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Random harmonic maps into spheres

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abstract

Let $S$ be a punctured Riemann surface with Euler characteristic $\chi(S)<0$. For any unitary representation $\rho: \pi_1(S) \to U(N)$, we introduce its renormalized energy and its harmonic representatives, which are equivariant harmonic maps from the universal cover of $S$ to the unit sphere in $\mathbb{C}^N$. Our main result is that if a sequence of unitary representations $\rho_j$ strongly converges, then their renormalized energies converge to $\frac{\pi}{4}|\chi(S)|$ and the shape of their harmonic representatives converges to a unique rescaled hyperbolic metric. Combining this statement with examples of strongly converging representations provided by random matrix theory, we derive the following applications. (1) If $\pi_1(S)$ is a free group, then for a random $\rho: \pi_1(S) \to U(N)$, the shape of its harmonic representatives concentrates around a rescaled hyperbolic metric with high probability as $N\to \infty$. (2) For any closed hyperbolic surface, a finite covering admits a harmonic immersion into some Euclidean unit sphere, which is almost isometric after rescaling. (3) There are closed, branched, minimal surfaces $\mathfrak{S}_j$ in some Euclidean unit spheres such that $\mathfrak{S}_j$ Benjamini-Schramm converges to a rescaled hyperbolic plane as $j\to \infty$, and the Gaussian curvature $K_j$ of $\mathfrak{S}_j$ satisfies $\lim_{j\to \infty} \frac{1}{\mathrm{Area}(\mathfrak{S}_j)}\int_{\mathfrak{S}_j} |K_j+8|=0.$

fields

math.SP 1

years

2026 1

verdicts

ACCEPT 1

representative citing papers

Bass notes of random hyperbolic surfaces of large genus

math.SP · 2026-07-07 · accept · novelty 2.0

A survey of recent results proving that random hyperbolic surfaces of large genus have near-optimal spectral gaps, after Hide–Magee, Anantharaman–Monk, and Hide–Macera–Thomas.

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  • Bass notes of random hyperbolic surfaces of large genus math.SP · 2026-07-07 · accept · none · ref 44 · internal anchor

    A survey of recent results proving that random hyperbolic surfaces of large genus have near-optimal spectral gaps, after Hide–Magee, Anantharaman–Monk, and Hide–Macera–Thomas.