166 research outputs found

    Spectroscopy of 35^{35}P using the one-proton knockout reaction

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    The structure of 35^{35}P was studied with a one-proton knockout reaction at88~MeV/u from a 36^{36}S projectile beam at NSCL. The γ\gamma rays from thedepopulation of excited states in 35^{35}P were detected with GRETINA, whilethe 35^{35}P nuclei were identified event-by-event in the focal plane of theS800 spectrograph. The level scheme of 35^{35}P was deduced up to 7.5 MeV usingγ−γ\gamma-\gamma coincidences. The observed levels were attributed to protonremovals from the sdsd-shell and also from the deeply-bound p_1/2p\_{1/2} orbital.The orbital angular momentum of each state was derived from the comparisonbetween experimental and calculated shapes of individual (γ\gamma-gated)parallel momentum distributions. Despite the use of different reactions andtheir associate models, spectroscopic factors, C2SC^2S, derived from the36^{36}S (−1p)(-1p) knockout reaction agree with those obtained earlier from36^{36}S(dd,\nuc{3}{He}) transfer, if a reduction factor R_sR\_s, as deducedfrom inclusive one-nucleon removal cross sections, is applied to the knockout transitions.In addition to the expected proton-hole configurations, other states were observedwith individual cross sections of the order of 0.5~mb. Based on their shiftedparallel momentum distributions, their decay modes to negative parity states,their high excitation energy (around 4.7~MeV) and the fact that they were notobserved in the (dd,\nuc{3}{He}) reaction, we propose that they may resultfrom a two-step mechanism or a nucleon-exchange reaction with subsequent neutronevaporation. Regardless of the mechanism, that could not yet be clarified, thesestates likely correspond to neutron core excitations in \nuc{35}{P}. Thisnewly-identified pathway, although weak, offers the possibility to selectivelypopulate certain intruder configurations that are otherwise hard to produceand identify.Comment: 5 figures, 1 table, accepted for publication in Physical Review

    Development of the (d,n) proton-transfer reaction in inverse kinematics for structure studies

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    Transfer reactions have provided exciting opportunities to study the structure of exotic nuclei and are often used to inform studies relating to nucleosynthesis and applications. In order to benefit from these reactions and their application to rare ion beams (RIBs) it is necessary to develop the tools and techniques to perform and analyze the data from reactions performed in inverse kinematics, that is with targets of light nuclei and heavier beams. We are continuing to expand the transfer reaction toolbox in preparation for the next generation of facilities, such as the Facility for Rare Ion Beams (FRIB), which is scheduled for completion in 2022. An important step in this process is to perform the (d,n) reaction in inverse kinematics, with analyses that include Q-value spectra and differential cross sections. In this way, proton-transfer reactions can be placed on the same level as the more commonly used neutron-transfer reactions, such as (d,p), (9Be,8Be), and (13C,12C). Here we present an overview of the techniques used in (d,p) and (d,n), and some recent data from (d,n) reactions in inverse kinematics using stable beams of 12C and 16O.Comment: 9 pages, 4 figures, presented at the XXXV Mazurian Lakes Conference on Physics, Piaski, Polan

    New γ\gamma-ray Transitions Observed in 19^{19}Ne with Implications for the 15^{15}O(α\alpha,γ\gamma)19^{19}Ne Reaction Rate

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    The 15^{15}O(α\alpha,γ\gamma)19^{19}Ne reaction is responsible for breakout from the hot CNO cycle in Type I x-ray bursts. Understanding the properties of resonances between Ex=4E_x = 4 and 5 MeV in 19^{19}Ne is crucial in the calculation of this reaction rate. The spins and parities of these states are well known, with the exception of the 4.14- and 4.20-MeV states, which have adopted spin-parities of 9/2−^- and 7/2−^-, respectively. Gamma-ray transitions from these states were studied using triton-γ\gamma-γ\gamma coincidences from the 19^{19}F(3^{3}He,tγt\gamma)19^{19}Ne reaction measured with GODDESS (Gammasphere ORRUBA Dual Detectors for Experimental Structure Studies) at Argonne National Laboratory. The observed transitions from the 4.14- and 4.20-MeV states provide strong evidence that the JπJ^\pi values are actually 7/2−^- and 9/2−^-, respectively. These assignments are consistent with the values in the 19^{19}F mirror nucleus and in contrast to previously accepted assignments

    Key 19^{19}Ne states identified affecting γ\gamma-ray emission from 18^{18}F in novae

