R14 (Au, M)51 (R = Y, La–Nd, Sm–Tb, Ho, Er, Yb, Lu; M = Al, Ga, Ge, In, Sn, Sb, Bi): Stability Ranges and Site Preference in the Gd14Ag51 Structure Type
Abstract
Twenty new ternary representatives of the Gd14Ag51 structure type have been synthesized within the R-Au-M family (R = Y, La–Nd, Sm–Tb, Ho, Er, Yb, Lu; M = Al, Ga, Ge, In, Sn, Sb, Bi) using solid state synthesis techniques. The list of post transition metals (M) involved in the formation of this type of structure could be augmented by five new representatives. All compounds crystallize in the hexagonal space group P6/m (#175) with the unit cell ranges of a = 12.3136(2)–12.918(1) Å and c = 8.9967(3)–9.385(1) Å, and incorporate different degrees of Au/M mixing. The involvement of the post transition element in the structure varies from one to another compound both qualitatively and quantitatively. A rather significant phase width can be expected for the majority of compounds, however, not without exclusions. The distribution of the post transition metals within the structure has been analyzed via single crystal X-ray diffraction. While the positional disorder of one near-origin Au position is expectable for all compounds due to steric reasons, two specimens show an obvious deviation from the others including another Au position split along the c axis. Lastly, possible factors affecting this behavior are discussed.
- Authors:
-
[2];
[3];
[4]
- Ames Lab., Ames, IA (United States); Iowa State Univ., Ames, IA (United States). Dept. of Materials Science and Engineering
- Ames Lab., Ames, IA (United States); Stockholm Univ. (Sweden). Dept. of Materials and Environmental Chemistry
- Ames Lab., Ames, IA (United States); Univ. of Genova, Genova (Italy). Dept. of Chemistry; Consiglio Nazionale delle Ricerche (CNR), Genova (Italy). SPIN Inst.
- Ames Lab., Ames, IA (United States); Iowa State Univ., Ames, IA (United States). Dept. of Materials Science and Engineering; Stockholm Univ. (Sweden). Dept. of Materials and Environmental Chemistry
- Publication Date:
- Research Org.:
- Ames Laboratory (AMES), Ames, IA (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC), Basic Energy Sciences (BES); Stockholm University Sweden
- OSTI Identifier:
- 1425473
- Report Number(s):
- IS-J-9581
Journal ID: ISSN 1528-7483
- Grant/Contract Number:
- AC02-07CH11358
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Crystal Growth and Design
- Additional Journal Information:
- Journal Volume: 18; Journal Issue: 2; Journal ID: ISSN 1528-7483
- Publisher:
- American Chemical Society
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 36 MATERIALS SCIENCE
Citation Formats
Celania, Chris, Smetana, Volodymyr, Provino, Alessia, Manfrinetti, Pietro, and Mudring, Anja-Verena. R14 (Au, M)51 (R = Y, La–Nd, Sm–Tb, Ho, Er, Yb, Lu; M = Al, Ga, Ge, In, Sn, Sb, Bi): Stability Ranges and Site Preference in the Gd14Ag51 Structure Type. United States: N. p., 2017.
Web. doi:10.1021/acs.cgd.7b01469.
Celania, Chris, Smetana, Volodymyr, Provino, Alessia, Manfrinetti, Pietro, & Mudring, Anja-Verena. R14 (Au, M)51 (R = Y, La–Nd, Sm–Tb, Ho, Er, Yb, Lu; M = Al, Ga, Ge, In, Sn, Sb, Bi): Stability Ranges and Site Preference in the Gd14Ag51 Structure Type. United States. https://doi.org/10.1021/acs.cgd.7b01469
Celania, Chris, Smetana, Volodymyr, Provino, Alessia, Manfrinetti, Pietro, and Mudring, Anja-Verena. Tue .
"R14 (Au, M)51 (R = Y, La–Nd, Sm–Tb, Ho, Er, Yb, Lu; M = Al, Ga, Ge, In, Sn, Sb, Bi): Stability Ranges and Site Preference in the Gd14Ag51 Structure Type". United States. https://doi.org/10.1021/acs.cgd.7b01469. https://www.osti.gov/servlets/purl/1425473.
@article{osti_1425473,
title = {R14 (Au, M)51 (R = Y, La–Nd, Sm–Tb, Ho, Er, Yb, Lu; M = Al, Ga, Ge, In, Sn, Sb, Bi): Stability Ranges and Site Preference in the Gd14Ag51 Structure Type},
author = {Celania, Chris and Smetana, Volodymyr and Provino, Alessia and Manfrinetti, Pietro and Mudring, Anja-Verena},
abstractNote = {Twenty new ternary representatives of the Gd14Ag51 structure type have been synthesized within the R-Au-M family (R = Y, La–Nd, Sm–Tb, Ho, Er, Yb, Lu; M = Al, Ga, Ge, In, Sn, Sb, Bi) using solid state synthesis techniques. The list of post transition metals (M) involved in the formation of this type of structure could be augmented by five new representatives. All compounds crystallize in the hexagonal space group P6/m (#175) with the unit cell ranges of a = 12.3136(2)–12.918(1) Å and c = 8.9967(3)–9.385(1) Å, and incorporate different degrees of Au/M mixing. The involvement of the post transition element in the structure varies from one to another compound both qualitatively and quantitatively. A rather significant phase width can be expected for the majority of compounds, however, not without exclusions. The distribution of the post transition metals within the structure has been analyzed via single crystal X-ray diffraction. While the positional disorder of one near-origin Au position is expectable for all compounds due to steric reasons, two specimens show an obvious deviation from the others including another Au position split along the c axis. Lastly, possible factors affecting this behavior are discussed.},
doi = {10.1021/acs.cgd.7b01469},
journal = {Crystal Growth and Design},
number = 2,
volume = 18,
place = {United States},
year = {Tue Dec 19 00:00:00 EST 2017},
month = {Tue Dec 19 00:00:00 EST 2017}
}
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Figures / Tables:
Table 1: Crystallographic Details and Refinement Parameters for Gd14(Au, Sb)51, Lu14(Au, Ga)51, and La14(Au, Bi)51
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