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At least 505 records · Page 28

ThAu 2 – , ThAu 2 O – , and ThAuOH – anions: Photoelectron spectroscopic and theoretical characterization

The thorium–gold negative ions ThAu 2 – , ThAu 2 O – , and ThAuOH – have been observed and experimentally characterized by anion photoelectron spectroscopy. These experiments are accompanied by extensive ab initio electronic structure calculations using a relativistic composite methodology based primarily on coupled cluster singles and doubles with perturbative triples calculations. The theoretical electron affinities (EAs) at 0 K agree with the experimental adiabatic EAs to within 0.02 eV for all species. Two separate isomers were located in the calculations for ThAuOH – , and detachment from both of these appears to be present in the photoelectron spectrum. Excited electronic states of the neutral molecules are reported at the equation of motion-coupled cluster singles and doubles level of theory. Atomization energies and heats of formation are also calculated for each neutral species and have expected uncertainties of 3 and 4 kcal/mol, respectively. The σ bonds between Th and Au are determined by natural bond orbital analysis to consist of predominately sd hybrids on Th bonding with the Au 6s orbital. In order to investigate the correspondence between the bonding in Th–Au and Th–F molecules, a limited number of calculations were also carried out on most of the F-analogs of this study. These results demonstrate that Au does behave like F in these cases, although the Th–F σ bonds are much more ionic compared to Th–Au. This results in an EA for ThF 2 that is 10 kcal/mol smaller than that of ThAu 2 . The EA values for the Th(IV) species, i.e., ThX 2 O and ThXOH, only differed, however, by 3–4 kcal/mol.

37 INORGANIC, ORGANIC, PHYSICAL, AND ANALYTICAL CH↗

Thermal energy mitigation and toroidal peaking effects in JET disruptions

Previous investigations on JET suggest half or less of plasma stored thermal energy W th is radiated (f rad,th ≲ 0.5) using either massive gas injection (MGI) or shattered pellet injection (SPI) disruption mitigation. We investigate whether the apparent incomplete f rad,th is explained by radiation peaking near the injection plume. High toroidal peaking throughout the pre-thermal quench is found in argon–deuterium MGI on JET, with typically >3× higher radiation near the injector than toroidally distant. Previously unexplained toroidal bolometry measurements in neon–deuterium SPI are reproduced with similar peaking using the Emis3D radiation analysis code. These observations align with results from Alcator C-Mod and KSTAR. This peaking is not captured by previous JET studies that found poor thermal mitigation. Two sets of neon–deuterium SPI and two sets of argon–deuterium MGI are analyzed using Emis3D. In SPI, f rad,th rises from no-plume estimates of 0.31 and 0.66 to lower bounds of 0.84 and 0.92, respectively, and f rad,th ∼ 1 is possible. In MGI, the toroidal spread of the peaking feature is poorly constrained. f rad,th up to 0.85 and 0.65 are possible using the largest possible spread, increasing from 0.42 and 0.28, although f rad,th ∼ 1 does not appear to be reached. Revised mitigation estimates on JET suggest a lower melt risk to the divertor in mitigated disruptions on ITER and SPARC than previously thought. However, peaking near injectors could increase flash melting risk on nearby plasma facing components.

70 PLASMA PHYSICS AND FUSION TECHNOLOGY↗

Differential ultrastructural alterations in the Vglut2 glutamatergic input to the substantia nigra pars compacta/pars reticulata following nigrostriatal dopamine loss in a progressive mouse model of Parkinson’s disease

