Proposition 11.2.10.4793125897B2 For $u\in \mathcal H_\omega $ and $v\in C^\infty (X,\mathbb R)$, put $\Omega _ t=(\omega +t\mathrm{dd}^{\mathrm{c}}u)^{n-1}$ for $0\leq t\leq 1$. Then
91AE93E20D38
11.2.11
AEF022344DD6For the Hermitian background $\theta =\omega $, the functional (11.2.7) integrates $\alpha $ along the segment from $0$ to $u\in \mathcal H_\omega $. When $\omega $ is not closed, the derivative of $E_\omega $ differs from $\alpha $ by the terms produced when integration by parts differentiates the background powers. Computing this difference gives the Euler equation of $E_\omega $ even when no primitive exists.
Proposition 11.2.10.4793125897B2 For $u\in \mathcal H_\omega $ and $v\in C^\infty (X,\mathbb R)$, put $\Omega _ t=(\omega +t\mathrm{dd}^{\mathrm{c}}u)^{n-1}$ for $0\leq t\leq 1$. Then
91AE93E20D38
11.2.11
Proof. Differentiating the radial integral in (11.2.7) in the direction $v$ gives
On the other hand,
The terms without a factor $nt$ cancel in the difference, leaving
The second equality is lemma 11.1.2. Expanding the last parenthesis by the product rule in the proof of lemma 11.2.2 gives (11.2.11). When $n=1$, one has $\Omega _ t=1$ and the right-hand side vanishes. $\square$
Proposition 11.2.12.0009683E4137 If $n=2$, then every $u\in \mathcal H_\omega $ satisfies
For every smooth real direction $v$, its differential satisfies
173E9E78941E
11.2.13
Proof. Expanding the radial integral gives the first identity. For $n=2$, one has $\Omega _ t=\omega +t\mathrm{dd}^{\mathrm{c}}u$, and since $\mathrm d$ and $\mathrm d^{\mathrm c}$ annihilate $\mathrm{dd}^{\mathrm{c}}u$, the derivatives $\mathrm d\Omega _ t$, $\mathrm d^{\mathrm c}\Omega _ t$ and $\mathrm{dd}^{\mathrm{c}}\Omega _ t$ are those of $\omega $. Formula (11.2.11) and $2\int _0^1t\, \mathrm dt=1$ give the second identity. $\square$
Consequently, if $n=2$ and $\mu $ is a fixed smooth real $(2,2)$-form on $X$, a critical point $u\in \mathcal H_\omega $ of the functional $E_\omega (u)-\int _ Xu\, \mu $ satisfies
rather than the Monge–Ampère equation $\omega _ u^2=\mu $. On a Gauduchon surface the term $u\mathrm{dd}^{\mathrm{c}}\omega $ vanishes, but the first-order torsion terms can persist. The radial Euler equation can therefore differ from the Monge–Ampère equation even when the total mass is invariant.
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