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We consider the inequality $f geqslant fstar f$ for real integrable functions on $d$ dimensional Euclidean space where $fstar f$ denotes the convolution of $f$ with itself. We show that all such functions $f$ are non-negative, which is not the case for the same inequality in $L^p$ for any $1 < p leqslant 2$, for which the convolution is defined. We also show that all integrable solutions $f$ satisfy $int f(x){rm d}x leqslant tfrac12$. Moreover, if $int f(x){rm d}x = tfrac12$, then $f$ must decay fairly slowly: $int |x| f(x){rm d}x = infty$, and this is sharp since for all $r< 1$, there are solutions with $int f(x){rm d}x = tfrac12$ and $int |x|^r f(x){rm d}x <infty$. However, if $int f(x){rm d}x = : a < tfrac12$, the decay at infinity can be much more rapid: we show that for all $a<tfrac12$, there are solutions such that for some $epsilon>0$, $int e^{epsilon|x|}f(x){rm d}x < infty$.
The paper studies the sampling discretization problem for integral norms on subspaces of $L^p(mu)$. Several close to optimal results are obtained on subspaces for which certain Nikolskii-type inequality is valid. The problem of norms discretization i
In this paper we introduce a new generalisation of the relative Fisher Information for Markov jump processes on a finite or countable state space, and prove an inequality which connects this object with the relative entropy and a large deviation rate
In this paper we investigate linear codes with complementary dual (LCD) codes and formally self-dual codes over the ring $R=F_{q}+vF_{q}+v^{2}F_{q}$, where $v^{3}=v$, for $q$ odd. We give conditions on the existence of LCD codes and present construct
One may define a trilinear convolution form on the sphere involving two functions on the sphere and a monotonic function on the interval $[-1,1]$. A symmetrization inequality of Baernstein and Taylor states that this form is maximized when the two fu
A review of the new of the problem of dark energy using modified gravity approach is considered. An explanation of the difficulties facing modern cosmology is given and different approaches are presented. We show why some models of gravity may suffer