1995
DOI: 10.1007/bf01324522
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Thermodynamic properties of the spin-Peierls transition in CuGeO3

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Cited by 21 publications
(16 citation statements)
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“…30 Assuming α=500 cm −1 and α=250 cm −1 in the 1.55 eV-c-polarized and 3.14 eV-bpolarized configurations, 15 we can estimate δT=3.6 K and δT=1.8 K, respectively. While the ratio of the estimated temperature increase (3.6 K/1.8 K≃2), related to the difference in the absorbed density of energy, is compatible with measured ratio (23 K/14 K≃1.6), the discrepancy of the absolute values can be attributed to the fact that the energy absorbed by the electronic transitions is delivered to a subset of optical lattice modes, i.e.…”
Section: Discussionmentioning
confidence: 99%
“…30 Assuming α=500 cm −1 and α=250 cm −1 in the 1.55 eV-c-polarized and 3.14 eV-bpolarized configurations, 15 we can estimate δT=3.6 K and δT=1.8 K, respectively. While the ratio of the estimated temperature increase (3.6 K/1.8 K≃2), related to the difference in the absorbed density of energy, is compatible with measured ratio (23 K/14 K≃1.6), the discrepancy of the absolute values can be attributed to the fact that the energy absorbed by the electronic transitions is delivered to a subset of optical lattice modes, i.e.…”
Section: Discussionmentioning
confidence: 99%
“…Experimentally it is still an open question if a spin gap in the incommensurate phase exists. The T 3 contributions to the specific heat at low temperatures [37,38] are explained in terms of gapless "phasons" [39].…”
Section: Perturbations Of the Pure Systemmentioning
confidence: 99%
“…For most of the inorganic substances (in particular for CuGeO 3 ) which have spinspin couplings of the order of 100K, lattice vibrations dominate the specific heat and it is an unsolved problem to extract its magnetic part. As a first approximation 19 it was assumed for CuGeO 3 that it is sufficient to subtract the contribution of the phonons and consider the rest as the contribution of the spins. We show that such an approximation is not justified even in the simple case of dispersionless phonons.…”
Section: B Specific Heat Phonon Occupation Numbermentioning
confidence: 99%