$30 off During Our Annual Pro Sale. View Details »

Temperature and pressure effects on phase stability from theoretical modelling: application to the tin-sulphide phase space

Temperature and pressure effects on phase stability from theoretical modelling: application to the tin-sulphide phase space

Presented at the 29th General Conference of the Condensed Matter Division of the European Physical Society on Materials Chemistry (CMD29).

Jonathan Skelton

August 23, 2022
Tweet

More Decks by Jonathan Skelton

Other Decks in Science

Transcript

  1. Ioanna Pallikara, Joseph M. Flitcroft and Jonathan M. Skelton
    Department of Chemistry, University of Manchester
    ([email protected])
    Temperature and pressure effects on phase stability
    from theoretical modelling:
    application to the tin-sulphide phase space

    View Slide

  2. The tin chalcogenides
    CMD29, 23rd August 2022 | Slide 2
    Dr Jonathan M. Skelton

    View Slide

  3. The tin sulphide phase space
    CMD29, 23rd August 2022 | Slide 3
    Dr Jonathan M. Skelton
    Rocksalt
    Pnma Cmcm 𝜋-cubic
    SnS2
    Sn2
    S3
    Zincblende

    View Slide

  4. “Cubic” tin sulphide
    CMD29, 23rd August 2022 | Slide 4
    Dr Jonathan M. Skelton
    1967
    2006
    2012
    2015
    2016
    2017
    Initial identification of rocksalt SnS by epitaxial growth
    First report of tetrahedral zincblende nanoparticles
    Modelling suggests ZB SnS is energetically and dynamically unstable
    Electron diffraction suggests ZB nanoparticles are a new phase in the
    cubic P21
    3 spacegroup (𝜋-SnS)
    Another report of ZB SnS
    Atomic structure of 𝜋-SnS solved by X-ray diffraction
    Modelling confirms 𝜋-SnS is energetically metastable and dynamically
    stable

    View Slide

  5. Energetics I: convex hull
    CMD29, 23rd August 2022 | Slide 5
    Dr Jonathan M. Skelton
    J. M. Skelton et al., J. Phys. Chem. C 121 (12), 6446 (2017)

    View Slide

  6. Structural dynamics of solids
    CMD29, 23rd August 2022 | Slide 6
    Dr Jonathan M. Skelton
    Consider the Taylor expansion of the crystal potential energy:
    The second-order force constants 𝚽!,!! can be used to derive the phonon modes
    within the harmonic approximation
    𝜑 𝒖 = Φ#
    + (
    !
    (
    $
    Φ!
    $𝑢!
    $ +
    1
    2
    (
    !,!!
    (
    $,%
    Φ
    !,!!
    $% 𝑢!
    $𝑢
    !!
    % +
    1
    3!
    (
    !,!!,!!!
    (
    $,%,&
    Φ
    !,!!,!!!
    $%& 𝑢!
    $𝑢
    !!
    % 𝑢
    !!!
    & + ⋯
    Third- and higher-order force constants e.g. 𝚽!,!!,!!! capture various forms of
    anharmonicity and can be used to build on the basic HA e.g. for a perturbative
    treatment of phonon lifetimes
    Lattice energy
    𝑈'())
    Atomic forces (vanish
    at equilibrium)
    Harmonic approx. Anharmonicity

    View Slide

  7. Dynamical stability
    CMD29, 23rd August 2022 | Slide 7
    Dr Jonathan M. Skelton
    U(Q)
    Q
    Real PES HA
    U(Q)
    Q
    Real PES HA
    𝑈 𝑄 =
    1
    2
    𝜇𝜔*𝑄*

    View Slide

  8. Dynamical stability
    CMD29, 23rd August 2022 | Slide 8
    Dr Jonathan M. Skelton
    J. M. Skelton et al., J. Phys. Chem. C 121 (12), 6446 (2017)

    View Slide

  9. Dynamical stability
    CMD29, 23rd August 2022 | Slide 9
    Dr Jonathan M. Skelton
    J. M. Skelton et al., J. Phys. Chem. C 121 (12), 6446 (2017)

