105 research outputs found
Detection of Elements at All Three r-process Peaks in the Metal-Poor Star HD 160617
We report the first detection of elements at all three r-process peaks in the
metal-poor halo star HD 160617. These elements include arsenic and selenium,
which have not been detected previously in halo stars, and the elements
tellurium, osmium, iridium, and platinum, which have been detected previously.
Absorption lines of these elements are found in archive observations made with
the Space Telescope Imaging Spectrograph onboard the Hubble Space Telescope. We
present up-to-date absolute atomic transition probabilities and complete line
component patterns for these elements. Additional archival spectra of this star
from several ground-based instruments allow us to derive abundances or upper
limits of 45 elements in HD 160617, including 27 elements produced by
neutron-capture reactions. The average abundances of the elements at the three
r-process peaks are similar to the predicted solar system r-process residuals
when scaled to the abundances in the rare earth element domain. This result for
arsenic and selenium may be surprising in light of predictions that the
production of the lightest r-process elements generally should be decoupled
from the heavier r-process elements.Comment: Published in the Astrophysical Journal (22 pages, 12 figures
You Call It Honor, We Call It Dishonor. Counterstorytelling & Confederate Monuments in Isle of Wight County, Virginia
This essay considers how everyday citizens use counterstorytelling as a persuasive tactic in sites of ordinary democracy like public hearings. Specifically, we examine the counterstories and stock stories shared during a public hearing held in Isle of Wight County, Virginia to determine the future of a confederate monument that stood in front of the county\u27s courthouse. By focusing closely on one particular counterstory, this essay considers counter storytelling as a form of racial countermemory that challenges dominant narratives by centralizing social justice and anti-racism. The authors aim to contribute to understandings of storytelling and its role within sites of participatory democracy, particularly concerning debates over contested memory objects
A Spectroscopic study of laser-induced Tin-Lead plasma: transition probabilities for spectral lines of Sn I
In this paper, we present transition probabilities for 97 spectral lines of Sn I, corresponding to transitions n(n = 6,7,8)s → 5p2, n(n = 5,6,7)d → 5p2, 5p3 → 5p2, n(n = 7)p → 6s, determined by measuring the intensities of the emission lines of a Laser-induced breakdown (emission) spectrometry (LIBS). The optical emission spectroscopy from a laser-induced plasma generated by a 10 640 Å radiation, with an irradiance of 1.4 × 1010 Wcm− 2 on an Sn–Pb alloy (an Sn content of approximately 20%), in vacuum, was recorded at 0.8 µs, and analysed between 1900 and 7000 Å. The population-level distribution and corresponding temperature were obtained using Boltzmann plots. The electron density of the plasma was determined using well-known Stark broadening parameters of spectral lines. The plasma under study had an electron temperature of 13,200 K and an electron number density of 2 × 1016 cm− 3. The experimental relative transition probabilities were put on an absolute scale using the branching ratio method to calculate Sn I multiplet transition probabilities from available radiative lifetime data of their upper states and plotting the Sn I emission spectrum lines on a Boltzmann plot assuming local thermodynamic equilibrium (LTE) to be valid and following Boltzmann's law. The LTE conditions and plasma homogeneity have been checked. Special attention was paid to the possible self-absorption of the different transitions. The experimental results obtained have been compared with the experimental values given by other authors
Evolution of nuclear structure in neutron-rich odd-Zn isotopes and isomers
Collinear laser spectroscopy was performed on Zn (Z=30) isotopes at ISOLDE, CERN. The study of hyperfine spectra of nuclei across the Zn isotopic chain, N=33–49, allowed the measurement of nuclear spins for the ground and isomeric states in odd-A neutron-rich nuclei up to N=50. Exactly one long-lived (>10 ms) isomeric state has been established in each 69–79Zn isotope. The nuclear magnetic dipole moments and spectroscopic quadrupole moments are well reproduced by large-scale shell–model calculations in the f5pg9 and fpg9d5 model spaces, thus establishing the dominant term in their wave function. The magnetic moment of the intruder Iπ=1/2+ isomer in 79Zn is reproduced only if the νs1/2 orbital is added to the valence space, as realized in the recently developed PFSDG-U interaction. The spin and moments of the low-lying isomeric state in 73Zn suggest a strong onset of deformation at N=43, while the progression towards 79Zn points to the stability of the Z=28 and N=50 shell gaps, supporting the magicity of 78Ni
Nuclear charge radii of ⁶²⁻⁸⁰Zn and their dependence on cross-shell proton excitations
Nuclear charge radii of ⁶²⁻⁸⁰Zn have been determined using collinear laser spectroscopy of bunched ion beams at CERN-ISOLDE. The subtle variations of observed charge radii, both within one isotope and along the full range of neutron numbers, are found to be well described in terms of the proton
excitations across the Z = 28 shell gap, as predicted by large-scale shell model calculations. It comprehensively explains the changes in isomer-to-ground state mean square charge radii of ⁶⁹⁻⁷⁹Zn, the inversion of the
odd-even staggering around N = 40 and the odd-even staggering systematics of the Zn charge radii. With two protons above Z = 28, the observed charge radii of the Zn isotopic chain show a cumulative effect of different aspects of nuclear structure including single particle structure, shell closure, correlations and deformations near the proposed doubly magic nuclei, ⁶⁸Ni and ⁷⁸Ni
Determination of radiative lifetimes of neutral bismuth by time-resolved uv-vuv laser spectroscopy
Perceptual quality of BRDF approximations: dataset and metrics
International audienceBidirectional Reflectance Distribution Functions (BRDFs) are pivotal to the perceived realism in image synthesis. While measured BRDF datasets are available, reflectance functions are most of the time approximated by analytical formulas for storage efficiency reasons. These approximations are often obtained by minimizing metrics such as L 2 —or weighted quadratic—distances, but these metrics do not usually correlate well with perceptual quality when the BRDF is used in a rendering context, which motivates a perceptual study. The contributions of this paper are threefold. First, we perform a large-scale user study to assess the perceptual quality of 2026 BRDF approximations, resulting in 84138 judgments across 1005 unique participants. We explore this dataset and analyze perceptual scores based on material type and illumination. Second, we assess nine analytical BRDF models in their ability to approximate tabulated BRDFs. Third, we assess several image-based and BRDF-based (Lp, optimal transport and kernel distance) metrics in their ability to approximate perceptual similarity judgments
Gamma Factory at CERN – novel research tools made of light
We discuss the possibility of creating novel research tools by producing and
storing highly relativistic beams of highly ionised atoms in the CERN
accelerator complex, and by exciting their atomic degrees of freedom with
lasers to produce high-energy photon beams. Intensity of such photon beams
would be by several orders of magnitude higher than offered by the presently
operating light sources, in the particularly interesting gamma-ray energy
domain of 0.1-400 MeV. In this energy range, the high-intensity photon beams
can be used to produce secondary beams of polarised electrons, polarised
positrons, polarised muons, neutrinos, neutrons and radioactive ions. New
research opportunities in a wide domain of fundamental and applied physics can
be opened by the Gamma Factory scientific programme based on the above primary
and secondary beams.Comment: 12 pages; presented by W. Placzek at the XXV Cracow Epiphany
Conference on Advances in Heavy Ion Physics, 8-11 January 2019, Cracow,
Polan
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