The crystal is part of the R–Mg–Zn family of crystals, where R=Y, Gd, Tb, Dy, Ho or Er. They were first discovered in 1994.[3] These form quasicrystals in the stoichiometry around R 9Mg 34Zn 57.[2] Magnetically, they form a spin glass at cryogenic temperatures.
While the experimental discovery of quasicrystals dates back to the 1980s, the relatively large, single grain nature of some Ho–Mg–Zn quasicrystals has made them a popular way to illustrate the concept.[4][5]
^Canfield, Paul C.; Fisher, Ian R. (2001). "High-temperature solution growth of intermetallic single crystals and quasicrystals". Journal of Crystal Growth. 225 (2–4). Elsevier BV: 155–161. doi:10.1016/s0022-0248(01)00827-2. ISSN0022-0248.
^ abFisher, I.R; Islam, Z; Zarestky, J; Stassis, C; Kramer, M.J; Goldman, A.I; Canfield, P.C (2000). "Magnetic properties of icosahedral R–Mg–Zn quasicrystals (R=Y, Tb, Dy, Ho and Er)". Journal of Alloys and Compounds. 303–304. Elsevier BV: 223–227. doi:10.1016/s0925-8388(00)00635-6. ISSN0925-8388.
^Tsai, A. P.; Niikura, A.; Inoue, A.; Masumoto, T.; Nishida, Y.; Tsuda, K.; Tanaka, M. (1994). "Highly ordered structure of icosahedral quasicrystals in Zn-Mg-RE (RE ≡ rare earth metals) systems". Philosophical Magazine Letters. 70 (3). Informa UK Limited: 169–175. doi:10.1080/09500839408240971. ISSN0950-0839.