Flash to Physics
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On Thu, Apr 2, 2009 at 6:07 PM, Physics Forums <gregbernhardt@gmail.com> wrote:
Dear FlashStarwalker,
apeiron has just replied to a thread you have subscribed to entitled - Another dark energy question. - in the Cosmology forum of Physics Forums.
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https://www.physicsforums.com/showthread.php?t=300465&goto=newpost
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FlashStarwalker - the notion of retrocausality from a future event horizon is very appealing as a general mechanism.
"Can you set aside your own enthusiasm enough to give a sketch of its current status within theory circles? Who is for it, who against it - the major lines of argument either way?"
James Woodward a professor of physics at Cal State in LA, Michael Ibison at Earth Tech Austin as well as Levit and Sarfatti are only ones active in the cosmological field today. Possibly John Cramer at U. Washington. AAAS had a retrocausality workshop June 2006 published by Dan Sheehan chairman of physics dept USD. Feynman & Hoyle first proposed it in 1940 and it was taken on by Fred Hoyle and J Narlikar. Bernard Carr, a former assistant to Hawking has written about it recently. He is at Queen Mary College, London. The point is if you try to explain dark energy density (not Omega DE) from the past horizon you get the wrong answer - it's way too big. You only get the right answer using the future horizon. Ergo ...
"For a start, there seem two quite different final fates depending on whether the universe is cruising to a halt, of forever gently accelerating away (big crunch and big rip cosmologies might well be ruled out by retro-causal considerations now?)."
exactly - it's ruled out say Levit & Sarfatti
"And does it connect yet with Lineweaver-Davies story about the blackbox photons (the radiation of event horizons) that will be all that is left at the Universe's heat death?"
i am not familiar with that - there is no heat death with dark energy. the accelerating universe is never in thermal equilibrium. that's why there is a future horizon - light takes infinite amount of proper time of the observer to travel a finite distance - that finite distance defines the location of the future horizon of the observer at any moment in her world line - see Davis Fig 1.1 "It seems a very significant new idea. So the ins and outs would be interesting to discuss."
understatement ;-)
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