negativzero said:
Thanks Marcus for your kind and prompt response. ...
I believe I was not kind or prompt enough. Sorry about the curtness.
You might like an article by Lawrence Krauss "the return of the static universe". It envisages the distant future assuming the standard LCDM model.
The Milky Way, having merged with some of its neighbor galaxies, persists indefinitely.
We get the same misunderstanding of "accelerated expansion" over and over again.
It doesn't mean that the growth speed of separations of a given size (like one megaparsec) will increase. In fact for one megaparsec the growth speed is now 70 km/s and is slated to go down to around 60 km/s in the very long run.
So any structure which has adjusted to the present mild expansion (like our galaxy has) will have an EASIER TIME IN THE FUTURE HOLDING TOGETHER.
When they say "accelerated expansion" this refers to something different: consider two objects which are stationary with respect to CMB (the background of ancient light). Assume they are not part of any bound structure like a galaxy or cluster of galaxies, and that they are drifting apart at the standard rate which is currently 1/146 of one percent per million years.
THEN THEIR SEPARATION WILL INCREASE EXPONENTIALLY. Because as they get farther apart, since it grows at roughly a constant percentage rate (or only very slowly declining percent rate) the separation has to grow exponentially like money in a bank savings account. As the base amount increases the yearly increment increases. So that is the acceleration.
the growth speed associated with a separation of a FIXED SIZE actually is DECREASING, but despite that if you track a given separation between two stationary observers over a long period of time you will see the separation increasing faster as it gets bigger (like the bank account).
Anyway in future according to standard LCDM model our galaxy will be bigger and have more stars than it does today. You might Google "krauss return static universe" and see if you like his description of the distant future.