    View Slide

  10. Imaginary modes in Cmcm SnX
    CMD29, 23rd August 2022 | Slide 10
    Dr Jonathan M. Skelton
    J. M. Skelton et al., Phys. Rev. Lett 117, 075502 (2016)

    View Slide

  11. Imaginary modes in Cmcm SnX
    CMD29, 23rd August 2022 | Slide 11
    Dr Jonathan M. Skelton
    J. M. Skelton et al., Phys. Rev. Lett 117, 075502 (2016)

    View Slide

  12. RS and ZB SnS under pressure
    CMD29, 23rd August 2022 | Slide 12
    Dr Jonathan M. Skelton
    J. M. Skelton et al., J. Phys. Chem. C 121 (12), 6446 (2017)

    View Slide

  13. Statistical thermodynamics I
    CMD29, 23rd August 2022 | Slide 13
    Dr Jonathan M. Skelton
    Using the harmonic approximation, we can calculate the Helmholtz free energy
    𝐴(𝑇):
    𝐴 𝑇 = 𝑈'()) + 𝐴+,- 𝑇 = 𝑈'()) + 𝑈+,-(𝑇) − 𝑇𝑆+,-(𝑇)
    The 𝐴+,- 𝑇 term is calculated using the bridge relation from the partition function
    𝑍+,- 𝑇 :
    𝑍+,-
    𝑇 = :
    𝐪/
    exp[− ⁄
    ℏ𝜔𝐪/ 2𝑘0𝑇]
    1 − exp[− ⁄
    ℏ𝜔𝐪/ 𝑘0𝑇]
    𝐴+,-
    𝑇 = −
    1
    𝑁
    𝑘0
    𝑇ln 𝑍+,-
    𝑇 =
    1
    𝑁
    1
    2
    (
    𝐪/
    ℏ𝜔𝐪/
    + 𝑘0
    𝑇 (
    𝐪/
    ln 1 − exp − ⁄
    ℏ𝜔𝐪/
    𝑘0
    𝑇
    In typical DFT calculations the 𝑈'())
    is temperature independent - the phonon
    frequencies allows the temperature-dependent Helmholtz energy to be
    calculated

    View Slide

  14. Energetics II: Helmholtz energy
    CMD29, 23rd August 2022 | Slide 14
    Dr Jonathan M. Skelton
    J. M. Skelton et al., J. Phys. Chem. C 121 (12), 6446 (2017)

    View Slide

  15. Statistical thermodynamics II
    CMD29, 23rd August 2022 | Slide 15
    Dr Jonathan M. Skelton
    Using the harmonic approximation, we can calculate the Helmholtz free energy
    𝐴(𝑇):
    𝐴(𝑇) = 𝑈'()) + 𝑈+,-(𝑇) − 𝑇𝑆+,-(𝑇)
    If we also take into account the volume dependence of 𝑈'())
    and the phonon
    frequencies, we can calculate the Gibbs free energy 𝐺(𝑇) (the quasi-harmonic
    approximation):
    𝐺 𝑇 = min
    1
    𝐴 𝑇; 𝑉 + 𝑝𝑉 = min
    1
    𝑈'())
    (𝑉) + 𝑈+,-
    (𝑇; 𝑉) − 𝑇𝑆+,-
    (𝑇; 𝑉) + 𝑝𝑉
    This is typically achieved by minimising a free-energy equation of state, which
    yields other properties such as 𝑉(𝑇) and 𝐵(𝑇) alongside 𝐺(𝑇)
    (𝐺 is arguably a more experimentally-relevant quantity, and we can also explore
    the effect of pressure through the 𝑝𝑉 term.)

