Sahoo, R. N.; Paul, M.; Köster, U.; Scott, R.; Tessler, M.; Zylstra, A.; Avila, M. L.; Dickerson, C.; Jayatissa, H.; Kohen, M.S.; et al
(, EPJ Web of Conferences)
Mattoon, C.M.; Vogt, R.; Escher, J.; Thompson, I.
(Ed.)
The cross-section of the thermal neutron capture41Ar(n,γ)42Ar(t1/2=32.9 y) reaction was measured by irradiating a40Ar sample at the high-flux reactor of Institut Laue-Langevin (ILL) Grenoble, France. The signature of the two-neutron capture has been observed by measuring the growth curve and identifying the 1524.6 keV γ-lines of the shorter-lived42K(12.4 h) β−daughter of42Ar. Our preliminary value of the41Ar(n,γ)42Ar thermal cross section is 240(80) mb at 25.3 meV. For the first time, direct counting of42Ar was performed using the ultra-high sensitivity technique of noble gas accelerator mass spectrometry (NOGAMS) at Argonne National Laboratory, USA.
Abstract We report40Ar‐39Ar step‐heating ages of Paleocene‐Eocene (P‐E) boundary impact spherules from Atlantic Margin coastal plain and open ocean sites. We test the hypothesis that the P‐E spherules are reworked from an earlier event (e.g., K‐Pg impact at ~66 Ma), which predicts a cooling age discordant from their depositional age of 55.93 ± 0.05 Ma at the P‐E boundary. Isochrons from the step‐heating analysis yield40Ar‐36Ar intercepts in excess of the modern in most cases, indicating that the spherules have excess radiogenic Ar (40Ar*), typical of impact glasses incompletely degassed before solidification. The weighted mean of the isochron‐corrected plateau age is 54.2 ± 2.5 Ma (1σ), and their isochron age is 55.4 ± 4.0 Ma, both indistinguishable from their P‐E depositional age, not supporting the K‐Pg reworking hypothesis. This is consistent with all other stratigraphic and geochemical evidence for an impact at the P‐E boundary and ejecta distribution by air fall.
Yan, Pei-Gen; Babb, James F
(, The Astrophysical Journal)
Abstract We calculate cross sections for fine-structure transitions of Ne+, Ar+, Ne2+, and Ar2+in collisions with atomic hydrogen by using quantum-mechanical methods. Relaxation rate coefficients are calculated for temperatures up to 10,000 K. The temperature-dependent critical densities for the relaxation of Ne+, Ar+, Ne2+, and Ar2+in collisions with H have been determined and compared to the critical densities for collisions with electrons. The present calculations will be useful for studies utilizing the infrared lines [Neii] 12.8, [Neiii] 15.6, [Neiii] 36.0, [Arii] 6.99, [Ariii] 8.99, and [Ariii] 21.8μm as diagnostics of, for example, planetary nebulae and star formation.
Tauxe, Lisa; Gans, Phillip; Mankinen, Edward A
(, Magnetics Information Consortium (MagIC))
Paleomagnetic, rock magnetic, or geomagnetic data found in the MagIC data repository from a paper titled: Paleomagnetism and40Ar/39Ar ages from volcanics extruded during the Matuyama and Brunhes Chrons near McMurdo Sound, Antarctica
Abstract Deccan Traps flood basalt volcanism affected ecosystems spanning the end‐Cretaceous mass extinction, with the most significant environmental effects hypothesized to be a consequence of the largest eruptions. The Rajahmundry Traps are the farthest exposures (~1,000 km) of Deccan basalt from the putative eruptive centers in the Western Ghats and hence represent some of the largest volume Deccan eruptions. Although the three subaerial Rajahmundry lava flows have been geochemically correlated to the Wai Subgroup of the Deccan Traps, poor precision associated with previous radioisotopic age constraints has prevented detailed comparison with potential climate effects. In this study, we use new40Ar/39Ar dates, paleomagnetic and volcanological analyses, and biostratigraphic constraints for the Rajahmundry lava flows to ascertain the timing and style of their emplacement. We find that the lower and middle flows (65.92 ± 0.25 and 65.67 ± 0.08 Ma, ±1σsystematic uncertainty) were erupted within magnetochron C29r and were a part of the Ambenali Formation of the Deccan Traps. By contrast, the uppermost flow (65.27 ± 0.08 Ma) was erupted in C29n as part of the Mahabaleshwar Formation. Given these age constraints, the Rajahmundry flows were not involved in the end‐Cretaceous extinction as previously hypothesized. To determine whether the emplacement of the Rajahmundry flows could have affected global climate, we estimated their eruptive CO2release and corresponding climate change using scalings from the LOSCAR carbon cycle model. We find that the eruptive gas emissions of these flows were insufficient to directly cause multi‐degree warming; hence, a causal relationship with significant climate warming requires additional Earth system feedbacks.
Garcia, Michael O., Jicha, Brian R., Marske, Jared P., and Pietruszka, Aaron J. How old is Kīlauea Volcano (Hawai‘i)? Insights from 40 Ar/ 39 Ar dating of the 1.7-km-deep SOH-1 core. Retrieved from https://par.nsf.gov/biblio/10024818. Geology 45.1 Web. doi:10.1130/G38419.1.
Garcia, Michael O., Jicha, Brian R., Marske, Jared P., & Pietruszka, Aaron J. How old is Kīlauea Volcano (Hawai‘i)? Insights from 40 Ar/ 39 Ar dating of the 1.7-km-deep SOH-1 core. Geology, 45 (1). Retrieved from https://par.nsf.gov/biblio/10024818. https://doi.org/10.1130/G38419.1
Garcia, Michael O., Jicha, Brian R., Marske, Jared P., and Pietruszka, Aaron J.
"How old is Kīlauea Volcano (Hawai‘i)? Insights from 40 Ar/ 39 Ar dating of the 1.7-km-deep SOH-1 core". Geology 45 (1). Country unknown/Code not available. https://doi.org/10.1130/G38419.1.https://par.nsf.gov/biblio/10024818.
@article{osti_10024818,
place = {Country unknown/Code not available},
title = {How old is Kīlauea Volcano (Hawai‘i)? Insights from 40 Ar/ 39 Ar dating of the 1.7-km-deep SOH-1 core},
url = {https://par.nsf.gov/biblio/10024818},
DOI = {10.1130/G38419.1},
abstractNote = {},
journal = {Geology},
volume = {45},
number = {1},
author = {Garcia, Michael O. and Jicha, Brian R. and Marske, Jared P. and Pietruszka, Aaron J.},
}
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