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Binary rare earth hexaborides (REB6) have different rare earth elements with different valence electron distributions, which lead to different strange physical properties and different emission properties. However, in the electron emission properties, whether PrB6, NdB6, SmB6 and GdB6 all have excellent emission properties remains to be further studied, and the physical mechanism affecting their emission properties needs investigating. In this paper, the electronic structures, work functions of typical binary single crystal REB6 (LaB6, CeB6, PrB6, NdB6, SmB6, GdB6) are studied by first principles calculations. The single crystal REB6 are prepared by optical zone melting method, and their thermionic electron emission properties are tested experimentally. The theoretical calculation results show that the typical binary REB6 have large densities of states near the Fermi level. The d-orbitals with broad distributions in conduction bands are beneficial to electron emission. The localized f-orbital electrons in valence bands are not conducive to their electron emission. The theoretical calculations of work functions of typical binary single crystal REB6 (100) surface are consistent with the analyses of their electronic structures. The theoretical calculation values of work functions are ordered as GdB6 (2.27 eV) < CeB6 (2.36 eV) < LaB6 (2.40 eV) < PrB6 (2.58 eV) < SmB6 (2.63 eV) < NdB6 (2.91 eV). The experimental test results of thermionic electron emission of single crystal show that the experimental thermionic electron properties are consistent with the theoretical ones. The LaB6 and CeB6 both have good thermionic and field emission properties, and the GdB6 has excellent field emission properties.
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Keywords:
- single crystal REB6 /
- first principles /
- work function /
- thermionic emission
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Google Scholar
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Google Scholar
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Google Scholar
Bao L H, Zhang J X, Zhou S L, Zhang N 2011 Acta Phys. Sin. 60 106501
Google Scholar
[4] Zhou N, Zhang W, Zhang X, Liu H, Lu Q, Xiao Y, Liu Y, Jin S, Liao N 2021 Vacuum 184 109929
Google Scholar
[5] Hoyoung J, Friemel G, Ollivier J, Dukhnenko A V, N Yu S, Filipov V B, Keimer B, Inosov D S 2014 Nat. Mater. 13 682
Google Scholar
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Google Scholar
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Google Scholar
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Google Scholar
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Google Scholar
[10] Paul S, Dohun K, Michael S F, Johnpierre P 2015 Phys. Rev. Lett. 114 096601
Google Scholar
[11] Sundermann M, Yavaş H, Chen K, Kim D J, Fisk Z, Kasinathan D, Haverkort M W, Thalmeier P, Severing A, Tjeng L H 2018 Phys. Rev. Lett. 120 016402
Google Scholar
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Google Scholar
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Google Scholar
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Google Scholar
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Google Scholar
[19] Lu F, Zhao J Z, Weng H M, Fang Z, Dai X 2013 Phys. Rev. Lett. 110 096401
Google Scholar
[20] Qin X, Liu X, Huang W, Bettinelli M, Liu X 2017 Chem. Rev. 117 4488
Google Scholar
[21] Elkelany K E, Ravoux C, Desmarais J K, Cortona P, Pan Y, Tse J S, Erba A 2018 Phys. Rev. B 97 245118
Google Scholar
[22] 包黎红, 那仁格日乐, 特古斯, 张忻, 张久兴 2013 62 196105
Google Scholar
Bao L H, Narengerile, Tegus O, Zhang X, Zhang J X 2013 Acta Phys. Sin. 62 196105
Google Scholar
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Google Scholar
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Google Scholar
Liu H L, Zhang X, Wang Y, Xiao Y X, Zhang J X 2018 Acta Phys. Sin. 67 048101
Google Scholar
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