    View Slide

  16. Energetics III: Gibbs vs Helmholtz
    CMD29, 23rd August 2022 | Slide 16
    Dr Jonathan M. Skelton
    I. Pallikara and J. M. Skelton, Phys. Chem. Chem. Phys. 23, 19219 (2021)

    View Slide

  17. Energetics IV: p/T phase diagram
    CMD29, 23rd August 2022 | Slide 17
    Dr Jonathan M. Skelton
    I. Pallikara and J. M. Skelton, Phys. Chem. Chem. Phys. 23, 19219 (2021)

    View Slide

  18. Cmcm SnS under pressure
    CMD29, 23rd August 2022 | Slide 18
    Dr Jonathan M. Skelton
    I. Pallikara and J. M. Skelton, Phys. Chem. Chem. Phys. 23, 19219 (2021)

    View Slide

  19. RS SnS -> 𝝅 SnS transition barrier
    CMD29, 23rd August 2022 | Slide 19
    Dr Jonathan M. Skelton
    I. Pallikara and J. M. Skelton, Phys. Chem. Chem. Phys. 23, 19219 (2021)

    View Slide

  20. Energetics IV: p/T phase diagram
    CMD29, 23rd August 2022 | Slide 20
    Dr Jonathan M. Skelton
    I. Pallikara and J. M. Skelton, Phys. Chem. Chem. Phys. 23, 19219 (2021)

    View Slide

  21. Application: thermoelectrics
    CMD29, 23rd August 2022 | Slide 21
    Dr Jonathan M. Skelton
    G. Tan et al., Chem. Rev. 116 (19), 12123 (2016)
    𝑍𝑇 =
    𝑆!𝜎
    𝜅"#" + 𝜅#$%
    𝑇
    𝑆 - Seebeck coefficient
    𝜎 - electrical conductivity
    𝜅"#"
    - electronic thermal conductivity
    𝜅#$%
    - lattice thermal conductivity

    View Slide

  22. Application: thermoelectrics
    CMD29, 23rd August 2022 | Slide 22
    Dr Jonathan M. Skelton
    J. M. Flitcroft et al., Solids 3 (1), 155 (2022)

    View Slide

  23. Application: thermoelectrics
    CMD29, 23rd August 2022 | Slide 23
    Dr Jonathan M. Skelton
    n
    [cm-3]
    T
    [K] 𝒁𝑻
    𝝈
    [S cm-1]
    𝑺
    [𝝁V K-1]
    𝑺𝟐𝝈
    [mW m-1 K-2]
    𝜿𝐭𝐨𝐭
    [W m-1 K-1]
    SnS (Pnma) 4.64 × 10-19 1000 1.75 252 272 1.87 1.07
    SnS (RS, Eq.) 1020 720 2.99 885 297 7.84 1.70
    SnS (RS, 13 GPa) 1020 800 1.48 999 303 9.19 4.33
    SnSe (Pnma) 4.64 × 10-19 1000 2.81 348 274 2.62 0.93
    SnSe (RS, Eq.) 1020 800 2.60 1196 302 10.90 3.02
    J. M. Flitcroft et al., Solids 3 (1), 155 (2022)

    View Slide

  24. Summary
    CMD29, 23rd August 2022 | Slide 24
    Dr Jonathan M. Skelton
    The tin sulphides Snx
    Sy
    have a rich phase space with five known or proposed SnS
    phases plus SnS2
    and Sn2
    S3
    Helmholtz and Gibbs free energy calculations using the HA/QHA predict the
    observed soft-mode phase transition between the Pnma and Cmcm phases
    Both RS and ZB SnS are dynamically unstable, but RS SnS can be stabilised under
    compression e.g. by epitaxial growth
    Sn2
    S3
    is predicted to be unstable with respect to disproportionation based on its
    lattice energy, but is stabilised at finite temperature by vibrational entropy
    The QHA 𝑝/𝑇 phase diagram of SnS features only the Pnma and Cmcm phases;
    pressure shifts the Pnma ↔ Cmcm transition to lower 𝑇, and above ~11-12 GPa the
    Cmcm phase becomes both energetically and dynamically stable
    If synthetically accessible, the RS phase of SnS has the potential to show superior
    thermoelectric properties to the Pnma phase

    View Slide

  25. Acknowledgements
    CMD29, 23rd August 2022 | Slide 25
    Dr Jonathan M. Skelton

    View Slide

  26. https://bit.ly/3AAaTBk
    These slides are available on Speaker Deck:

    View Slide