72,057 research outputs found

    Crystallization of random matrix orbits

    Full text link
    Three operations on eigenvalues of real/complex/quaternion (corresponding to β=1,2,4\beta=1,2,4) matrices, obtained from cutting out principal corners, adding, and multiplying matrices can be extrapolated to general values of β>0\beta>0 through associated special functions. We show that β\beta\to\infty limit for these operations leads to the finite free projection, additive convolution, and multiplicative convolution, respectively. The limit is the most transparent for cutting out the corners, where the joint distribution of the eigenvalues of principal corners of a uniformly-random general β\beta self-adjoint matrix with fixed eigenvalues is known as β\beta-corners process. We show that as β\beta\to\infty these eigenvalues crystallize on the irregular lattice of all the roots of derivatives of a single polynomial. In the second order, we observe a version of the discrete Gaussian Free Field (dGFF) put on top of this lattice, which provides a new explanation of why the (continuous) Gaussian Free Field governs the global asymptotics of random matrix ensembles.Comment: 25 pages. v2: misprints corrected, to appear in IMR

    Hydrodynamics and perfect fluids: uniform description of soft observables in Au+Au collisions at RHIC

    Full text link
    It is argued that the use of the initial Gaussian energy density profile for hydrodynamics leads to much better uniform description of the RHIC heavy-ion data than the use of the standard initial condition obtained from the Glauber model. With the modified Gaussian initial conditions we successfully reproduce the transverse-momentum spectra, v2, and the pionic HBT radii (including their azimuthal dependence). The emerging consistent picture of hadron production hints that a solution of the long standing RHIC HBT puzzle has been found.Comment: Talk presented by WF at the XXXVIII International Symposium on Multiparticle Physic

    Degenerate elliptic operators in one dimension

    Full text link
    Let HH be the symmetric second-order differential operator on L_2(\Ri) with domain C_c^\infty(\Ri) and action Hφ=(cφ)H\varphi=-(c \varphi')' where c\in W^{1,2}_{\rm loc}(\Ri) is a real function which is strictly positive on \Ri\backslash\{0\} but with c(0)=0c(0)=0. We give a complete characterization of the self-adjoint extensions and the submarkovian extensions of HH. In particular if ν=ν+ν\nu=\nu_+\vee\nu_- where ν±(x)=±±x±1c1\nu_\pm(x)=\pm\int^{\pm 1}_{\pm x} c^{-1} then HH has a unique self-adjoint extension if and only if ν∉L2(0,1)\nu\not\in L_2(0,1) and a unique submarkovian extension if and only if ν∉L(0,1)\nu\not\in L_\infty(0,1). In both cases the corresponding semigroup leaves L2(0,)L_2(0,\infty) and L2(,0)L_2(-\infty,0) invariant. In addition we prove that for a general non-negative c\in W^{1,\infty}_{\rm loc}(\Ri) the corresponding operator HH has a unique submarkovian extension.Comment: 28 page

    A rectangular additive convolution for polynomials

    Full text link
    We define the rectangular additive convolution of polynomials with nonnegative real roots as a generalization of the asymmetric additive convolution introduced by Marcus, Spielman and Srivastava. We then prove a sliding bound on the largest root of this convolution. The main tool used in the analysis is a differential operator derived from the "rectangular Cauchy transform" introduced by Benaych-Georges. The proof is inductive, with the base case requiring a new nonasymptotic bound on the Cauchy transform of Gegenbauer polynomials which may be of independent interest

    Quantum nature of black holes

    Full text link
    I reconsider Hawking's analysis of the effects of gravitational collapse on quantum fields, taking into account interactions between the fields. The ultra-high energy vacuum fluctuations, which had been considered to be an awkward peripheral feature of the analysis, are shown to play a key role. By interactions, they can scatter particles to, or create pairs of particle at, ultra-high energies. The energies rapidly become so great that quantum gravity must play a dominant role. Thus the vicinities of black holes are essentially quantum-gravitational regimes.Comment: 7 pages, 5 figures. Honorable mention in the 2004 Gravity Research Foundation Essay Competitio

    Leavitt RR-algebras over countable graphs embed into L2,RL_{2,R}

    Full text link
    For a commutative ring RR with unit we show that the Leavitt path algebra LR(E)L_R(E) of a graph EE embeds into L2,RL_{2,R} precisely when EE is countable. Before proving this result we prove a generalised Cuntz-Krieger Uniqueness Theorem for Leavitt path algebras over RR.Comment: 17 pages. At the request of a referee the previous version of this paper has been split into two papers. This version is the first of these papers. The second will also be uploaded to the arXi
    corecore