Is vacuum energy transient or permanent? Vacuum energy is based on Heisenberg's energy–time uncertainty principle which says that $\Delta E$ can exist for $\Delta t$.  This $\Delta E$ can produce electron positron pair for $\Delta t$ by which time they annihilate.  My question / confusion is that upon annihilation a pair of photons are produced, and this photon energy continues to exist beyond $\Delta t$, perhaps forever.  Is this correct understanding, as this seems to imply that $\Delta E$ can exist forever?
 A: No, your understanding is incorrect. The “vacuum bubble” Feynman diagrams contributing to the vacuum energy density don’t have any external lines. All particles are virtual, not real.
The following image shows two of an infinite number of such diagrams. In the simplest such diagram (the loop at the top), an electron and positron simply emerge from the vacuum and return to the vacuum. There are no real photons produced, and the process is not really annihilation.
In more complicated vacuum diagrams, such as the second loop, all photons are virtual, not real.

The image is from this discussion of vacuum energy. (The wavy line is actually a virtual graviton, not a virtual photon, but a similar diagram with a virtual photon would exist.)
If the vacuum were constantly producing real photons from virtual electrons and positrons, we would presumably have observed them!
A:  Answer using QFT in flat spacetime 
In quantum field theory in flat spacetime, the vacuum is a stationary state. It's energy is well-defined: $\Delta E=0$ in a stationary state. This is consistent with $\Delta E\Delta t\gtrsim\hbar$, because $\Delta t$ is undefined for a stationary state: in a stationary state, nothing "happens," ever. The energy of a stationary state is permanent. 
To get a state in which something happens, we need to consider a superposition of different stationary states having different energies. If the spread in the energies involved in the superposition is $\Delta t$, then the time-scale over which the state can change in time is $\Delta t\sim \hbar/\Delta E$. A stationary state has $\Delta E=0$, so $\Delta t$ is "infinite": the state never changes. Nothing happens.
 What about curved spacetime? 
This answer is based on QFT in flat spacetime, which ignores gravity. In this obviously-incomplete model, the overall energy of the vacuum state has no physical significance: it is unobservable. We can shift it arbitrarily without affecting any testable predictions, just by adjusting the constant term in the lagrangian. 
The situation changes when gravity is taken into account, because then the vacuum energy does have observable effects. Physics doesn't yet have a satisfying resolution of the vacuum-energy issue in that context. We don't even know exactly what "vacuum" means in that context.
 Perspective about virtual particles 
Feynman diagrams and the "virtual particle" language come from perturbation theory. Perturbation theory is a useful computational method, because it relates vacuum expectation values of the full theory (which is mathematically difficult) to various combinations of "vacuum" expectation values of an easier theory, but the vacuum state in the easier theory is a different state than the vacuum state in the full theory. Roughly speaking, the bubble diagrams illustrated in the answer by G. Smith represent terms in the perturbative expansion of the normalization factor that relates these two different states.
We have some idea of how to include gravity in perturbation theory, but this doesn't solve the "vacuum energy" problem. For that, we need a better understanding of quantum gravity than we currently have.
