1. In-flight production of an isomeric beam of $^{16}$N
- Author
-
C.R. Hoffman, T.L. Tang, M. Avila, Y. Ayyad, K.W. Brown, J. Chen, K.A. Chipps, H. Jayatissa, B.P. Kay, C. Müller-Gatermann, H.J. Ong, J. Song, and G.L. Wilson
- Subjects
Nuclear Theory (nucl-th) ,Nuclear and High Energy Physics ,Physics - Instrumentation and Detectors ,Nuclear Theory ,Physics::Accelerator Physics ,FOS: Physical sciences ,Instrumentation and Detectors (physics.ins-det) ,Nuclear Experiment (nucl-ex) ,Nuclear Experiment ,Instrumentation - Abstract
An in-flight beam of $^{16}$N was produced via the single-neutron adding ($d$,$p$) reaction in inverse kinematics at the recently upgraded Argonne Tandem Linear Accelerator System (ATLAS) in-flight system. The amount of the $^{16}$N beam which resided in its excited 0.120-MeV $J^{\pi}=0^-$ isomeric state (T$_{1/2}\approx5$ $\mu$s) was determined to be 40(5)% at a reaction energy of 7.9(3) MeV/$u$, and 24(2)% at a reaction energy of 13.2(2) MeV/$u$. The isomer measurements took place at an experimental station $\approx30$ m downstream of the production target and utilized an Al beam-stopping foil and a HPGe Clover detector. Composite $^{16}$N beam rate determinations were made at the experimental station and the focal plane of the Argonne in-flight radioactive ion-beam separator (RAISOR) with Si $\Delta$E-E telescopes. A Distorted Wave Born Approximation (DWBA) approach was coupled with the known spectroscopic information on $^{16}$N in order to estimate the relative $^{16}$N isomer yields and composite $^{16}$N beam rates. In addition to the observed reaction-energy dependence of the isomer fraction, a large sensitivity to angular acceptance of the recoils was also observed., Comment: 21 pages, 7 figures
- Published
- 2022
- Full Text
- View/download PDF