Recent investigations show that steady solutions share many features with
turbulent Rayleigh--B\'enard convection (RBC) and form the state space skeleton
of turbulent dynamics. Previous computations of steady roll solutions in
two-dimensional (2D) RBC between no-slip boundaries reveal that for fixed
Rayleigh number Ra and Prandtl number Pr, the heat-flux-maximizing solution
is always in the high-wavenumber regime. In this study, we explore the
high-wavenumber steady convection roll solutions that bifurcate supercritically
from the motionless conductive state for 2D RBC between stress-free boundaries.
Our computations confirm the existence of a local heat-flux-maximizing solution
in the high-wavenumber regime. To elucidate the asymptotic properties of this
solution, we perform computations over eight orders of magnitude in the
Rayleigh number, 108β€Raβ€1016.5, and two orders of magnitude in
the Prandtl number, 10β1β€Prβ€103/2. The numerical results
indicate that as Raββ, the local heat-flux-maximizing aspect ratio
ΞlocβββRaβ1/4, the Nusselt number Nu(Ξlocββ)βRa0.29, and the Reynolds number Re(Ξlocββ)βPrβ1Ra2/5,
with all prefactors depending on Pr. Moreover, the interior flow of the local
Nu-maximizing solution can be well described by an analytical heat-exchanger
solution, and the connection to the high-wavenumber asymptotic solution given
by Blennerhassett & Bassom is discussed. With a fixed aspect ratio
0.06β€Ξβ€Ο/5 at Pr=1, however, our computations show that as Ra
increases, the steady rolls converge to the semi-analytical asymptotic
solutions constructed by Chini & Cox, with scalings NuβΌRa1/3 and
ReβΌPrβ1Ra2/3. Finally, a phase diagram is delineated to gain a
panorama of steady solutions in the high-Rayleigh-number-wavenumber plane