australia.
We calculate the cross sections of atomic ionization by absorption of scalar particles in the energy range from a few eV to 100 keV. We consider both nonrelativistic particles (dark matter candidates) and relativistic particles that may be produced inside the Sun. We provide numerical results for atoms relevant for direct dark matter searches (O, Na, Ar, Ca, Ge, I, Xe, W and Tl).
View Article and Find Full Text PDFJ Chem Theory Comput
October 2019
Center for Computational Materials, Oden Institute for Computational Engineering and Sciences , The University of Texas at Austin, Austin , Texas 78712 , United States.
Using an implementation based on real-space wave functions, we perform GW calculations of the HOMO and LUMO energies of molecules and atoms in the GW100 set. Our main conclusions are as follows: (1) Different implementations of the GW approximation show much better agreements for HOMO (highest occupied molecular orbital) energies than for LUMO (lowest unoccupied molecular orbital) energies. The mean absolute differences between the results calculated with different pseudopotential codes range from 100 to 200 meV.
View Article and Find Full Text PDFJ Appl Physiol (1985)
December 2019
Institute for Exercise and Environmental Medicine, Texas Health Presbyterian Dallas, Dallas, Texas.
This study aimed to quantify the sedative effects, detection rates, and cardiovascular responses to xenon. On 3 occasions, participants breathed xenon (FXe 30% for 20 min; FXe 50% for 5 min; FXe 70% for 2 min) in a nonblinded design. Sedation was monitored by a board-certified anesthesiologist.
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