In the context of the universe's eventual heat death, the discussion centers on whether all matter could become superconducting or exist as quantum condensates. The fate of matter is linked to the half-life of protons; if protons decay, all matter will ultimately transform into low-energy photons. If protons do not decay, quantum tunneling could lead to all matter behaving like a liquid at low temperatures. The potential for superconductivity or condensates to dominate in a future cosmological era remains uncertain and hinges on these fundamental processes. Ultimately, the future state of matter is deeply tied to the behavior of protons over vast timescales.