Abstract Loss of nigrostriatal dopamine (DA) in Parkinson's disease results in over‐activation/bursting of the subthalamic nucleus (STN). The STN projects to the substantia nigra (SN) pars compacta (SNpc) and pars reticulata (SNpr). The vesicular glutamate transporter 2 (Vglut2) is localized within at least STN terminals synapsing within the SN, but it is not known if there are differential changes in the Vglut2+ input to the SNpc versus SNpr following DA loss. The goal/rationale of this current study was to determine whether there were differential changes in the density/levels of glutamate immuno‐gold labeling within Vglut2+ nerve terminals synapsing in the SNpc/SNpr and in the proportion of Vglut2+ terminals contacting tyrosine hydroxylase (TH) positively(+) or negatively(−) labeled dendrites following DA loss. Within the SNpc, there was a significant increase (51.3%) in the density of nerve terminal glutamate immuno‐gold labeling within Vglut2+ terminals synapsing on TH(−) dendrites following MPTP versus the vehicle ( VEH ) group. There was a significant decrease (16%) in the percentage of Vglut2+ terminals contacting TH(+) labeled dendrites in the MPTP‐ versus VEH‐treated group within the SNpc. Within the SNpr, there was a significant decrease in the density of glutamate immuno‐gold labeling in Vglut2+ terminals contacting TH(+) (71.5%) and TH(−) (55.5%) labeled dendrites, suggesting an increase in glutamate release. There was no change in the percentage of Vglut2+ terminals contacting TH(+) or TH(−) dendrites in the SNpr. We conclude that there is a differential effect following DA loss on the glutamate input from Vglut2+ terminals synapsing within the SNpr versus SNpc.

Moore, Cynthia↗

Efficient implementation of weighted ENO schemes

In this paper, we further analyze, test, modify and improve the high order WENO (weighted essentially non-oscillatory) finite difference schemes of Liu, Osher and Chan. It was shown by Liu et al. that WENO schemes constructed from the r-th order (in L1 norm) ENO schemes are (r+1)-th order accurate. We propose a new way of measuring the smoothness of a numerical solution, emulating the idea of minimizing the total variation of the approximation, which results in a 5-th order WENO scheme for the case r = 3, instead of the 4-th order with the original smoothness measurement by Liu et al. This 5-th order WENO scheme is as fast as the 4-th order WENO scheme of Liu et al., and both schemes are about twice as fast as the 4-th order ENO schemes on vector supercomputers and as fast on serial and parallel computers. For Euler systems of gas dynamics, we suggest computing the weights from pressure and entropy instead of the characteristic values to simplify the costly characteristic procedure. The resulting WENO schemes are about twice as fast as the WENO schemes using the characteristic decompositions to compute weights, and work well for problems which do not contain strong shocks or strong reflected waves. We also prove that, for conservation laws with smooth solutions, all WENO schemes are convergent. Many numerical tests, including the 1D steady state nozzle flow problem and 2D shock entropy wave interaction problem, are presented to demonstrate the remarkable capability of the WENO schemes, especially the WENO scheme using the new smoothness measurement, in resolving complicated shock and flow structures. We have also applied Yang's artificial compression method to the WENO schemes to sharpen contact discontinuities.

Jiang, Guang-Shan↗

A dopaminergic projection to the rat mammillary nuclei demonstrated by retrograde transport of wheat germ agglutinin-horseradish peroxidase and tyrosine hydroxylase immunohistochemistry

The presence and distribution of dopaminergic neurons and terminals in the hypothalamus of the rat were studied by tyrosine hydroxylase (TH) immunohistochemistry. Strongly labelled TH-immunoreactive neurons were seen in the dorsomedial hypothalamic nucleus, periventricular region, zona incerta, arcuate nucleus, and supramammillary nucleus. A few TH-positive neurons were also identified in the dorsal and ventral premammillary nucleus, as well as the lateral hypothalamic area. TH-immunoreactive fibres and terminals were unevenly distributed in the mammillary nuclei; small, weakly labelled terminals were scattered in the medial mammillary nucleus, while large, strongly labelled, varicose terminals were densely concentrated in the internal part of the lateral mammillary nucleus. A few dorsoventrally oriented TH-positive axon bundles were also identified in the lateral mammillary nucleus. A dopaminergic projection to the mammillary nuclei from the supramammillary nucleus and lateral hypothalamic area was identified by double labelling with retrograde transport of wheat germ agglutinin-horseradish peroxidase and TH-immunohistochemistry. The lateral mammillary nucleus receives a weak dopaminergic projection from the medial, and stronger projections from the lateral, caudal supramammillary nucleus. The double-labelled neurons in the lateral supramammillary nucleus appear to encapsulate the caudal end of the mammillary nuclei. The medial mammillary nucleus receives a very light dopaminergic projection from the caudal lateral hypothalamic area. These results suggest that the supramammillary nucleus is the principal source of the dopaminergic input to the mammillary nuclei, establishing a local TH-pathway in the mammillary complex. The supramammillary cell groups are able to modulate the limbic system through its dopaminergic input to the mammillary nuclei as well as through its extensive dopaminergic projection to the lateral septal nucleus.

