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Solid Phase Transitions in the Liquid Limit

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Abstract

We address the fundamental difference between solid-solid and liquid-liquid phase transitions within the Ericksen’s nonlinear elasticity paradigm. To highlight ideas, we consider the simplest nontrivial 2D problem and work with a prototypical two-phase Hadamard material which allows one to weaken the rigidity and explore the nature of solid-solid phase transitions in a “near-liquid” limit. In the language of calculus of variations we probe limits of quasiconvexity in an “almost liquid” solid by comparing the thresholds for cooperative (laminate based) and non-cooperative (inclusion based) nucleation. Using these two types of nucleation tests we obtain for our model material surprisingly tight two-sided bounds on the elastic binodal without directly computing the quasiconvex envelope.

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Notes

  1. In principle, our methodology is also applicable in 3D. In this paper we have chosen a 2D setting to make the ideas and techniques fully transparent and to be able to illustrate them graphically.

  2. Formula (3.2) only needs to hold in an arbitrary neighborhood of \([d_{1},d_{2}]\). The potential \(h(d)\) can be modified outside of that neighborhood arbitrarily, as long as \(h^{**}(d)=h(d)\) there. In particular, the singular behavior of \(h(d)\) as \(d\to 0^{+}\), required in nonlinear elasticity, can be easily assured.

  3. We use the notation ± to make two statements at the same time, one for the “+” sign, the other for the “−” sign. For example, our statement says that the matrix \(\boldsymbol{F}_{+}\) has two singular values \(\varepsilon _{0}\) and \(\varepsilon _{+}\) and the matrix \(\boldsymbol{F}_{-}\) has two singular values \(\varepsilon _{0}\) and \(\varepsilon _{-}\).

  4. Technically, at the W-points there could be other, not necessarily diagonal critical states, however, by continuity, the diagonal critical points would still deliver the global minimum of \(\Psi (\boldsymbol{F})\).

  5. This inequality is equivalent to \(|\mathrm {dev}(\boldsymbol{H})|^{2}\ge 0\), where \(2\mathrm {dev}(\boldsymbol{H})=\boldsymbol{H}+\boldsymbol{H}^{T}-(\mathrm {Tr}\,\boldsymbol{H})\boldsymbol{I}_{2}\).

  6. We can assume. without loss of generality, that \(h(d)\ge 0\) and \(h(d)=0\) only at \(d=d_{1}\) and \(d=d_{2}\).

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Funding

YG was supported by the National Science Foundation under Grant No. DMS-2005538. The work of LT was supported by the French grant ANR-10-IDEX-0001-02 PSL.

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Dedicated to the memory of Jerry Ericksen, a wizard

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Appendix:  Calculation of the Jump Set for Hadamard Materials

Appendix:  Calculation of the Jump Set for Hadamard Materials

Here we recall the calculation of the jump set from [27] for energies (3.1).

We start with the first equation in (2.3) expressing the kinematic compatibility of the deformation gradients \(\boldsymbol{F}_{+}\) and \(\boldsymbol{F}_{-}\). Taking the determinant of both sides we obtain

$$ d_{+}=d_{-}+\mathrm {cof}\boldsymbol{F}_{-}\boldsymbol{n}\cdot \boldsymbol{a},\quad d_{\pm}=\det \boldsymbol{F}_{\pm}. $$
(A.1)

Using the formula

$$ \boldsymbol{P}(\boldsymbol{F})=\mu \boldsymbol{F}+h'(\det \boldsymbol{F})\mathrm {cof}\boldsymbol{F}$$

for the Piola–Kirchhoff stress we compute

$$ \lbrack \!\lbrack \boldsymbol{P}\rbrack \!\rbrack \boldsymbol{n}=\mu \boldsymbol{a}+\lbrack \!\lbrack h' \rbrack \!\rbrack \mathrm {cof}\boldsymbol{F}_{-}\boldsymbol{n}, $$

where we have used the well-known relation \(\mathrm {cof}(\boldsymbol{F}_{-}+\boldsymbol{a}\otimes \boldsymbol{n})\boldsymbol{n}=(\mathrm {cof}\boldsymbol{F}_{-})\boldsymbol{n}\). Similarly,

$$ \lbrack \!\lbrack \boldsymbol{P}\rbrack \!\rbrack ^{T}\boldsymbol{a}=\mu |\boldsymbol{a}|^{2}\boldsymbol{n}+\lbrack \!\lbrack h' \rbrack \!\rbrack \mathrm {cof}\boldsymbol{F}_{-}^{T}\boldsymbol{a}. $$

Thus, the second and the third equations in (2.3) become

$$ \boldsymbol{a}=-\frac{\lbrack \!\lbrack h' \rbrack \!\rbrack }{\mu} \mathrm {cof}\boldsymbol{F}_{-}\boldsymbol{n},\qquad \lbrack \!\lbrack h' \rbrack \!\rbrack ^{2} \mathrm {cof}(\boldsymbol{C}_{-})\boldsymbol{n}=\mu ^{2}|\boldsymbol{a}|^{2}\boldsymbol{n}, $$
(A.2)

where \(\boldsymbol{C}_{\pm}=\boldsymbol{F}_{\pm}^{T}\boldsymbol{F}_{\pm}\) is the Cauchy–Green strain tensor. We conclude that \(\boldsymbol{n}\) must be an eigenvector of \(\boldsymbol{C}_{-}\). Equations (A.2) permit us to find a relation between the two Cauchy–Green tensors \(\boldsymbol{C}_{\pm}\). Using the kinematic compatibility equation (2.3)1 we compute

$$ \boldsymbol{C}_{+}=\boldsymbol{C}_{-}+\boldsymbol{F}_{-}^{T}\boldsymbol{a}\otimes \boldsymbol{n}+\boldsymbol{n}\otimes \boldsymbol{F}_{-}^{T} \boldsymbol{a}+|\boldsymbol{a}|^{2} \boldsymbol{n}\otimes \boldsymbol{n}. $$

