  We propose structures of size between $\sim 1$ meter to 100 meters that
drastically alter the local distribution of the Cosmic Neutrino Background
($C\nu B$). These structures have a shape reminiscent of a sea urchin: They
consist of rods of width $w$ and length $L \gg w$ periodically arranged on the
surface of sphere of radius $R\sim L$. Such a structure functions as a
diffraction phase grating and produces a region around its center where the
fractional neutrino-antineutrino asymmetry is $\sim k\delta_\nu L$, where $k$
is the neutrino momentum, and $\delta_\nu$ the deviation of the neutrino index
of refraction from unity. The asymmetry has a gradient set by the rod width.
  We find that the local neutrino asymmetry can be enhanced by
$\mathcal{O}(\text{few}\times 10^6)$ relative to the naive Standard Model
expectation, for reasonably sized structures. This results in a force
$\mathcal{O}(10^3)$ times bigger than the one we recently pointed out due to
the neutrinos' reflection on the surface of the Earth. While in this paper we
do not propose a concrete detection setup, we estimate that the
$\mathcal{O}(G_F)$ force on a test mass can be close to the Standard Quantum
Limit of a torsion balance or a low frequency harmonic oscillator.
  Finally, we show that this $C \nu B$ diffractor can be used as a Dark Matter
diffractor. For example, the QCD axion Dark Matter with decay constant $f_a$
around $10^9$ GeV can be sufficiently diffracted to produce a gradient force
that is up to $\mathcal{O}(10^2)$ times larger than the one from the $C \nu B$.
  This is the first setup of this kind and the simplicity of our design
suggests that there could be significant improvements that escape us.
