1,792 research outputs found

    Continuity and estimates of the Liouville heat kernel with applications to spectral dimensions

    Get PDF
    The Liouville Brownian motion (LBM), recently introduced by Garban, Rhodes and Vargas and in a weaker form also by Berestycki, is a diffusion process evolving in a planar random geometry induced by the Liouville measure MγM_\gamma, formally written as Mγ(dz)=eγX(z)γ2E[X(z)2]/2dzM_\gamma(dz)=e^{\gamma X(z)-{\gamma^2} \mathbb{E}[X(z)^2]/2}\, dz, γ(0,2)\gamma\in(0,2), for a (massive) Gaussian free field XX. It is an MγM_\gamma-symmetric diffusion defined as the time change of the two-dimensional Brownian motion by the positive continuous additive functional with Revuz measure MγM_\gamma. In this paper we provide a detailed analysis of the heat kernel pt(x,y)p_t(x,y) of the LBM. Specifically, we prove its joint continuity, a locally uniform sub-Gaussian upper bound of the form pt(x,y)C1t1log(t1)exp(C2((xyβ1)/t)1β1)p_t(x,y)\leq C_{1} t^{-1} \log(t^{-1}) \exp\bigl(-C_{2}((|x-y|^{\beta}\wedge 1)/t)^{\frac{1}{\beta -1}}\bigr) for t(0,12]t\in(0,\frac{1}{2}] for each β>12(γ+2)2\beta>\frac{1}{2}(\gamma+2)^2, and an on-diagonal lower bound of the form pt(x,x)C3t1(log(t1))ηp_{t}(x,x)\geq C_{3}t^{-1}\bigl(\log(t^{-1})\bigr)^{-\eta} for t(0,tη(x)]t\in(0,t_{\eta}(x)], with tη(x)(0,12]t_{\eta}(x)\in(0,\frac{1}{2}] heavily dependent on xx, for each η>18\eta>18 for MγM_{\gamma}-almost every xx. As applications, we deduce that the pointwise spectral dimension equals 22 MγM_\gamma-a.e.\ and that the global spectral dimension is also 22.Comment: 36 page

    Neutrinos and Big-Bang Nucleosynthesis

    Get PDF
    Observations of clusters and super clusters of galaxies have indicated that the Universe is more dominated by baryons than ever estimated in the homogeneous cosmological model for primordial nucleosynthesis. Recent detections of possibly low deuterium abundance in Lyman-α\alpha clouds along the line of sight to high red-shift quasars have raised another potential difficulty that \he4 is overproduced in any cosmological models which satisfy the low deuterium abundance constraint. We show that the inhomogeneous cosmological model with degenerate electron-neutrino can resolve these two difficulties.Comment: 7 pages, latex, 3 figures. To appear in Nucl. Phys. A62
    corecore