Bulletin of the American Physical Society
5th Joint Meeting of the APS Division of Nuclear Physics and the Physical Society of Japan
Volume 63, Number 12
Tuesday–Saturday, October 23–27, 2018; Waikoloa, Hawaii
Session LH: Instrumentation IV |
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Chair: Michael Carpenter, Argonne National Laboratory Room: Hilton Kona 2/3 |
Saturday, October 27, 2018 9:00AM - 9:15AM |
LH.00001: Commissioning of EMMA Matthew Williams, Barry S Davids, Nicholas Esker, Kevan Hudson, Devin S Connolly, Naimat Khan, Peter Machule The Electromagnetic Mass Analyser (EMMA) is a new recoil mass spectrometer located in the ISAC-II facility at TRIUMF. EMMA is designed to separate the products of nuclear reactions from the un-reacted beam, and to disperse those products onto detectors at the focal plane in accordance with their mass/charge ratio. The absolute transport efficiency of EMMA has been mapped as a function of energy and angle in a series of in-beam and alpha-source test studies. In addition to these test studies, EMMA has also been successfully used to identify recoils produced from fusion evaporation and radiative capture reactions; the former induced by a radioactive ion beam. This work will ultimately be used to calculate the transport efficiency for arbitrary recoil distributions; thereby allowing measurements of absolute cross sections, which is of vital importance to advancing the nuclear structure and nuclear astrophysics program at TRIUMF. |
Saturday, October 27, 2018 9:15AM - 9:30AM |
LH.00002: Direct measurement of atomic number for superheavy nuclei search Kunihiro Fujita, Takao Saito, Toshitaka Niwase, Keigo Bando, Kenta Manabe, Kazuya Shirasaka, Yoshihide Suekawa, Kousuke Morita A direct measurement of the atomic number is demanded for the experiments of the superheavy nuclei synthesis such as 119th element search, since the conventional method of analyzing the alpha-decay chain have a limitation of identification for spontaneous-fission nuclei. We have developed a Bragg curve detector(BCD) employing a digital signal processing technique to improve the separation efficiency especially for low-energy superheavy ions. Although the height of Bragg peaks induced by heavy ions of less than 1.5 MeV/u are not proportional to the incident energy, the waveform analysis makes it possible to identify the nuclei having the different atomic number. The performance test of the developed detector was performed at Kyushu University Center for Accelerator and Beam Applied Science. The heavy ion beams supplied from the Tandem accelerator were scattered and injected to the BCD. The measured waveforms of the BCD well matched to the simulation results using Garfield++ with a field map obtained from Gmsh and Elmer. A sufficiently high separation efficiency was achieved at the same energy particles with different atomic number. |
Saturday, October 27, 2018 9:30AM - 9:45AM |
LH.00003: Directly Measuring SHE Mass Numbers with FIONA Jennifer L Pore, Jacklyn Gates, Gregory K Pang, Jeffrey T Kwarsick, Kenneth E Gregorich Super Heavy Elements (SHEs), which occur at the extreme limits of proton (Z) and neutron (N) numbers, are ideal testing grounds for investigations of exotic atomic and nuclear properties. Unfortunately, these elements are extremely difficult to study as they are short-lived and have alpha-decay chains that end in the spontaneous fission of nuclei with poorly-established Z and N. Presently, relative mass number (A) assignments for observed SHE isotopes are mostly well understood, but their placement on the nuclidic chart is heavily dependent on the extrapolated accuracy of the current nuclear mass models. It is extremely important to make a direct-experimental measurement of a SHE A so that we can anchor all of the relative A assignments, thus confirming the A of all observed SHEs. Lawrence Berkeley National Laboratory (LBNL) has a long history of studying SHEs with the Berkeley Gas-Filled Separator (BGS), which has recently been coupled to the newly-constructed apparatus For the Investigation of Nuclide A (FIONA). FIONA was designed to cool and bunch ions selected by the BGS before transporting them into a low-background area where they are separated and identified by their mass-to-charge ratio (A/q) on a tens-of-milliseconds timescale. Recent results will be presented. |
Saturday, October 27, 2018 9:45AM - 10:00AM |
