Virtual Pairs and the Fate of the Universe

In summary, the presence of a cosmological event horizon in a deSitter spacetime results in the creation of particles, most of them photons. The energy density of photons depends on the temperature, which in turn depends on the area of the horizon. If the universe is expanding exponentially, the event horizon remains at a constant distance from the comoving observers and the energy density of the particles created by the event horizon will remain constant in time. However, if the universe is flat and remains flat until then, then every slight perturbation in its energy density will change its curvature and space may evolve in a different way.
  • #1
Hellburner
10
0
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?
 
Astronomy news on Phys.org
  • #2
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
 
Last edited:
  • #3
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.
 
  • #4
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.
 
Last edited:
  • #5

What is the concept of virtual pairs?

Virtual pairs refer to a phenomenon in quantum mechanics where particles and antiparticles spontaneously appear and disappear in pairs in a vacuum. These pairs have opposite charges and quickly annihilate each other, making them difficult to detect.

How do virtual pairs relate to the fate of the universe?

According to some theories, virtual pairs play a crucial role in the fate of the universe. The constant creation and annihilation of these pairs can cause fluctuations in the vacuum energy, which can contribute to the expansion of the universe.

Can virtual pairs be observed?

Virtual pairs cannot be directly observed, but their effects can be detected through various experiments and observations. For example, the Casimir effect is a result of the presence of virtual pairs in a vacuum.

What is the significance of virtual pairs in cosmology?

The study of virtual pairs is important in understanding the fundamental nature of the universe and its evolution. It also has implications in areas such as particle physics and black hole thermodynamics.

Can virtual pairs affect the stability of the universe?

Some theories suggest that the constant creation and annihilation of virtual pairs can contribute to the acceleration of the universe's expansion, leading to a potential instability. However, this is still a subject of ongoing research and debate in the scientific community.

Similar threads

Replies
7
Views
878
  • Astronomy and Astrophysics
Replies
6
Views
2K
  • Special and General Relativity
Replies
11
Views
694
  • Astronomy and Astrophysics
Replies
1
Views
1K
  • Astronomy and Astrophysics
Replies
1
Views
1K
Replies
4
Views
2K
Replies
24
Views
2K
  • Quantum Physics
Replies
9
Views
1K
Replies
29
Views
2K
Replies
10
Views
1K
Back
Top