Identification of new transitions and mass assignments of levels in<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mmultiscripts><mml:mi>Pr</mml:mi><mml:mprescripts /><mml:none /><mml:mrow><mml:mn>143</mml:mn><mml:mo>–</mml:mo><mml:mn>153</mml:mn></mml:mrow></mml:mmultiscripts></mml:mrow></mml:math>

Wang, E. H.; Lemasson, A.; Hamilton, J. H.; Ramayya, A. V.; Hwang, J. K.; Eldridge, J. M.; Navin, A.; Rejmund, M.; Bhattacharyya, S.; Liu, S. H.; Brewer, N. T.; Luo, Y. X.; Rasmussen, J. O.; Liu, H. L.; Zhou, Haibiao; Liu, Y. X.; Li, H. J.; Sun, Y.; Fang, Xu; Zhu, S. J.; Ter-Akopian, G. M.; Oganessian, Yu. Ts.; Caamaño, M.; Clément, E.; Delaune, O.; Farget, F.; Jacquot, B.

doi:10.1103/physrevc.92.034317

Cited by 14 publications

(4 citation statements)

References 41 publications

(68 reference statements)

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“…Although not directly comparable with the estimated rates in Ref. 79 for the different targets, there is an important discrepancy between them. As shown in the excitation functions plotted in Ref.…”

Section: Telluriumcontrasting

confidence: 66%

“…In addition, as presented in Ref. 79, flux-averaged cross-sections for neutron activation in natural tellurium were measured by irradiating at LANSCE TeO 2 powder with the neutron beam containing neutrons of kinetic energies up to ∼800 MeV and having an energy spectrum similar to that of cosmic-ray neutrons at sea-level; gamma ray analysis was performed in Berkeley Low Background Facility. The cross sections obtained for 110m Ag and 60 Co, the two isotopes identified as the most relevant ones Table 4.…”

Section: Telluriummentioning

confidence: 99%

“…Production rates (in µBq kg −1 ) at sea level presented in Ref 79. for isotopes induced in TeO 2 combining measured cross sections at different energies and in Ref 81.…”

mentioning

confidence: 99%

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Cosmogenic activation of materials

Cebrián¹

2013

AIP Conference Proceedings

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Experiments looking for rare events like the direct detection of dark matter particles, neutrino interactions or the nuclear double beta decay are operated deep underground to suppress the effect of cosmic rays. But the production of radioactive isotopes in materials due to previous exposure to cosmic rays is an hazard when ultra-low background conditions are required. In this context, the generation of long-lived products by cosmic nucleons has been studied for many detector media and for other materials commonly used. Here, the main results obtained on the quantification of activation yields on the Earth's surface will be summarized, considering both measurements and calculations following different approaches. The isotope production cross sections and the cosmic ray spectrum are the two main ingredients when calculating this cosmogenic activation; the different alternatives for implementing them will be discussed. Activation that can take place deep underground mainly due to cosmic muons will be briefly commented too. Presently, the experimental results for the cosmogenic production of radioisotopes are scarce and discrepancies between different calculations are important in many cases, but the increasing interest on this background source which is becoming more and more relevant can help to change this situation.

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Section: Telluriumcontrasting

confidence: 66%

Section: Telluriummentioning

confidence: 99%

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Cosmogenic activation of materials

Cebrián¹

2013

AIP Conference Proceedings

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“…The use of the VAMOS++ spectrometer with the EXOGAM [26] large γ-ray array allowed the first assignment of prompt γ rays in several members of the isotopic chains of Ag [27], Rh [28], Cd and In [24,25]. The combination of prompt γ-ray data-sets obtained in coincidence with the VA-MOS++ magnetic spectrometers with those obtained using high fold γ-ray techniques using Gammasphere allowed extended studies in the isotopic chains of Y [29], Pr [30] and Pm [31], which illustrate the complementarity of both methods. Furthermore, the experiments with VAMOS++ and EXOGAM using the Recoil Distance Doppler-Shift Method (RDDS) [32] allowed the measurement of lifetimes of excited states in isotopes of Zr [33], Y and Nb [34] and Tc and Rh [35].…”

Section: Introductionmentioning

confidence: 99%

Advancements of $$\gamma $$-ray spectroscopy of isotopically identified fission fragments with AGATA and VAMOS++

et al. 2023

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γ-ray spectroscopy of fission fragments is a powerful method for studies of nuclear structure properties. Recent results on the spectroscopy of fission fragments, using the combination of the AGATA γ-ray tracking array and the VAMOS++ large acceptance magnetic spectrometer at GANIL, are reported. A comparison of the performance of the large germanium detector arrays EXOGAM and AGATA illustrates the advances in γ-ray spectroscopy of fission fragments. Selected results are highlighted for prompt γ-ray spectroscopy studies, measurements of short lifetimes of excited states with the Recoil Distance Doppler-Shift method, using both AGATA and VAMOS++ and prompt-delayed γ-ray spectroscopy studies using AGATA, VAMOS++ and EXOGAM.

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Nuclear Data Sheets for A=153

Nica

2020

Nuclear Data Sheets

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Identification of new transitions and mass assignments of levels inPr143–153

Cited by 14 publications

References 41 publications

Cosmogenic activation of materials

Cosmogenic activation of materials

Advancements of $$\gamma $$-ray spectroscopy of isotopically identified fission fragments with AGATA and VAMOS++

Nuclear Data Sheets for A=153

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