"Pseudo-Conformal" Sound Speed in the Core of Compact Stars

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 $v_s^2\mathrm{/}{c}^2\approx 1\mathrm{/}3$ 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.