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In atomic nuclei, the spin-orbit interaction originates from the coupling of the orbital motion of a nucleon with its intrinsic spin. Recent experimental and theoretical works have suggested a weakening of the spin-orbit interaction in neutron-rich nuclei far from stability. To study this phenomenon, we have investigated the spin-orbit energy splittings of single-hole and single-particle valence neutron orbits of 132Sn. The spectroscopic strength of single-hole states in 131Sn was determined from the measured differential cross sections of the tritons from the neutron-removing 132Sn(d, t)131Sn reaction, which was studied in inverse kinematics at the Holifield Radioactive Ion Beam Facility at Oak Ridge National Laboratory. The spectroscopic factors of the lowest 3/2+, 1/2+ and 5/2+ states were found to be consistent with their maximal values of (2j+1), confirming the robust N=82 shell closure at 132Sn. We compared the spin-orbit splitting of neutron single-hole states in 131Sn to those of single-particle states in 133Sn determined in a recent measurement of the 132Sn(d, p)133Sn reaction. We found a significant reduction of the energy splitting of the weakly bound 3p orbits compared to the well-bound 2d orbits, and that all the observed energy splittings can be reproduced remarkably well by calculations using a one-body spin-orbit interaction and a Woods–Saxon potential of standard radius and diffuseness. The observed reduction of spin-orbit splitting can be explained by the extended radial wavefunctions of the weakly bound orbits, without invoking a weakening of the spin-orbit strength. Keywords: Nuclear structure, Spin-orbit interaction, Transfer reactions, Doubly-magic nuclei, Shell model

Direct measurements of ( α , p ) reactions of astrophysical interest with radioactive beams presents serious challenges because of the difficult nature of helium targets and the typical low intensities of the beams. To address this, a new technique has been developed for measurements of low-energy ( α , p ) reactions with heavy ion beams using an extended 4 He gas target and a newly developed gas recirculating system. The system was used to measure the 4 He(19F, 1 H)22Ne reaction as a demonstration. Excitation functions of the 19F( α , p )22Ne and 19F( α , p ′ )22Ne ∗ reactions were successfully measured to show the viability of this technique. Details of the approach and future plans are given.

We report the coating of metal-free graphitic carbon nitride (g-C3N4) onto titanium dioxide (TiO2) nanorods via a thermal evaporation method. Prior to g-C3N4 coating, TiO2 nanoclusters were grown on TiO2 nanorods to enhance the surface area by dipping in a TiCl3 solution for 12, 24 and 36 h. The prepared films were analyzed to assess the improvement in absorbance and reduction in recombination losses. Nanoclustered TiO2 grown for 24 h and then coated with a g-C3N4 film (i.e., TC_24h_CN) had the highest photocurrent of 235 and 290 μA, respectively, when measured by transient photocurrent and linear sweep voltammetry techniques. The enhanced performance resulted from a reduced recombination of electron-hole pairs. The TC_24h_CN film displayed an excellent photoresponse over 15 h of exposure to visible light and hence could potentially be used in water purification device technology.

The astrophysical F 18 ( p , α ) O 15 rate determines, in large part, the extent to which the observable radioisotope 18 F is produced in novae. This rate, however, has been extremely uncertain owing to the unknown properties of a strong subthreshold resonance and its possible interference with higher-lying resonances. The new Jet Experiments in Nuclear Structure and Astrophysics (JENSA) gas-jet target has been used for the first time to determine the spin of this important resonance and significantly reduce uncertainties in the F 18 ( p , α ) O 15 rate.

To take full advantage of advanced exotic beam facilities, target technology must also be advanced. Particularly important to the study of astrophysical reaction rates is the creation of localized and dense targets of hydrogen and helium. The Jet Experiments in Nuclear Structure and Astrophysics (JENSA) gas-jet target has been constructed for this purpose. JENSA was constructed at Oak Ridge National Laboratory (ORNL) where it was tested and characterized, and has now moved to the ReA3 reaccelerated beam hall at the National Superconducting Cyclotron Laboratory (NSCL) at Michigan State University for use with radioactive beams.

A cascaded hybrid phase-locked loop (PLL) fabricated in a 65-nm CMOS process consumes 21 mW and occupies 0.4 mm2. An all-digital PLL (ADPLL) with piecewise linear calibrated hierarchical time-to-digital converter is proposed to achieve a wide operation range, and a charge-pump PLL (CPPLL) with an auxiliary (AUX) charge-pump for low current mismatch is cascaded to filter out the ADPLL output noise. The ADPLL achieves low long-term jitter regardless of the leakage current, and the CPPLL realizes low short-term jitter using a self-biased technique and the AUX charge pump. A phase-selectable divider is also proposed to divide the clock frequency while keeping the relative phase difference constant. The measured peak-to-peak short-term and long-term jitters at an output frequency of 315 MHz are 40 and 70 pspp, respectively, with a multiplication factor of 1024.

We propose a novel modulation profile for a spread spectrum clock generator (SSCG). The proposed piecewise linear (PWL) modulation profile significantly reduces electromagnetic interference with a simple implementation. Two SSCGs with two- and three-slope-PWL modulation profiles are used. Both SSCGs consist of the proposed spread spectrum control profile generator and a phase-locked loop that includes a high-resolution fractional divider to reduce quantization noise from a delta-sigma modulator. The SSCG with the two-slope-PWL modulation profile was fabricated in a 0.18 μm 1P4M CMOS technology. The measured peak power reduction level of the two-slope-PWL modulation profile is 14.2 dB with 5000 ppm down spreading at 1.5 GHz. The SSCG occupies an active area of 0.49 mm2 and consumes 40 mW of power at 1.5 GHz. The SSCG with the three-slope-PWL modulation profile was fabricated in a 0.13 μm 1P6M CMOS technology. The measured peak power reduction level of the three-slope-PWL modulation profile is 10.3 and 10.52 dB with 5000 ppm down spreading at 162 and 270 MHz, respectively. The SSCG occupies an active area of 0.096 mm2 and dissipates 1 mW of power at 270 MHz.

Novel program and read schemes are presented to break barriers in scaling of NAND flash memory such as threshold voltage endurance from floating gate interference, and charge loss tolerance. To enhance threshold voltage endurance and charge loss tolerance, we introduced three schemes; MSB Re-PGM scheme, Moving Read scheme and Adaptive Code Selection scheme. Using the MSB Re-PGM scheme, threshold voltage distribution width is improved about 200 mV. The PGM throughput is enhanced from 1500 μs to 1250 μs. With the Moving Read scheme about half order of UBER is improved with 10 bit ECC. Also, Adaptive Code Selection scheme are used to decrease a current consumption. There is 5.5% current reduction. With these techniques, 32-Gb MLC NAND flash memory has been fabricated using a 32 nm CMOS process technology. Its program throughput reaches 13.0 MB/s at a multi-plane program operation with cache operation keeping a desirable threshold voltage distribution.

A high-density supersonic gas-jet target named JENSA (Jet Experiments in Nuclear Structure and Astrophysics) has been constructed and commissioned at Oak Ridge National Laboratory. The target creates a localized (∼ 4 mm wide) thick (∼10 19 atoms/cm2) concentration of gaseous atoms (H, He, N, etc...) that are suitable for use in high-resolution experiments with radioactive beams. The interaction point of the beam with the gas-jet target is surrounded by silicon strip detectors from the SuperORRUBA (Oak Ridge Rutgers University Barrel Array) to detect reaction products with good energy (∼30 keV) and angular resolution (∼1 degree). Initial experiments are discussed along with plans for future use at Michigan State University.