Applying \(\boldsymbol{F}_{-}^{T}\) to the first equation in (A.2) we obtain \(\boldsymbol{F}_{-}^{T}\boldsymbol{a}=-(\lbrack \!\lbrack h' \rbrack \!\rbrack /\mu )d_{-}\boldsymbol{n}\), so that

$$ \lbrack \!\lbrack \boldsymbol{C}\rbrack \!\rbrack =\left (|\boldsymbol{a}|^{2}-\frac{2\lbrack \!\lbrack h' \rbrack \!\rbrack d_{-}}{\mu}\right ) \boldsymbol{n}\otimes \boldsymbol{n}. $$
(A.3)

It follows that the Cauchy–Green tensors \(\boldsymbol{C}_{+}\) and \(\boldsymbol{C}_{-}\) are simultaneously diagonalizable, since, by (A.2) \(\boldsymbol{n}\) is an eigenvector of \(\boldsymbol{C}_{-}\). According to equation (A.3) symmetric matrices \(\boldsymbol{C}_{+}\) and \(\boldsymbol{C}_{-}\) have the same pair of mutually orthogonal eigenvectors \(\boldsymbol{n}\) and \(\boldsymbol{n}^{\perp}\) with the same eigenvalues corresponding to \(\boldsymbol{n}^{\perp}\). Hence, singular values of \(\boldsymbol{F}_{\pm}\) would be \((\varepsilon _{\pm}, \varepsilon _{0})\), the first one corresponding to the eigenvector \(\boldsymbol{n}\) of \(\boldsymbol{C}_{\pm}\). Substituting the first equation in (A.2) into (A.1) we obtain

$$ d_{+}=d_{-}-\frac{\lbrack \!\lbrack h' \rbrack \!\rbrack }{\mu} \mathrm {cof}\boldsymbol{C}_{-}\boldsymbol{n}\cdot \boldsymbol{n}=d_{-}- \frac{\lbrack \!\lbrack h' \rbrack \!\rbrack d_{-}^{2}}{\mu \varepsilon _{-}^{2}}, $$

which can be written in the more symmetric form as

$$ \mu \frac{\lbrack \!\lbrack d \rbrack \!\rbrack }{\lbrack \!\lbrack h' \rbrack \!\rbrack }=-\varepsilon _{0}^{2}=- \frac{d_{\pm}^{2}}{\varepsilon _{\pm}^{2}}. $$
(A.4)

This will be the equation for the jump set, when we determine \(d_{+}\) as a function of \(d_{-}\) from the Maxwell relation (the last equation in (2.3), which hasn’t been used so far). It is well-known that the Maxwell relation does not change if we add any quadratic function of \(\boldsymbol{F}\) to the energy. Thus, the term \(\mu |\boldsymbol{F}|^{2}/2\) can be disregarded and the Maxwell relation becomes

Recalling that due to (A.1) \((\mathrm {cof}\boldsymbol{F}_{+})\boldsymbol{n}\cdot \boldsymbol{a}=(\mathrm {cof}\boldsymbol{F}_{-})\boldsymbol{n}\cdot \boldsymbol{a}=\lbrack \!\lbrack d \rbrack \!\rbrack \) we obtain

(A.5)

Equation (A.5) has a geometric meaning. It says that the secant line joining \((d_{-},h'(d_{-}))\) and \((d_{-},h'(d_{-}))\) together with the graph of \(h'(d)\) bound two regions of equal areas. For a double-well shaped potential \(h(d)\) there exists a single interval \((d_{1},d_{2})\) on which \(h(d)\) differs from its convex hull, which on \((d_{1},d_{2})\) agrees with the common tangent line at \(d_{1}\) and \(d_{2}\) to the graph of \(h(d)\). In terms of \(h'(d)\) this double-tangency can also be interpreted geometrically as the horizontal “Maxwell line” with the equal area property. In that case there exist \(d_{0}\in (d_{1},d_{2})\), such that for any \(d_{-}\in (d_{1},d_{0})\) there is a unique \(d_{+}\in (d_{0},d_{2})\) satisfying (A.5). In other words, for every \(d_{-}\in (d_{1},d_{0})\) there is a unique \(d_{+}=D(d_{-})\) with equal area property. (By continuity we can set \(D(d_{0})=d_{0}\).) Regarding the function \(D(d)\) as known, equation (A.4) provides the explicit description of the jump set in terms of the singular values of \(\boldsymbol{F}_{\pm}\).

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Grabovsky, Y., Truskinovsky, L. Solid Phase Transitions in the Liquid Limit. J Elast (2023). https://doi.org/10.1007/s10659-023-10022-z

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