LH.00004: Development of α-ToF detector for correlation measurement of atomic masses and decay properties T. Niwase, M. Wada, P. Schury, Y. Ito, D. Kaji, M. Rosenbusch, S. Kimura, K. Morimoto, H. Haba, S. Ishizawa, K. Morita, H. Miyatake, H. Wollnik The atomic mass is a unique quantity for each nucleus. Precise mass measurement allows us to identify the atomic number as well as the mass number. Recently, we measured the masses of fusion evaporation products provided from GARIS-II + MRTOF system. Next plan is the measurement the masses of superheavy nuclei (SHN) to identify the nuclides, the expected event rate is less than one event per day due to small cross section. We should accurately distinguish a true event from large background events such as molecular ions. For this purpose, we have developed an α-ToF detector, the time correlation between a time-of-flight signal and α decay signals can discriminate background events. The α-ToF detector is made of a commercial MagneToF detector and a Si PIN diode. When a heavy ion is hit on the MagneToF, secondary electron(SE) are emitted from the Impact plate of MagneToF and the electron are isochronously transported by a magnetic field an amplified by a multiplier to provide a timing signal of the ion. We replaced the impact plate with an SE emission material coated Si PIN diode. We tested the detector by using a 241Am alpha source, from the result of the test, we confirmed that the correlation between the timing signal and the decay energy can be measured using the α-ToF. |
Saturday, October 27, 2018 10:00AM - 10:15AM |
LH.00005: Follow-Ups on Great Achievements: New MRTOF-MS Projects at RIKEN-RIBF M. Rosenbusch, H. Haba, Y. Hirayama, S. Ishizawa, Y. Ito, D. Kaji, S. Kimura, H. Koura, H. Miyatake, J. Y. Moon, K. Morimoto, S. Nishimura, T. Niwase, P. Schury, A. Takamine, T. Tanaka, H. Ueno, M. Wada, Y. Watanabe, H. Wollnik The exotic isotopes of 249-253Md [1] and many other rare species like 210-214Ac/Ra [2] and intermediate-mass nuclei [3] and about 70 other isotopes have successfully been measured using a multi-reflection time-of-flight spectrograph (MRTOF-MS) at the super-heavy element (SHE)-mass facility of RIKEN-KEK [4]. After successful completion of the first SHE-Mass campaign, the setup has been redesigned for higher efficiencies. It has been relocated (with GARIS-II) to be behind the RRC accelerator with the new aim to measure the masses of 284Nh and 288Mc. Further MRTOF-MS devices are being developed to perform mass measurements of the most exotic species produced at RIKEN and will be placed in various locations as behind RIKEN's zero-degree spectrometer for symbiotic operation with other experiments. In this contribution, an overview of the future plans for low-energy precision mass measurements will be provided. [1] Y. Ito et al., Phys. Rev. Lett. 120, 102501 (2018) [2] M. Rosenbusch et al., Phys. Rev. C 97, 064306 (2018) [3] S. Kimura et al., IJMS 430, 134 (2018) [4] P. Schury et al., Nucl. Instr. Meth. B 335, 39 (2014) |
Saturday, October 27, 2018 10:15AM - 10:30AM |
LH.00006: Development of CHIP-TRAP: the Central Michigan University High Precision Penning Trap Nadeesha D Gamage, Madhawa V Horana Gamage, Kerim Gulyuz, Rachel Sandler, Matthew Redshaw At Central Michigan University we are developing the CHIP-TRAP mass spectrometer with the goal of performing ultra-high precision (<0.1 ppb) mass measurements on long-lived and stable isotopes. Of particular interest is a measurement of the 163Ho – 163Dy mass difference to provide the 163Ho electron capture Q value, which is required for direct neutrino mass determination experiments with 163Ho. CHIP-TRAP will consist of pair of hyperbolic precision measurement traps and a cylindrical capture/filter trap housed inside a 12 T superconducting magnet. Ions will be produced with a laser ablation ion source and a Penning ionization gauge type source and transported to the capture trap using electrostatic ion optics. Ions will be identified and contaminants removed in the capture trap, then transferred to one of the precision measurement traps where their cyclotron frequency will be measured via image charge detection techniques. We describe the design, construction and commissioning of the ion sources and ion transport beamline and the status of CHIP-TRAP. |
Saturday, October 27, 2018 10:30AM - 10:45AM |
LH.00007: Installation of an Enge Split-Pole Spectrograph at Notre Dame D.W. Bardayan, P.D. O'Malley, D. Robertson, E. Stech, M. Wiescher The structure of neutron-deficient exotic nuclei determines the proton-capture rates in a variety of explosive astrophysical events. Such nuclei can be studied using light-ion transfer reactions at the Notre Dame Nuclear Science Lab (NSL). To facilitate these studies, an Enge Split-Pole spectrograph is being transferred to the NSL from Oak Ridge National Laboratory. The progress of the installation and plans for its use will be detailed in this presentation. |
Saturday, October 27, 2018 10:45AM - 11:00AM |