Non-NASA Center↗

NASA's Habitation Development Status: Current Concepts and ISRU Opportunities

Introduction: The National Aeronautics and Space Administration (NASA) is embarking on a bold journey to return humankind to the Moon and onward to Mars with innovative commercial, international, and academic partnerships [1]. Under the Artemis series of missions, NASA seeks to establish sustained human exploration of deep space through an objectives-based approach [2]. This approach drives the identification of needed system functionality and the current and future capabilities which will eventually allow humanity to sustainably live beyond Earth. Providing evolvable and scalable habitation is a cornerstone function that calls for the collection and integration of current, developmental, and future technologies that can meet near-term exploration needs while growing into long-term sustained presence. NASA is advancing in-space habitation through its Next Space Technologies for Exploration Partnerships (NextSTEP) model while designing lunar, Mars transit, and Mars surface habitat government reference concepts for Artemis missions. These efforts have unveiled possible near-term opportunities for the in-space resource utilization community if human habitation is considered a future customer of space resources. NextSTEP Habitation Development: NASA is closely working with commercial partners under its NextSTEP Appendix A model to advance habitation systems in the arena of inflatable and composite habitation structures. Such efforts promise efficiencies in volumetric packaging and overall spacecraft mass respectively. Recent testing by commercial partners have helped to quantify possible failure mechanisms for inflatable structures while advancing their technology towards eventual flight certification. The advancement of such Class II habitation structures, in which the habitat is only fully deployed once in-space or on a planetary surface [3], is critical to providing increased habitable volume for long-duration missions with no additional mass penalties. The progression of such technology is infused into NASA’s government reference concepts for notional deep space habitation concepts. Current Government Reference Concepts: To best inform the formulation of future collaborative solicitations, NASA employs the practice of internally developing reference concepts for future exploration elements. These concepts aid in identifying the functions and capabilities needed to complete NASA missions as well as feasible solutions within the timeframe needed. Government reference concepts for a lunar Surface Habitat, Mars Transit Habitat, and Mars Sur-face Habitat are continuously being developed and updated to better guide the Agency’s overall exploration architecture. Lunar Surface Habitat. As NASA returns to the Moon, it is evaluating possible lunar surface habitation concepts. The Surface Habitat (SH) reference concept entails a hybrid metallic-inflatable structure capable of initially housing two crew for surface stays of up to 30 days in duration [4]. While initial missions may span ~7 days in duration, consideration is being given to expanding SH’s capability to support a crew of four for up to 60 days over its 15-year design life [5]. Functionally, the SH serves as a ‘hub’ for all Artemis crewed surface operations, providing internal volume for maintenance, medical, logistics, science utilization, and extravehicular activity (EVA) support in addition to core habitation functionality such as environmental control and life support (ECLS) and power generation and distribution among many others. Additionally, NASA has entered a study agreement with the Italian Space Agency (Agenzia Spaziale Italiana – ASI) to investigation a possible Multi-Purpose Habitat (MPH) as an additional or augmenting habit-able element for the lunar surface [6]. Mars Transit Habitat. NASA’s current architectural concept for initial human missions to Mars entails the utilization of a transit habitat (TH) to transport a four-person crew to and from Mars orbit, departing from and returning to a lunar near-rectilinear halo orbit (NRHO), over the course of a ~1,200-day mission [5]. While holding a similar 15-year design lifetime, TH will also support a series of analog mission activities in NRHO to gradually test the systems and interaction with lunar surface elements, some of which may be adapted for Mars surface exploration. Holding similar functional capabilities as SH, TH is sized to support much longer durations in space and greater logistical independence. Mars Surface Habitat. NASA is still exploring the concept of operations for initial crewed missions to Mars. As such, the Mars Surface Habitat (MSH) concept is still in its infancy as options for mobile, pressurized habitation and stationary habitats are being explored. It is expected MSH will leverage heavily from the lunar SH and possible lunar pressurized rover, however the very different Martian environment will likely necessitate modifications. ISRU Opportunities: Despite the advancements under NASA’s NextSTEP habitation work and continually optimized reference concepts, NASA is facing near-term mass and power challenges that may create opportunities to the ISRU community by providing yet another possible customer for space resources. While NASA desires to use regenerative ECLS systems (ECLSS) for all habitation concepts, their operation comes with initial mass penalties and maintenance overheads when compared to simpler open-loop architectures. Because of this, NASA is currently pro-posing an open-loop, consumables-based architecture for its surface habitats to achieve initial launch and delivery lander mass targets while scarring for the in-corporation of regenerative ECLSS to meet longer mission durations and sustained presence. With such an architecture, oxygen and potable water are needed consumables, which initial ISRU systems may be able to provide in a pilot capacity. Although the TH is expecting to utilize regenerative ECLSS, advancements in lunar surface-based ISRU and possible re-supply of spacecraft in lunar or Mars orbit could significantly reduce the logistical need for ECLSS related spares on TH and possibly allow a similar open-loop and consumables-based architecture. Table 1 Notional ECLSS consumables per mission use for SH and TH [5]. SH (28-day) Open Loop: Water (kg) 288 | Oxygen (kg) 30 TH (1110-day) Closed-Loop: Water (kg) 182 | Oxygen (kg) 123 In addition to ECLSS mass concerns, the SH is facing challenges with energy storage to support operations over periods of darkness exceeding 100 hours. Both battery and fuel cell-based power architectures are being traded, opening options for external power generation and energy storage. One possibility is ISRU-produced H2 and O2 feeding external primary fuel cell systems which could supplement habitation power generation while reducing initial mass and volume until much more powerful fission power systems might be deployed. Conclusion: Significant advancements are being made in evolvable habitation concepts that span from near-term technologies, such as inflatable structures under NextSTEP, to potentially revolutionary capabilities like the lunar surface construction as funded through the Moon-to-Mars Planetary Autonomous Construction Technologies (MMPACT) project [7]. As NASA investigates both heritage capabilities and rap-idly advancing, disruptive technologies, there are likely many near-term opportunities for initial ISRU capabilities to significantly aid human habitation and increase self-sufficiency beyond Earth.

