  We present the argument that "pseudo-conformal" symmetry permeates from low
density near nuclear matter to high density in the core of massive neutron
stars. As a support of this argument, we describe how the quenched $g_A\approx
1$ in nuclei and the sound speed $v_s^2/c^2\approx 1/3$ in compact stars are
controlled by emerging scale invariance in nuclear interactions. In our
description, quasi-baryons could "masquerade" de-confined quarks in the
interior of compact stars.
