2011
DOI: 10.1103/physrevlett.107.207202
|View full text |Cite
|
Sign up to set email alerts
|

Response of Acoustic Phonons to Charge and Orbital Order in the 50% Doped Bilayer ManganiteLaSr2Mn2O7

Abstract: We report an inelastic neutron scattering study of acoustic phonons in the charge and orbitally ordered bilayer manganite LaSr(2)Mn(2)O(7). For excitation energies less than 15 meV, we observe an abrupt increase (decrease) of the phonon energies (linewidths) of a transverse acoustic phonon branch at q = (h, h, 0), h ≤ 0.3, upon entering the low temperature charge and orbital ordered state (T(COO) = 225 K). This indicates a reduced electron-phonon coupling due to a decrease of electronic states at the Fermi lev… Show more

Help me understand this report
View preprint versions

Search citation statements

Order By: Relevance

Paper Sections

Select...
2
1
1

Citation Types

3
6
0

Year Published

2014
2014
2022
2022

Publication Types

Select...
6
1
1

Relationship

0
8

Authors

Journals

citations
Cited by 11 publications
(9 citation statements)
references
References 38 publications
3
6
0
Order By: Relevance
“…It is interesting to compare the results in MgV 2 O 4 to metallic systems with acoustic instabilities. Our results show similarities to the measurements by F. Weber et al 71 who determined the dispersion of the TA-phonons in a metallic manganite. In this material, a charge and orbital ordering (COO) sets in at low temperatures.…”
Section: Discussionsupporting
confidence: 91%
See 1 more Smart Citation
“…It is interesting to compare the results in MgV 2 O 4 to metallic systems with acoustic instabilities. Our results show similarities to the measurements by F. Weber et al 71 who determined the dispersion of the TA-phonons in a metallic manganite. In this material, a charge and orbital ordering (COO) sets in at low temperatures.…”
Section: Discussionsupporting
confidence: 91%
“…In this material, a charge and orbital ordering (COO) sets in at low temperatures. Above T COO , F. Weber et al 71 report a softening of the TA phonon at q = 1 4 1 4 0 by ∆E ≈ 0.25 meV accompanied by an increase in linewidth ∆Γ HW HM ≈ 0.25 meV. Similar anomalies have been reported in other metallic manganites on decreasing temperature.…”
Section: Discussionsupporting
confidence: 65%
“…2(b) is given by v s d −1 where d is obtained from the nominal layer thicknesses (estimated from x-ray reflectivity measurements) and v s = 7 17 v s,YBCO + 10 17 v manganite is the weighted average of the c-axis speed of sound in the two materials (here we are using the most common 7 nm YBCO layer and 10 nm manganite layer thicknesses) 21 . The value of v s is 4750 ± 200 m.s −1 as determined from the bulk-moduli and densities 34,35 , but similar values are obtained from other measurements of the speed of sound [36][37][38][39] .The width of the line in Fig. 2(b) comes from the uncertainty in v s for the individual YBCO and manganite layers.…”
supporting
confidence: 79%
“…2(b) is given by v s d −1 , where d is obtained from the nominal layer thicknesses (estimated from x-ray reflectivity measurements) and v s = 7 17 v s,YBCO + 10 17 v s,manganite is the weighted average of the caxis speed of sound in the two materials (here we are using the most common 7-nm YBCO layer and 10-nm manganite layer thicknesses) [24]. The value of v s is 4750 ± 200 m s −1 as determined from the bulk moduli and densities [39,40], but similar values are obtained from other measurements of the speed of sound [41][42][43][44]. The width of the line in Fig.…”
Section: B Sample Dependencementioning
confidence: 65%