A ug 2 00 9 One - radius results for supermedian functions on R d , d ≤ 2

A note on the Roman domatic number of a digraph

Roman dominating function} on a digraph $D$ with vertex set $V(D)$ is a labeling$fcolon V(D)to {0, 1, 2}$such that every vertex with label $0$ has an in-neighbor with label $2$. A set ${f_1,f_2,ldots,f_d}$ ofRoman dominating functions on $D$ with the property that $sum_{i=1}^d f_i(v)le 2$ for each $vin V(D)$,is called a {em Roman dominating family} (of functions) on $D$....

nd - m at . s up r - co n ] 2 9 A ug 2 00 2 Direct Correlation between Tc and CuO 2 Bilayer Spacing in YBa 2 Cu 3 O 7 − x

ar X iv : h ep - l at / 0 60 80 21 v 1 2 8 A ug 2 00 6 The pion form factor from lattice QCD with two dynamical flavours

We compute the electromagnetic form factor of the pion using non-perturbatively O(a) improved Wilson fermions. The calculations are done for pion masses down to 400 MeV and for lattice spacings of 0.07 – 0.11 fm. We check for finite size effects by repeating some of the measurements on smaller lattices. The large number of lattice parameters we use allows us to extrapolate to the physical point...

A ug 2 00 4 Automorphic Distributions , L - functions , and Voronoi Summation for GL ( 3 )

Role of Initial Data in Higher Dimensional Quasi-Spherical Gravitational Collapse

X iv :g rqc /0 30 80 37 v1 1 2 A ug 2 00 3 Role of Initial Data in Higher Dimensional Quasi-Spherical Gravitational Collapse Ujjal Debnath and Subenoy Chakraborty Department of Mathematics, Jadavpur University, Calcutta-32, India. (Dated: February 7, 2008) We study the gravitational collapse in (n+2)-D quasi-spherical Szekeres space-time (which possess no killing vectors) with dust as the matte...