5,008 research outputs found

    Stellar 36,38^{36,38}Ar(n,γ)37,39(n,\gamma)^{37,39}Ar reactions and their effect on light neutron-rich nuclide synthesis

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    The 36^{36}Ar(n,γ)37(n,\gamma)^{37}Ar (t1/2t_{1/2} = 35 d) and 38^{38}Ar(n,γ)39(n,\gamma)^{39}Ar (269 y) reactions were studied for the first time with a quasi-Maxwellian (kT47kT \sim 47 keV) neutron flux for Maxwellian Average Cross Section (MACS) measurements at stellar energies. Gas samples were irradiated at the high-intensity Soreq applied research accelerator facility-liquid-lithium target neutron source and the 37^{37}Ar/36^{36}Ar and 39^{39}Ar/38^{38}Ar ratios in the activated samples were determined by accelerator mass spectrometry at the ATLAS facility (Argonne National Laboratory). The 37^{37}Ar activity was also measured by low-level counting at the University of Bern. Experimental MACS of 36^{36}Ar and 38^{38}Ar, corrected to the standard 30 keV thermal energy, are 1.9(3) mb and 1.3(2) mb, respectively, differing from the theoretical and evaluated values published to date by up to an order of magnitude. The neutron capture cross sections of 36,38^{36,38}Ar are relevant to the stellar nucleosynthesis of light neutron-rich nuclides; the two experimental values are shown to affect the calculated mass fraction of nuclides in the region A=36-48 during the weak ss-process. The new production cross sections have implications also for the use of 37^{37}Ar and 39^{39}Ar as environmental tracers in the atmosphere and hydrosphere.Comment: 18 pages + Supp. Mat. (13 pages) Accepted for publication in Phys. Rev. Let

    Probing the single-particle character of rotational states in 19^{19}F using a short-lived isomeric beam

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    A beam containing a substantial component of both the Jπ=5+J^{\pi}=5^+, T1/2=162T_{1/2}=162 ns isomeric state of 18^{18}F and its 1+1^+, 109.77-min ground state has been utilized to study members of the ground-state rotational band in 19^{19}F through the neutron transfer reaction (d(d,p)p) in inverse kinematics. The resulting spectroscopic strengths confirm the single-particle nature of the 13/2+^+ band-terminating state. The agreement between shell-model calculations, using an interaction constructed within the sdsd shell, and our experimental results reinforces the idea of a single-particle/collective duality in the descriptions of the structure of atomic nuclei

    Independent measurement of the Hoyle state β\beta feeding from 12B using Gammasphere

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    Using an array of high-purity Compton-suppressed germanium detectors, we performed an independent measurement of the β\beta-decay branching ratio from 12B^{12}\mathrm{B} to the second-excited (Hoyle) state in 12C^{12}\mathrm{C}. Our result is 0.64(11)%0.64(11)\%, which is a factor 2\sim 2 smaller than the previously established literature value, but is in agreement with another recent measurement. This could indicate that the Hoyle state is more clustered than previously believed. The angular correlation of the Hoyle state γ\gamma cascade has also been measured for the first time. It is consistent with theoretical predictions

    Fusion reactions of 58,64Ni+124Sn

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    International audience; In order to better understand the influence of transfer in sub-barrier nuclear reactions, cross sections for the system ^58,64Ni+^124Sn have been measured down to 0.5-1 mub and compared to detailed coupledchannel calculations. In agreement with a phenomenological Q-value systematics, calculations show the importance of including the coupling to the transfer channel for these heavy systems. No clear evidence of fusion hindrance is observed, probably due to the fact that the cross sections measured in this experiment are not low enough for the appearance of that phenomenon

    Operational experience with the GEM detector assembly lines for the CMS forward muon upgrade

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    The CMS Collaboration has been developing large-area triple-gas electron multiplier (GEM) detectors to be installed in the muon Endcap regions of the CMS experiment in 2019 to maintain forward muon trigger and tracking performance at the High-Luminosity upgrade of the Large Hadron Collider (LHC); 10 preproduction detectors were built at CERN to commission the first assembly line and the quality controls (QCs). These were installed in the CMS detector in early 2017 and participated in the 2017 LHC run. The collaboration has prepared several additional assembly and QC lines for distributed mass production of 160 GEM detectors at various sites worldwide. In 2017, these additional production sites have optimized construction techniques and QC procedures and validated them against common specifications by constructing additional preproduction detectors. Using the specific experience from one production site as an example, we discuss how the QCs make use of independent hardware and trained personnel to ensure fast and reliable production. Preliminary results on the construction status of CMS GEM detectors are presented with details of the assembly sites involvement
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