Well, there are some fairly reliable maximum bounds, I suppose:
https://en.wikipedia.org/wiki/Ultimate_fate_of_the_universe
There is a strong consensus among cosmologists that the shape of the universe is considered “flat” (parallel lines stay parallel) and will continue to expand forever.[2][3]
The ultimate fate of an open universe with dark energy is either universal heat death or a “Big Rip”[12][13][14][15] where the acceleration caused by dark energy eventually becomes so strong that it completely overwhelms the effects of the gravitational, electromagnetic and strong binding forces.
Neither a universal heat death nor a Big Rip — and we expect one of the two to occur — seems likely to be conducive to capitalism.
https://en.wikipedia.org/wiki/Heat_death_of_the_universe
The heat death of the universe (also known as the Big Chill or Big Freeze)[1][2] is a hypothesis on the ultimate fate of the universe, which suggests the universe will evolve to a state of no thermodynamic free energy, and will therefore be unable to sustain processes that increase entropy.
The theory suggests that from the “Big Bang” through the present day, matter and dark matter in the universe are thought to have been concentrated in stars, galaxies, and galaxy clusters, and are presumed to continue to do so well into the future. Therefore, the universe is not in thermodynamic equilibrium, and objects can do physical work.[15]:§VID The decay time for a supermassive black hole of roughly 1 galaxy mass (10¹¹ solar masses) because of Hawking radiation is in the order of 10¹⁰⁰ years,[16] so entropy can be produced until at least that time. Some large black holes in the universe are predicted to continue to grow up to perhaps 10¹⁴ M☉ during the collapse of superclusters of galaxies. Even these would evaporate over a timescale of up to 10¹⁰⁶ years.[17] After that time, the universe enters the so-called Dark Era and is expected to consist chiefly of a dilute gas of photons and leptons.[15]:§VIA With only very diffuse matter remaining, activity in the universe will have tailed off dramatically, with extremely low energy levels and extremely long timescales.
https://en.wikipedia.org/wiki/Big_Rip
In physical cosmology, the Big Rip is a hypothetical cosmological model concerning the ultimate fate of the universe, in which the matter of the universe, from stars and galaxies to atoms and subatomic particles, and even spacetime itself, is progressively torn apart by the expansion of the universe at a certain time in the future, until distances between particles will infinitely increase.
In their paper, the authors consider a hypothetical example with w = −1.5, H0 = 70 km/s/Mpc, and Ωm = 0.3, in which case the Big Rip would happen approximately 22 billion years from the present. In this scenario, galaxies would first be separated from each other about 200 million years before the Big Rip. About 60 million years before the Big Rip, galaxies would begin to disintegrate as gravity becomes too weak to hold them together. Planetary systems like the Solar System would become gravitationally unbound about three months before the Big Rip, and planets would fly off into the rapidly expanding universe. In the last minutes, stars and planets would be torn apart, and the now-dispersed atoms would be destroyed about 10¯¹⁹ seconds before the end (the atoms will first be ionized as electrons fly off, followed by the dissociation of the atomic nuclei). At the time the Big Rip occurs, even spacetime itself would be ripped apart and the scale factor would be infinity.
