  We elucidate the nature of the correction to the Hartle-Hawking wavefunction
presented in hep-th/$0505104$ and hep-th/$0406107$. The correction comes from
the quantum fluctuation of the metric that spontaneously breaks the classical
deSitter symmetry. This converts the tunneling from nothing to a deSitter-like
universe via a $S^{4}$ instantion to that via a barrel instanton, which is
bounded from below. Its generalization to 10 dimensional spacetime allows us to
find the preferred sites in the stringy cosmic landscape. We comment on how
some of the problems of the Hartle-Hawking wavefunction are avoided with the
new modified wavefunction of the universe, when applied to the spontaneous
creation of an inflationary universe. We also summarize our arguments on the
validity of the Hartle-Hawking wavefunction in the minisuperspace
approximation, as opposed to the WKB formula suggested by Linde and Vilenkin.
