English

Radial Fast Diffusion on the Hyperbolic Space

Analysis of PDEs 2017-05-17 v3 Differential Geometry

Abstract

We consider radial solutions to the fast diffusion equation ut=Δumu_t=\Delta u^m on the hyperbolic space HN\mathbb{H}^{N} for N2N \ge 2, m(ms,1)m\in(m_s,1), ms=N2N+2m_s=\frac{N-2}{N+2}. By radial we mean solutions depending only on the geodesic distance rr from a given point oHNo \in \mathbb{H}^N. We investigate their fine asymptotics near the extinction time TT in terms of a separable solution of the form V(r,t)=(1t/T)1/(1m)V1/m(r){\mathcal V}(r,t)=(1-t/T)^{1/(1-m)}V^{1/m}(r), where VV is the unique positive energy solution, radial w.r.t. oo, to ΔV=cV1/m-\Delta V=c\,V^{1/m} for a suitable c>0c>0, a semilinear elliptic problem thoroughly studied in \cite{MS08}, \cite{BGGV}. We show that uu converges to V{\mathcal V} in relative error, in the sense that um(,t)/Vm(,t)10\|{u^m(\cdot,t)}/{{\mathcal V}^m(\cdot,t)}-1\|_\infty\to0 as tTt\to T^-. In particular the solution is bounded above and below, near the extinction time TT, by multiples of (1t/T)1/(1m)e(N1)r/m(1-t/T)^{1/(1-m)}e^{-(N-1)r/m}.

Keywords

Cite

@article{arxiv.1302.4093,
  title  = {Radial Fast Diffusion on the Hyperbolic Space},
  author = {Gabriele Grillo and Matteo Muratori},
  journal= {arXiv preprint arXiv:1302.4093},
  year   = {2017}
}

Comments

To appear in Proc. London Math. Soc

R2 v1 2026-06-21T23:27:39.499Z