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- Publisher Website: 10.1103/PhysRevB.109.054305
- Scopus: eid_2-s2.0-85185399885
- WOS: WOS:001198615900003
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Article: Impact of strain-insensitive low-frequency phonon modes on lattice thermal transport in A 2 X B 6-type perovskites
| Title | Impact of strain-insensitive low-frequency phonon modes on lattice thermal transport in A 2 X B 6-type perovskites |
|---|---|
| Authors | |
| Issue Date | 14-Feb-2024 |
| Publisher | American Physical Society |
| Citation | Physical Review B, 2024, v. 109, n. 5 How to Cite? |
| Abstract | Substrate induces mechanical strain on perovskite devices, which can result in alterations to its lattice dynamics and thermal transport. Herein, we have performed a theoretical investigation on the anharmonic lattice dynamics and thermal property of perovskite Rb2SnBr6 and Cs2SnBr6 under strains using perturbation theory up to the fourth-order terms and the unified thermal transport theory. We demonstrate a pronounced hardening of low-frequency optical phonons as temperature increases, indicating strong lattice anharmonicity and the necessity of adopting temperature-dependent interatomic force constants in the lattice thermal conductivity (𝜅L) calculations. It is found that the low-lying optical phonon modes of Rb2SnBr6 are extremely soft and their phonon energies are almost strain independent, which ultimately lead to a lower 𝜅L and a weaker strain dependence than Cs2SnBr6. We further reveal that the strain dependence of these phonon modes in the A2𝑋𝐵6 -type perovskites weakens as their vibrational frequency decreases. This study deepens the understanding of lattice thermal transport in perovskites A2𝑋B6 and provides a perspective on the selection of materials that meet the expected thermal behaviors in practical applications. |
| Persistent Identifier | http://hdl.handle.net/10722/345901 |
| ISSN | 2023 Impact Factor: 3.2 2023 SCImago Journal Rankings: 1.345 |
| ISI Accession Number ID |
| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | Cheng, R | - |
| dc.contributor.author | Zeng, Z | - |
| dc.contributor.author | Wang, C | - |
| dc.contributor.author | Ouyang, N | - |
| dc.contributor.author | Chen, Y | - |
| dc.date.accessioned | 2024-09-04T07:06:21Z | - |
| dc.date.available | 2024-09-04T07:06:21Z | - |
| dc.date.issued | 2024-02-14 | - |
| dc.identifier.citation | Physical Review B, 2024, v. 109, n. 5 | - |
| dc.identifier.issn | 2469-9950 | - |
| dc.identifier.uri | http://hdl.handle.net/10722/345901 | - |
| dc.description.abstract | <p>Substrate induces mechanical strain on perovskite devices, which can result in alterations to its lattice dynamics and thermal transport. Herein, we have performed a theoretical investigation on the anharmonic lattice dynamics and thermal property of perovskite Rb2SnBr6 and Cs2SnBr6 under strains using perturbation theory up to the fourth-order terms and the unified thermal transport theory. We demonstrate a pronounced hardening of low-frequency optical phonons as temperature increases, indicating strong lattice anharmonicity and the necessity of adopting temperature-dependent interatomic force constants in the lattice thermal conductivity (𝜅L) calculations. It is found that the low-lying optical phonon modes of Rb2SnBr6 are extremely soft and their phonon energies are almost strain independent, which ultimately lead to a lower 𝜅L and a weaker strain dependence than Cs2SnBr6. We further reveal that the strain dependence of these phonon modes in the A2𝑋𝐵6 -type perovskites weakens as their vibrational frequency decreases. This study deepens the understanding of lattice thermal transport in perovskites A2𝑋B6 and provides a perspective on the selection of materials that meet the expected thermal behaviors in practical applications.<br></p> | - |
| dc.language | eng | - |
| dc.publisher | American Physical Society | - |
| dc.relation.ispartof | Physical Review B | - |
| dc.title | Impact of strain-insensitive low-frequency phonon modes on lattice thermal transport in A 2 X B 6-type perovskites | - |
| dc.type | Article | - |
| dc.identifier.doi | 10.1103/PhysRevB.109.054305 | - |
| dc.identifier.scopus | eid_2-s2.0-85185399885 | - |
| dc.identifier.volume | 109 | - |
| dc.identifier.issue | 5 | - |
| dc.identifier.eissn | 2469-9969 | - |
| dc.identifier.isi | WOS:001198615900003 | - |
| dc.identifier.issnl | 2469-9950 | - |
