We are concerned with the global stability and non-vanishing vacuum states of large strong solutions to the full compressible Navier–Stokes equations on the torus ({mathbb {T}}^3), and the main goal of this work is twofold. First, it is shown that the global strong solutions converge to an equilibrium state exponentially in (L^2) in the presence of vacuum provided that the density (rho ) and the temperature (theta ) are bounded uniformly in (L^infty ). This improves the previous related works in (Ann. Inst. H. Poincaré C Anal. Non Linéaire, 37 (2020), no. 2, 457–488) and (J. Math. Fluid Mech., 24 (2022), no. 2, Paper No. 31), where both (rho (x, t)) and (theta (x, t)) possess uniform-in-time positive lower and upper bounds, and (rho (x,t)) is bounded uniformly in the Hölder space (C^alpha ) for some (0<alpha <1). Moreover, we remove the extra restriction (2mu >lambda ) in their results. Second, by employing some new ideas, we show that the density and temperature converge to their equilibrium states exponentially in the (L^infty )-norm if additionally the initial density has positive lower bound, which extends the isentropic case in (SIAM J. Math. Anal., 55 (2023), no. 2, 882–899) to the non-isentropic case. As a by-product, we get that the vacuum state will persist for any time as long as the initial density contains vacuum.
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