habitation↗

Materials Data on ThCd2 by Materials Project

ThCd2 crystallizes in the hexagonal P6/mmm space group. The structure is three-dimensional. Th is bonded in a 12-coordinate geometry to two equivalent Th and twelve equivalent Cd atoms. Both Th–Th bond lengths are 3.38 Å. All Th–Cd bond lengths are 3.42 Å. Cd is bonded in a 11-coordinate geometry to six equivalent Th and five equivalent Cd atoms. There are three shorter (2.97 Å) and two longer (3.38 Å) Cd–Cd bond lengths.

36 MATERIALS SCIENCE↗

Materials Data on ThAl2 by Materials Project

ThAl2 is Cubic Laves structured and crystallizes in the cubic Fd-3m space group. The structure is three-dimensional. Th is bonded in a 12-coordinate geometry to four equivalent Th and twelve equivalent Al atoms. All Th–Th bond lengths are 3.49 Å. All Th–Al bond lengths are 3.34 Å. Al is bonded to six equivalent Th and six equivalent Al atoms to form a mixture of face, edge, and corner-sharing AlTh6Al6 cuboctahedra. All Al–Al bond lengths are 2.85 Å.

36 MATERIALS SCIENCE↗

Materials Data on ThCoSn by Materials Project

ThCoSn crystallizes in the hexagonal P-62m space group. The structure is three-dimensional. Th is bonded in a 11-coordinate geometry to five Co and six equivalent Sn atoms. There are four shorter (3.01 Å) and one longer (3.04 Å) Th–Co bond lengths. There are two shorter (3.21 Å) and four longer (3.35 Å) Th–Sn bond lengths. There are two inequivalent Co sites. In the first Co site, Co is bonded in a 9-coordinate geometry to six equivalent Th and three equivalent Sn atoms. All Co–Sn bond lengths are 2.82 Å. In the second Co site, Co is bonded in a 9-coordinate geometry to three equivalent Th and six equivalent Sn atoms. All Co–Sn bond lengths are 2.74 Å. Sn is bonded in a 12-coordinate geometry to six equivalent Th and four Co atoms.

