2011
DOI: 10.1007/s11664-011-1607-z
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Heat Capacity Study on Anharmonicity in Ae8Ga16Ge30 (Ae = Sr and Ba)

Abstract: The heat capacity of single-crystalline samples of Sr 8 Ga 16 Ge 30 (SGG) and Ba 8 Ga 16 Ge 30 (BGG) clathrates was measured to investigate the anharmonicity of the encapsulated atoms. At low temperatures, BGG can be well described by a standard Debye model, and the C p /T 3 versus T plot can be fitted with two Einstein temperatures: h E1 = 42 K and h E2 = 74 K. On the other hand, SGG shows deviation from the Debye model. Moreover, neither the Einstein model nor the soft potential model (SPM) alone can fit the… Show more

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Cited by 13 publications
(14 citation statements)
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References 24 publications
(30 reference statements)
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“…The humps in C V /T 3 of type-I Ba 8 Ga 16 Sn 30 (β-BGS) and type-I Sr 8 Ga 16 Ge 30 appear around T ≃5 [K] (Avila et al, 2008;Suekuni et al, 2007Suekuni et al, , 2008aUmeo et al, 2005;Xu et al, 2011). See Fig.…”
Section: Excess Specific Heats Over Debye Phonons At Temperatures Of ...mentioning
confidence: 97%
“…The humps in C V /T 3 of type-I Ba 8 Ga 16 Sn 30 (β-BGS) and type-I Sr 8 Ga 16 Ge 30 appear around T ≃5 [K] (Avila et al, 2008;Suekuni et al, 2007Suekuni et al, , 2008aUmeo et al, 2005;Xu et al, 2011). See Fig.…”
Section: Excess Specific Heats Over Debye Phonons At Temperatures Of ...mentioning
confidence: 97%
“…Several others have recognized this and have attempted to provide evidence for these properties while others have modified the model to make the TLS and distribution more meaningful [11,24,50,51]. A major flaw in this theory is this lack of understanding the source and distribution of the TLSs.…”
mentioning
confidence: 99%
“…Typically, such excess specific heats due to guest "rattling" can be associated with the peak occurring in a temperature range whose center is normally 10-100 times smaller than the Debye temperature [37]. Previous reports identified the characteristic humps that were determined around T~5 K, in the case of Type-I β-Rb 8 Ga 16 Sn 30 (β-RGS) and Type-I Sr 8 Ga 16 Ge 30 [38][39][40][41][42][43] compounds. Our computational work presents this form of hump in the Type-II Rb 24 Ga 24 Sn 112 clathrate, owing primarily to two sorts of isotropic Einstein oscillators that originate from the 28 atom and 20 atom cages, respectively.…”
Section: Vibrtional and Thermal Properties Of Rb 24 Ga 24 Sn 112 And mentioning
confidence: 99%