Virtual Pairs and the Fate of the Universe

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Discussion Overview

The discussion revolves around the implications of virtual particle-antiparticle pairs created near the event horizon of the universe, particularly their potential effects on the mass and topology of the universe as it expands. Participants explore concepts from general relativity and quantum mechanics, considering how these ideas might relate to dark energy and the fate of the universe.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • Some participants suggest that virtual particle-antiparticle pairs could continuously add mass to the universe as the event horizon expands, raising questions about the universe's mass and topology.
  • Others argue that while general relativity (GR) typically treats vacuum as having zero density, a quantum perspective suggests it is filled with virtual particles, leading to a potential mismatch in energy density expectations known as the "Lambda problem."
  • One participant proposes that if the energy density from virtual pairs contributes to dark energy, it could affect the universe's expansion dynamics, although they note that these particles are not specifically created at the event horizon but are present everywhere.
  • Another viewpoint discusses the possibility of a conservation law that might require mass lost behind the cosmological event horizon to be compensated by new particles created from Zero Point Energy, linking this to the evolution of structure in the universe.
  • A different participant mentions that in a deSitter spacetime, the energy density of particles detected by an observer within the cosmological event horizon remains constant over time, suggesting negligible influence on the universe's expansion.
  • There is also a mention of the potential for slight perturbations in energy density to affect the curvature of a flat universe, although the overall expansion is expected to continue indefinitely due to dark energy.

Areas of Agreement / Disagreement

Participants express multiple competing views regarding the role of virtual particles and their implications for cosmology. There is no consensus on how these concepts interact with the universe's expansion and topology.

Contextual Notes

Participants reference various cosmological models and concepts, including the effects of dark energy and the nature of event horizons, but do not resolve the complexities or assumptions inherent in these discussions.

Hellburner
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I was thinking... virtual particle-antiparticle pairs created just inside the event horizon of the universe continuously adding mass to the universe at an ever increasing rate as the event horizon expands and accelerates... How does this effect the mass/topology of the universe and could this eventually close the universe? Am I misunderstanding something?
 
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Welcome to these Forums Hellburner! An interesting question.

GR states empty (of electro-magnetic fields etc.) vacuum has zero density, a quantum approach would suggest that it is full of virtual particles of potentially huge energy density. So you can take your choice.

Normally cosmology takes a GR approach, at least until you get to the initial 'singularity' or worry about Dark Energy, in this cosmological case the expanding universe does not impinge on virtual pairs and they in turn have no effect on the expansion of the universe.

However if you now do think about DE then this energy density could be made up of Zero Point Energy of virtual pairs in the false vacuum. There is then what is known as the "Lambda problem", a mismatch of around 10^140 or so (depending on who you read) in density expectations between quantum theory and that required to 'fix' GR cosmology. These virtual pairs are then required to have a double effect, they add mass to the universe conveniently making the cosmological density up to the critical density, and they effect the dynamics of the expansion making it accelerate (at times!).

However these are not virtual particles being created along the event horizon, they are just there, everywhere. I think you must be thinking of Hawking radiation from a Black Hole in your post #1.

Garth
 
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Hellburner said:
I was thinking... virtual particle-antiparticle pairs created just inside the event horizon of the universe continuously adding mass to the universe at an ever increasing rate as the event horizon expands and accelerates... How does this effect the mass/topology of the universe and could this eventually close the universe? Am I misunderstanding something?
Or it might be that there is some sort of conservation law requiring that whatever mass is lost behind the present cosmological event horizon be compensated for by the creation of new particles by the Zero Point Energy of the quantum fields. I suppose if this effect were real, then it could be traced all the way back to the creation of the very first particles (whether massive or not). It seems to me that particles in and of themselves represent the perpetuation of some sort of structure and form contrary to the effects of entropy which seems to want to obliterate structure. I wonder if a conservation of entropy or information could be responsible the structures that evolve as the universe expands. I think of space expanding before any particle was created, and I suspect that somehow that the expansion of space itself is responsible for how the first particle inside the universe came to be.
 
Hellburner said:
I was thinking... virtual particle-antiparticle pairs created just inside the event horizon of the universe continuously adding mass to the universe at an ever increasing rate as the event horizon expands and accelerates... How does this effect the mass/topology of the universe and could this eventually close the universe? Am I misunderstanding something?
If I understand correctly you are talking about the particles created due to the existence of a cosmological event horizon in a deSitter spacetime, same as the particles created due to a Hawking horizon in a Schwarzschild spacetime, or due to a Rindler horizon in case of an accelerated observer in a Minkowski spacetime.

In such a case the observer located within the cosmological event horizon detects a thermal distribution of particles (most of them photons). The energy density of photons depends on the temperature (Stefan-Boltzmann law), which in turn depends on the area of the horizon. In an exponentially expanding universe (which will be the fate of our universe, as currently believed) the event horizon remains at a constant distance from the comoving observers (at the Hubble sphere) and thus does not change its area. This means that the energy density of the particles created by the event horizon will remain constant in time.

Since this energy density will be also very small (I recall John Baez made a calculation of the temperature which is available somewhere in his web), its influence will be negligible. However, if the universe is exactly flat and remains flat until then (a very improbable coincidence), then every slight perturbation in its energy density will change its curvature. Although it will expand forever due to the action of the dark energy (which, due to its high energy density, accelerates the expansion regardless of the curvature), its geometry will change with this slight perturbation and space may evolve in a different way.
 
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