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    Detection of nuclear-decay γ\gamma rays provides a sensitive thermometer of nova nucleosynthesis. The most intense γ\gamma-ray flux is thought to be annihilation radiation from the β+\beta^+ decay of 18^{18}F, which is destroyed prior to decay by the 18^{18}F(pp,α\alpha)15^{15}O reaction. Estimates of 18^{18}F production had been uncertain, however, because key near-threshold levels in the compound nucleus, 19^{19}Ne, had yet to be identified. This Letter reports the first measurement of the 19^{19}F(3^{3}He,tγt\gamma)19^{19}Ne reaction, in which the placement of two long-sought 3/2+^+ levels is suggested via triton-γ\gamma-γ\gamma coincidences. The precise determination of their resonance energies reduces the upper limit of the rate by a factor of 1.5−171.5-17 at nova temperatures and reduces the average uncertainty on the nova detection probability by a factor of 2.1.Comment: 6 pages, 4 figure

    Spectroscopy of 28^{28}Na: shell evolution toward the drip line

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    Excited states in 28^{28}Na have been studied using the β\beta-decay of implanted 28^{28}Ne ions at GANIL/LISE as well as the in-beam γ\gamma-ray spectroscopy at the NSCL/S800 facility. New states of positive (Jπ^{\pi}=3,4+^+) and negative (Jπ^{\pi}=1-5−^-) parity are proposed. The former arise from the coupling between 0d_5/2\_{5/2} protons and a 0d_3/2\_{3/2} neutron, while the latter are due to couplings with 1p_3/2\_{3/2} or 0f_7/2\_{7/2} neutrons. While the relative energies between the Jπ^{\pi}=1-4+^+ states are well reproduced with the USDA interaction in the N=17 isotones, a progressive shift in the ground state binding energy (by about 500 keV) is observed between 26^{26}F and 30^{30}Al. This points to a possible change in the proton-neutron 0d_5/2\_{5/2}-0d_3/2\_{3/2} effective interaction when moving from stability to the drip line. The presence of Jπ^{\pi}=1-4−^- negative parity states around 1.5 MeV as well as of a candidate for a Jπ^{\pi}=5−^- state around 2.5 MeV give further support to the collapse of the N=20 gap and to the inversion between the 0f_7/2\_{7/2} and 1p_3/2\_{3/2} levels below Z=12. These features are discussed in the framework of Shell Model and EDF calculations, leading to predicted negative parity states in the low energy spectra of the 26^{26}F and 25^{25}O nuclei.Comment: Exp\'erience GANIL/LISE et NSCL/S80

    Thrombin-induced CCN2 expression as a target for anti-fibrotic therapy in scleroderma

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    Scleroderma (systemic sclerosis, SSc) is a fibrotic disease for which there is no therapy. CCN2 (connective tissue growth factor, CTGF) is a marker and mediator of fibrosis. Previously, it has been shown that thrombin induces CCN2 expression in fibroblasts. In a recent fascinating report, Bogatkevich et al. (Arthritis Rheum 60:3455–3464, 2009) show that dabigatran, an inhibitor of thrombin action, blocks the overexpression of CCN2 by scleroderma fibroblasts and reverses the contractile phenotype of these cells. These results strongly suggest that dabigatran may be a potential antifibrotic drug for the treatment of fibrosing diseases such as scleroderma

    Conformation and dynamics of human urotensin II and urotensin related peptide in aqueous solution

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    Conformation and dynamics of the vasoconstrictive peptides human urotensin II (UII) and urotensin related peptide (URP) have been investigated by both unrestrained and enhanced-sampling molecular-dynamics (MD) simulations and NMR spectroscopy. These peptides are natural ligands of the G-protein coupled urotensin II receptor (UTR) and have been linked to mammalian pathophysiology. UII and URP cannot be characterized by a single structure but exist as an equilibrium of two main classes of ring conformations, <i>open</i> and <i>folded</i>, with rapidly interchanging subtypes. The <i>open</i> states are characterized by turns of various types centered at K<sup>8</sup>Y<sup>9</sup> or F<sup>6</sup>W<sup>7</sup> predominantly with no or only sparsely populated transannular hydrogen bonds. The <i>folded</i> conformations show multiple turns stabilized by highly populated transannular hydrogen bonds comprising centers F<sup>6</sup>W<sup>7</sup>K<sup>8</sup> or W<sup>7</sup>K<sup>8</sup>Y<sup>9</sup>. Some of these conformations have not been characterized previously. The equilibrium populations that are experimentally difficult to access were estimated by replica-exchange MD simulations and validated by comparison of experimental NMR data with chemical shifts calculated with density-functional theory. UII exhibits approximately 72% <i>open</i>:28% <i>folded</i> conformations in aqueous solution. URP shows very similar ring conformations as UII but differs in an <i>open:folded</i> equilibrium shifted further toward <i>open</i> conformations (86:14) possibly arising from the absence of folded N-terminal tail-ring interaction. The results suggest that the different biological effects of UII and URP are not caused by differences in ring conformations but rather by different interactions with UTR
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