36 MATERIALS SCIENCE↗

Materials Data on Th6CoBr15 by Materials Project

Th6CoBr15 crystallizes in the cubic Im-3m space group. The structure is three-dimensional and consists of two Th6CoBr15 frameworks. Th is bonded to one Co and five Br atoms to form a mixture of edge and corner-sharing ThCoBr5 octahedra. The corner-sharing octahedral tilt angles are 0°. The Th–Co bond length is 2.79 Å. There are four shorter (2.93 Å) and one longer (3.09 Å) Th–Br bond lengths. Co is bonded in an octahedral geometry to six equivalent Th atoms. There are two inequivalent Br sites. In the first Br site, Br is bonded in an L-shaped geometry to two equivalent Th atoms. In the second Br site, Br is bonded in a linear geometry to two equivalent Th atoms.

36 MATERIALS SCIENCE↗

Materials Data on Th2Zn17 by Materials Project

Th2Zn17 crystallizes in the trigonal R-3m space group. The structure is three-dimensional. Th is bonded in a 10-coordinate geometry to nineteen Zn atoms. There are a spread of Th–Zn bond distances ranging from 3.16–3.47 Å. There are four inequivalent Zn sites. In the first Zn site, Zn is bonded to two equivalent Th and ten Zn atoms to form a mixture of distorted face, edge, and corner-sharing ZnTh2Zn10 cuboctahedra. There are a spread of Zn–Zn bond distances ranging from 2.60–2.77 Å. In the second Zn site, Zn is bonded to two equivalent Th and ten Zn atoms to form a mixture of distorted face, edge, and corner-sharing ZnTh2Zn10 cuboctahedra. There are a spread of Zn–Zn bond distances ranging from 2.66–2.97 Å. In the third Zn site, Zn is bonded to three equivalent Th and nine Zn atoms to form a mixture of distorted face, edge, and corner-sharing ZnTh3Zn9 cuboctahedra. There are two shorter (2.59 Å) and one longer (2.89 Å) Zn–Zn bond lengths. In the fourth Zn site, Zn is bonded in a 2-coordinate geometry to one Th and thirteen Zn atoms. The Zn–Zn bond length is 2.61 Å.

36 MATERIALS SCIENCE↗

Materials Data on Th2Cu by Materials Project

CuTh2 crystallizes in the hexagonal P6/mmm space group. The structure is three-dimensional. Th is bonded in a distorted q6 geometry to five equivalent Th and six equivalent Cu atoms. There are three shorter (3.10 Å) and two longer (3.12 Å) Th–Th bond lengths. All Th–Cu bond lengths are 3.47 Å. Cu is bonded in a 12-coordinate geometry to twelve equivalent Th and two equivalent Cu atoms. Both Cu–Cu bond lengths are 3.12 Å.

36 MATERIALS SCIENCE↗

Materials Data on Th6FeBr15 by Materials Project

Th6FeBr15 crystallizes in the cubic Im-3m space group. The structure is three-dimensional and consists of two Th6FeBr15 frameworks. Th is bonded to one Fe and five Br atoms to form a mixture of edge and corner-sharing ThFeBr5 octahedra. The corner-sharing octahedral tilt angles are 0°. The Th–Fe bond length is 2.77 Å. There are four shorter (2.94 Å) and one longer (3.05 Å) Th–Br bond lengths. Fe is bonded in an octahedral geometry to six equivalent Th atoms. There are two inequivalent Br sites. In the first Br site, Br is bonded in a linear geometry to two equivalent Th atoms. In the second Br site, Br is bonded in an L-shaped geometry to two equivalent Th atoms.

36 MATERIALS SCIENCE↗

Materials Data on ThMg2 by Materials Project

ThMg2 is Cubic Laves structured and crystallizes in the cubic Fd-3m space group. The structure is three-dimensional. Mg is bonded to six equivalent Mg and six equivalent Th atoms to form a mixture of corner, edge, and face-sharing MgTh6Mg6 cuboctahedra. All Mg–Mg bond lengths are 3.02 Å. All Mg–Th bond lengths are 3.55 Å. Th is bonded in a 12-coordinate geometry to twelve equivalent Mg and four equivalent Th atoms. All Th–Th bond lengths are 3.70 Å.

