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Here pressure is understood to be the excess pressure that results after subtraction of hydrostatic pressure induced by some conservative force, e.g., gravity. This excess pressure is therefore the pressure change due to dynamic effects.
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p does not contribute to the second integral in Eq. (5.4), but for the purposes at hand it is found convenient to retain the integral in its present form.
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Roman indices i, j, k, l have been used here, instead of the greek indices α, β, γ, δ Eq. (5.13), in order to avoid confusion with the scalars α and β in Eq. (6.1).
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The analysis used by Nunan and Keller, which allows for an explicit evaluation of the particles' angular velocity, cannot be straightforwardly applied to noncubic lattices as it relies greatly on cubic symmetries.
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