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Leon Fidele Ruganzu Uwimbabazi

Publications and source records attributed to Leon Fidele Ruganzu Uwimbabazi.

2 recordsLinked to original sources

Voronoi limit measures for iterates of constant-coefficient differential operators on rational functions with simple poles

Bøgvad and Hägg proved that for a rational function with simple poles, the zeros of successive derivatives accumulate on the Voronoi diagram of the pole set, and the normalized zero-counting measures converge to a canonical probability measure supported on this diagram. We extend this result from pure derivatives to iterates of an arbitrary monic constant-coefficient differential operator. Let $h(z)=A(z)/B(z)$ be a reduced rational function, where $B$ is monic of degree $b\ge2$ with distinct zeros $S=\{z_1,\dots,z_b\}$, and let $P(D)=\sum_{j=0}^m c_jD^j$ be a monic constant-coefficient differential operator of order $m\ge1$. After clearing denominators, we can write $P(D)^n(h)=\widetilde A_n/B^{mn+1}$ and study the zeros of the numerator polynomials $\widetilde A_n$. If $r:=\min\{j:c_j\neq0\}$, then (after passing to the proper part of $h$ when $r>0$) the associated zero-counting measures converge vaguely to $$\frac{m(b-1)}{bm-r}\,μ_S,$$ where $μ_S$ is the Bøgvad--Hägg probability measure supported on the Voronoi diagram $V_S$. In particular, the limit is a probability measure exactly when $P(D)=D^m$; otherwise a proportion $\frac{m-r}{bm-r}$ of zeros escapes to infinity (in the sense of vague convergence). When $r<m$, the unshifted logarithmic potentials diverge, but an explicit factorial renormalization yields $L^1_{\mathrm{loc}}(\mathbb C)$ convergence to a subharmonic limit with Riesz measure $\frac{m(b-1)}{bm-r}\,μ_S$. Apart from this scalar factor, the limiting measure is determined solely by the pole configuration; the coefficients of $P(D)$ affect only an additive constant in the limiting potential.

math.CV↗

On Chaplygin models in f(G) gravity

The current work treats cosmological perturbation in a mixture of standard matter, Chaplygin gas as well as Gauss-bonnet fluids using a 1+3 covariant approach in the context of modified $f(G)$ gravity. We define the gradient variables to obtain linear perturbation equations. After scalar and redshift transformations, we consider both an original Chaplygin and generalized Chaplygin gas models under Gauss-bonnet gravity. For pedagogical purposes, the consideration of polynomial $f(G)$ gravity model was used to solve the perturbation equations for short- and long- wavelength modes and investigate the late time evolution. The numerical solutions were obtained. The results show that the energy overdensity perturbations decay with an increase in redshift. The treatment recovers GR results under limiting cases.

gr-qc↗