  We analyze the tomographic representation for the Friedmann-Robertson-Walker
(FRW) model within the Loop Quantum Cosmology framework. We focus on the Wigner
quasi-probability distributions associated with Gaussian and Schr\"odinger cat
states, and then, by applying a Radon integral transform for those Wigner
functions, we are able to obtain the symplectic tomograms which define
measurable probability distributions that fully characterize the quantum model
of our interest. By appropriately introducing the quantum dispersion for a
rotated and squeezed quadrature operator in terms of the position and momentum,
we efficiently interpret the properties of such tomograms, being consequent
with Heisenberg's uncertainty principle. We also obtain, by means of the dual
tomographic symbols, the expectation value for the volume operator, which
coincides with the values reported in the literature. We expect that our
findings result interesting as the introduced tomographic representation may be
further benefited from the well-developed measure techniques in the areas of
Quantum optics and Quantum information theory.