36 MATERIALS SCIENCE↗

Materials Data on Th2Fe17 by Materials Project

Th2Fe17 crystallizes in the trigonal R-3m space group. The structure is three-dimensional. Th is bonded in a 10-coordinate geometry to nineteen Fe atoms. There are a spread of Th–Fe bond distances ranging from 3.04–3.29 Å. There are four inequivalent Fe sites. In the first Fe site, Fe is bonded to two equivalent Th and ten Fe atoms to form a mixture of edge, corner, and face-sharing FeTh2Fe10 cuboctahedra. There are a spread of Fe–Fe bond distances ranging from 2.45–2.62 Å. In the second Fe site, Fe is bonded to two equivalent Th and ten Fe atoms to form a mixture of distorted edge, corner, and face-sharing FeTh2Fe10 cuboctahedra. There are a spread of Fe–Fe bond distances ranging from 2.47–2.75 Å. In the third Fe site, Fe is bonded to three equivalent Th and nine Fe atoms to form a mixture of edge, corner, and face-sharing FeTh3Fe9 cuboctahedra. There are two shorter (2.48 Å) and one longer (2.65 Å) Fe–Fe bond lengths. In the fourth Fe site, Fe is bonded in a 2-coordinate geometry to one Th and thirteen Fe atoms. The Fe–Fe bond length is 2.40 Å.

36 MATERIALS SCIENCE↗

Materials Data on YbTh3 by Materials Project

Th3Yb is Uranium Silicide structured and crystallizes in the cubic Pm-3m space group. The structure is three-dimensional. Th is bonded to eight equivalent Th and four equivalent Yb atoms to form ThYb4Th8 cuboctahedra that share corners with twelve equivalent ThYb4Th8 cuboctahedra, edges with eight equivalent YbTh12 cuboctahedra, edges with sixteen equivalent ThYb4Th8 cuboctahedra, faces with four equivalent YbTh12 cuboctahedra, and faces with fourteen equivalent ThYb4Th8 cuboctahedra. All Th–Th bond lengths are 3.58 Å. All Th–Yb bond lengths are 3.58 Å. Yb is bonded to twelve equivalent Th atoms to form YbTh12 cuboctahedra that share corners with twelve equivalent YbTh12 cuboctahedra, edges with twenty-four equivalent ThYb4Th8 cuboctahedra, faces with six equivalent YbTh12 cuboctahedra, and faces with twelve equivalent ThYb4Th8 cuboctahedra.

36 MATERIALS SCIENCE↗

Materials Data on LuTh3 by Materials Project

Th3Lu is Uranium Silicide structured and crystallizes in the cubic Pm-3m space group. The structure is three-dimensional. Th is bonded to eight equivalent Th and four equivalent Lu atoms to form ThLu4Th8 cuboctahedra that share corners with twelve equivalent ThLu4Th8 cuboctahedra, edges with eight equivalent LuTh12 cuboctahedra, edges with sixteen equivalent ThLu4Th8 cuboctahedra, faces with four equivalent LuTh12 cuboctahedra, and faces with fourteen equivalent ThLu4Th8 cuboctahedra. All Th–Th bond lengths are 3.56 Å. All Th–Lu bond lengths are 3.56 Å. Lu is bonded to twelve equivalent Th atoms to form LuTh12 cuboctahedra that share corners with twelve equivalent LuTh12 cuboctahedra, edges with twenty-four equivalent ThLu4Th8 cuboctahedra, faces with six equivalent LuTh12 cuboctahedra, and faces with twelve equivalent ThLu4Th8 cuboctahedra.

36 MATERIALS SCIENCE↗

Materials Data on SmTh3 by Materials Project

Th3Sm is Uranium Silicide structured and crystallizes in the cubic Pm-3m space group. The structure is three-dimensional. Th is bonded to eight equivalent Th and four equivalent Sm atoms to form ThSm4Th8 cuboctahedra that share corners with twelve equivalent ThSm4Th8 cuboctahedra, edges with eight equivalent SmTh12 cuboctahedra, edges with sixteen equivalent ThSm4Th8 cuboctahedra, faces with four equivalent SmTh12 cuboctahedra, and faces with fourteen equivalent ThSm4Th8 cuboctahedra. All Th–Th bond lengths are 3.57 Å. All Th–Sm bond lengths are 3.57 Å. Sm is bonded to twelve equivalent Th atoms to form SmTh12 cuboctahedra that share corners with twelve equivalent SmTh12 cuboctahedra, edges with twenty-four equivalent ThSm4Th8 cuboctahedra, faces with six equivalent SmTh12 cuboctahedra, and faces with twelve equivalent ThSm4Th8 cuboctahedra.

36 MATERIALS SCIENCE↗