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The Infinite Dyson Brownian Motion with $β=2$ Does Not Have a Spectral Gap

Kohei Suzuki

TL;DR

This work addresses whether the unlabelled infinite Dyson Brownian motion at inverse temperature $\beta=2$ admits a spectral gap for its Dirichlet form. The authors construct a one-parameter family of linear statistics $U_\sigma$ from the $\mathsf{sine}_2$ point process via $u_\sigma(x)=x e^{-x^2/(2\sigma^2)}$ and compute both the variance $\mathrm{Var}(U_\sigma)$ using the intensity and two-point correlation $\rho^{(2)}$, and an upper bound for the energy $\mathcal E(U_\sigma)$. They show $\mathrm{Var}(U_\sigma) \ge \frac{\sigma^2}{4\pi}\left(1-e^{-4\pi^2\sigma^2}\right)$ while $\mathcal E(U_\sigma) \le \sqrt{\pi}\,\sigma + \frac{3\sqrt{\pi}}{4}\,\sigma$, leading to $\inf_{F} \frac{\mathcal E(F)}{\mathrm{Var}(F)} \le \frac{\mathcal E(U_\sigma)}{\mathrm{Var}(U_\sigma)} \to 0$ as $\sigma\to\infty$. This yields a negative result: no spectral gap for any closed extension of the Dirichlet form when $\beta=2$. The concluding discussion connects this to variance growth of linear statistics and hyperuniformity, suggesting that a spectral gap could only arise under substantially slower variance growth than in the Poisson or sine$_2$ cases.

Abstract

We prove that the Dirichlet forms associated with the unlabelled infinite Dyson Brownian motion with the inverse temperature $β=2$ do not have a spectral gap.

The Infinite Dyson Brownian Motion with $β=2$ Does Not Have a Spectral Gap

TL;DR

This work addresses whether the unlabelled infinite Dyson Brownian motion at inverse temperature admits a spectral gap for its Dirichlet form. The authors construct a one-parameter family of linear statistics from the point process via and compute both the variance using the intensity and two-point correlation , and an upper bound for the energy . They show while , leading to as . This yields a negative result: no spectral gap for any closed extension of the Dirichlet form when . The concluding discussion connects this to variance growth of linear statistics and hyperuniformity, suggesting that a spectral gap could only arise under substantially slower variance growth than in the Poisson or sine cases.

Abstract

We prove that the Dirichlet forms associated with the unlabelled infinite Dyson Brownian motion with the inverse temperature do not have a spectral gap.
Paper Structure (2 sections, 1 theorem, 19 equations)

This paper contains 2 sections, 1 theorem, 19 equations.

Key Result

Theorem 1

Any closed extension $(\mathcal{E}, \mathcal{F})$ of $(\mathcal{E}, \mcF\mcC^\infty_b(\mathcal{D}))$ does not have a spectral gap, i.e.,

Theorems & Definitions (3)

  • Theorem
  • proof : Proof of the Theorem \ref{['t:maind']}
  • proof : Proof of \ref{['c:s']}