The bit about gravitational energy is entirely incorrect. It's about 30% matter (currently). Gravitational energy is a somewhat nebulous concept which would be extremely misleading to use in this context, because dark energy influences the expansion history through gravity as well. It's just that different kinds of matter have different impact on the expansion rate.
Dark energy also doesn't "expand space". The expansion is already there. Dark energy just prevents the expansion rate from falling too low. It acts, in effect, as a repulsive force. Basically, it changes gravity in the Newtonian limit from:
[tex]F = -{G m_1 m_2 \over r^2}[/tex]
to:
[tex]F = -{G m_1 m_2 \over r^2} + {1 \over 3}\Lambda r[/tex]
This has an impact everywhere in the universe. But the value of [itex]\Lambda[/itex] is so small that it's unmeasurable on scales shorter than billions of light years.
Finally, the the density ratios today really don't tell you much of anything about our universe (except for the ratio of normal matter to dark matter: that's pretty stable over time). The problem is that the density ratios are a function of time. A billion years ago, matter would have been a larger portion of the total energy density. 12 billion years ago dark energy was a negligible component of the total energy density.
In order to get a handle on what the makeup of the universe means, you have to look at each component individually. The dark energy remains roughly constant over time. As the square of the expansion rate is proportional to the density, this means that the current ~70km/s/Mpc expansion rate will slowly decrease to ~60km/s/Mpc in the far future. As long as the dark energy is constant, it will remain at that rate indefinitely. The matter density, meanwhile, will decrease over time until nothing but empty space remains.