Bismuth is one of the rare materials in which second sound has been experimentally observed. Our exact calculations of thermal transport with the Boltzmann equation predict the occurrence of this Poiseuille phonon flow between approximate to 1.5 and approximate to 3.5 K, in a sample size of 3.86 and 9.06 mm, consistent with the experimental observations. Hydrodynamic heat flow characteristics are given for any temperature: heat wave propagation length, drift velocity, and Knudsen number. We discuss a gedanken experiment allowing us to assess the presence of a hydrodynamic regime in any bulk material.

Hydrodynamic heat transport regime in bismuth: a theoretical viewpoint / Markov, Maxime; Sjakste, Jelena; Barbarino, Giuliana; Fugallo, Giorgia; Paulatto, Lorenzo; Lazzeri, Michele; Mauri, Francesco; Francesco and, Vast; Nathalie,. - In: PHYSICAL REVIEW LETTERS. - ISSN 1092-0145. - 120:7(2018). [10.1103/PhysRevLett.120.075901]

Hydrodynamic heat transport regime in bismuth: a theoretical viewpoint

Mauri;
2018

Abstract

Bismuth is one of the rare materials in which second sound has been experimentally observed. Our exact calculations of thermal transport with the Boltzmann equation predict the occurrence of this Poiseuille phonon flow between approximate to 1.5 and approximate to 3.5 K, in a sample size of 3.86 and 9.06 mm, consistent with the experimental observations. Hydrodynamic heat flow characteristics are given for any temperature: heat wave propagation length, drift velocity, and Knudsen number. We discuss a gedanken experiment allowing us to assess the presence of a hydrodynamic regime in any bulk material.
2018
Phonon; thermal transport; first princliples calculations
01 Pubblicazione su rivista::01a Articolo in rivista
Hydrodynamic heat transport regime in bismuth: a theoretical viewpoint / Markov, Maxime; Sjakste, Jelena; Barbarino, Giuliana; Fugallo, Giorgia; Paulatto, Lorenzo; Lazzeri, Michele; Mauri, Francesco; Francesco and, Vast; Nathalie,. - In: PHYSICAL REVIEW LETTERS. - ISSN 1092-0145. - 120:7(2018). [10.1103/PhysRevLett.120.075901]
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11573/1159867
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