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Title: Goldstone-like phonon modes in a (111)-strained perovskite

Abstract

Goldstone modes are massless particles resulting from spontaneous symmetry breaking. While such modes are found in elementary particle physics as well as in condensed-matter systems like superfluid helium, superconductors, and magnons, structural Goldstone modes are rare. Epitaxial strain in thin films can induce structures and properties not accessible in bulk and has been intensively studied for (001)-oriented perovskite oxides. In this work we predict Goldstone-like phonon modes in (111)-strained SrMnO3 by first-principles calculations. Under compressive strain the coupling between two in-plane rotational instabilities gives rise to a Mexican hat-shaped energy surface characteristic of a Goldstone mode. Conversely, large tensile strain induces in-plane polar instabilities with no directional preference, giving rise to a continuous polar ground state. Such phonon modes with U(1) symmetry could emulate structural condensed-matter Higgs modes. The mass of this Higgs boson, given by the shape of the Mexican hat energy surface, can be tuned by strain through proper choice of substrate.

Authors:
 [1];  [2];  [1];  [1];  [1];  [1]
  1. Norwegian Univ. of Science and Technology (NTNU), Trondheim (Norway)
  2. Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States); Univ. of California, Berkeley, CA (United States)
Publication Date:
Research Org.:
Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States)
Sponsoring Org.:
USDOE Office of Science (SC), Basic Energy Sciences (BES) (SC-22). Materials Sciences & Engineering Division; Research Council of Norway; Swiss National Science Foundation (SNSF); USDOE
OSTI Identifier:
1505516
Alternate Identifier(s):
OSTI ID: 1416632
Grant/Contract Number:  
AC02-05CH11231; AC02-05-CH11231
Resource Type:
Accepted Manuscript
Journal Name:
Physical Review Materials
Additional Journal Information:
Journal Volume: 2; Journal Issue: 1; Journal ID: ISSN 2475-9953
Publisher:
American Physical Society (APS)
Country of Publication:
United States
Language:
English
Subject:
75 CONDENSED MATTER PHYSICS, SUPERCONDUCTIVITY AND SUPERFLUIDITY

Citation Formats

Marthinsen, A., Griffin, S. M., Moreau, M., Grande, T., Tybell, T., and Selbach, S. M. Goldstone-like phonon modes in a (111)-strained perovskite. United States: N. p., 2018. Web. doi:10.1103/physrevmaterials.2.014404.
Marthinsen, A., Griffin, S. M., Moreau, M., Grande, T., Tybell, T., & Selbach, S. M. Goldstone-like phonon modes in a (111)-strained perovskite. United States. https://doi.org/10.1103/physrevmaterials.2.014404
Marthinsen, A., Griffin, S. M., Moreau, M., Grande, T., Tybell, T., and Selbach, S. M. Thu . "Goldstone-like phonon modes in a (111)-strained perovskite". United States. https://doi.org/10.1103/physrevmaterials.2.014404. https://www.osti.gov/servlets/purl/1505516.
@article{osti_1505516,
title = {Goldstone-like phonon modes in a (111)-strained perovskite},
author = {Marthinsen, A. and Griffin, S. M. and Moreau, M. and Grande, T. and Tybell, T. and Selbach, S. M.},
abstractNote = {Goldstone modes are massless particles resulting from spontaneous symmetry breaking. While such modes are found in elementary particle physics as well as in condensed-matter systems like superfluid helium, superconductors, and magnons, structural Goldstone modes are rare. Epitaxial strain in thin films can induce structures and properties not accessible in bulk and has been intensively studied for (001)-oriented perovskite oxides. In this work we predict Goldstone-like phonon modes in (111)-strained SrMnO3 by first-principles calculations. Under compressive strain the coupling between two in-plane rotational instabilities gives rise to a Mexican hat-shaped energy surface characteristic of a Goldstone mode. Conversely, large tensile strain induces in-plane polar instabilities with no directional preference, giving rise to a continuous polar ground state. Such phonon modes with U(1) symmetry could emulate structural condensed-matter Higgs modes. The mass of this Higgs boson, given by the shape of the Mexican hat energy surface, can be tuned by strain through proper choice of substrate.},
doi = {10.1103/physrevmaterials.2.014404},
journal = {Physical Review Materials},
number = 1,
volume = 2,
place = {United States},
year = {Thu Jan 11 00:00:00 EST 2018},
month = {Thu Jan 11 00:00:00 EST 2018}
}

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Works referencing / citing this record:

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