[ExI] The Universe is disappearing
Anders Sandberg
anders at aleph.se
Wed Aug 12 13:02:11 UTC 2015
(Seems my original post got eaten by entropy; here is a repost)
The media are reporting it as evidence of the End of the Universe or the imminent heat death:
http://news.discovery.com/space/galaxies/universe-is-dying-galactic-survey-shows-150810.htm
http://arxiv.org/abs/1508.02076
Basically, the energy production is going down.
This is unsurprising to anybody keeping up with star formation trends (http://arxiv.org/abs/1202.3436). There is also a common view that planet formation peaked way back, leaving Earth as one of the later planets (still, there is a possibility that because of gas infall there will be enough of a long tail of future planet formation that makes us early anyway: http://arxiv.org/abs/1508.01202 ).
Still, I wonder if this isn't good news for us intelligent creatures, for three reasons:
First, high star formation also means high supernova and GRB rates; as Cirkovic et al have argued, this might even have precluded the formation of intelligent life until recently (and some people think it causes a galactic habitable zone).
Second, a lot of stellar energy doesn't mean a lot of lifezones: the lifezone radius and width scales as the square root of the luminosity, making it scale as mass to the power 1.75. But the lifespan of a star scales as mass^-2.5, so the total "width-years" scales as mass^-0.75 - we get more space and time for life among low-mass stars. Since lighter stars are more common than heavier (along some power law distribution), we can conclude that while luminosity often gets dominated by the young bluewhite stars most of the habitability is produced among the dimmer ones (also, see http://www.sciencemag.org/content/346/6210/732 - there may be a lot of ejected dim stars between galaxies). Since the dim ones last long, the total amount of lifezone may be going up.
Third, it also means that less matter is burned into unusable radiation before we can get to it and use it to produce life, intelligence and complexity. The radiation losses are not that large if we can convert matter directly into energy (a few percent tops), but if there is a tech ceiling limiting us to fusion (direct or through Dyson shells) then we may want to avoid having the stars go out too quickly.
Anders Sandberg, Future of Humanity Institute Philosophy Faculty of Oxford University
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