Mike2
- 1,312
- 0
I was not able to get the info from that site. Does this require a subscription or special on-line reader program?Chronos said:
The discussion centers on the potential modification of gravity as a means to address the dark energy dilemma, exploring theoretical frameworks and implications of event horizons in cosmology. Participants reference recent papers and propose various hypotheses regarding the nature of gravity, cosmological constants, and the behavior of matter in relation to event horizons.
Participants express a range of views on the implications of event horizons and the nature of gravity modifications. There is no consensus on the validity of the proposed ideas, and multiple competing perspectives remain throughout the discussion.
Participants reference various theoretical frameworks and papers, but the discussion includes unresolved assumptions about the nature of event horizons and the implications of modifications to gravity. The relationship between potential energy, mass, and cosmological constants is also not fully clarified.
I was not able to get the info from that site. Does this require a subscription or special on-line reader program?Chronos said:
I wonder if the big Freeze of galaxies that leave our horizon so we can no longer see them... what effect would that have on information content of the visible universe? Is that saying that information cannot leave our visible universe? The entropy, S=Q/T. If everything freezes at the horizon, then Q tends to zero, but also T tends to zero. Would Q include the rest mass which is energy?Mike2 said:In any event, if the disappearance of mass behind the horizon which causes the loss of negative gravitational potential (on average), is equal to an increase of a positive potential at each point, then does this increase in potential energy (=mass?) at each point cause particle creation in otherwise empty space? Does the information lost behind the horizon return to us in particle creation throughout the rest of space?
Interesting paper. The authors note that if the U continues to expand, the CMB will eventually be redshifted into the noise of the Hawking radiation at the event horizon and the information in the CMB will be lost to us.In a universe dominated by a small cosmological constant or by eternal dark energy with equation of state w < -1/3, observers are surrounded by event horizons. The horizons limit how much of the universe the observers can ever access.