LH.00008: New Developments with the Enge Split-Pole Spectrograph at Florida State University Erin Good, Catherine M Deibel, Lagy T Baby, Powell E Barber, Jeffery C Blackmon, Paul D Cottle, Kenneth Hanselman, Ashley A Hood, Jon Lighthall, Gordon McCann, Khang Pham, Ingo Wiedenhover The large acceptance Enge Split-Pole Spectrograph (SPS), formerly at Yale University, has recently been installed at Florida State University with a complement of new and upgraded auxiliary detectors and data acquisition systems. This setup can be used to measure nuclear structure information such as excitation energies, branching ratios, and angular distributions of states populated via transfer reactions. The auxiliary detector systems in conjunction with the SPS will be used for a variety of nuclear structure and astrophysics applications, including indirect measurements of reaction rates involving proton-rich nuclei, spectroscopic factors for exploring complete proton shell closures, unbound single proton states in the $\it{fp}$-shell, super-radiance in the $\it{sd}$-shell, and the measurement of ($\alpha$, p) reactions important in X-ray burst nucleosynthesis. The commissioning and first scientific runs with the SPS will be discussed. |
Saturday, October 27, 2018 11:00AM - 11:15AM |
LH.00009: Detector System for the Enge Split-Pole Spectrograph at Florida State University Khang H Pham, Erin Good, Catherine M Deibel, Jeffery C Blackmon, Jon Lighthall, Ashley A Hood, Lagy T Baby, Powell E Barber, Paul D Cottle, Ingo Wiedenhoever, Gordon McCann, Kenneth Hanselman As a collaborative project between Louisiana State University (LSU) and Florida State University (FSU), a large-acceptance Enge Split-Pole Spectrograph (SPS) was recently installed at FSU. The SPS is used to conduct charged-particle spectroscopy experiments using stable beams to study transfer reactions of interest to nuclear structure and astrophysics. Along with the SPS's installation, auxiliary detector systems have been refurbished and developed. These include the Silicon Array for Branching Ratio Experiments (SABRE) and the Focal Plane Detector (FPD). SABRE is an array of silicon detectors that is used to detect charged-particle decays to determine the angular momentum distributions of decay particles and branching ratios. The FPD is a proportional counter positioned at the focal plane of the SPS, where it measures the energy loss and two different positions along the path of the reaction products dispersed by the SPS to determine particle identification and magnetic rigidity. The design, development, and commissioning of these detectors will be discussed. |
Saturday, October 27, 2018 11:15AM - 11:30AM |
LH.00010: Commissioning of the Solenoid Spectrometer for Nuclear AstroPhysics at Notre Dame Jacob M Allen, Noah Applegate, Daniel Bardayan, Drew T Blankstein, Emmanuel Garcia, Matthew R Hall, Oscar B Hall, James J Kolata, Patrick D O'Malley, Frederick D Becchetti, Jeffery C Blackmon, Steven D. Pain
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Saturday, October 27, 2018 11:30AM - 11:45AM |
LH.00011: Establishing a model for the number of generated neutron using irradiated protons to a target in an accelerator-based neutron source for boron neutron capture therapy. Satoshi Nakamura, Hiroshi Igaki, Akihisa Wakita, Masashi Ito, Shie Nishioka, Kotaro Iijima, Hiroki Nakayama, Mihiro Takemori, Yoshihisa Abe, Kazuma Kobayashi, Kana Takahashi, Koji Inaba, Kae Okuma, Naoya Murakami, Yuko Nakayama, Hiroyuki Okamoto, Jun Itami An accelerator-based neutron source for boron neutron capture therapy (BNCT) is installing into National Cancer Center Hospital. In clinical situations, controlling the number of generated neutron is important for BNCT in order to provide an adequate radiotherapy. The purpose of this study is to establish a model for the number of generated neutron using irradiated protons to a target in the neutron source. Experiments were performed with an accelerator-based neutron source with a solid-state Li target (Cancer Care Intelligence systems, Inc.). A maximum thermal load to the target reaches 50 kW to acquire sufficient neutrons for BNCT. According to previous studies, the thermal load induces decrement of the Li target thickness, and its decrement induces reduction of the number of generated neutron per unit of proton current. Thus, the model was established by considering the thermal loads in this study. The calculated neutron flux using the model was compared with the measured one. Mean difference and standard deviation between the calculated and the measured neutron flux was (0.0±1.0)%. The model might be able to reflect interactions between the target and protons adequately. Therefore, the accelerator-based neutron source has a potential to perform BNCT using the model. |
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