Understanding Vacuum Energy: A Key to Unifying QFT and GR?

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Discussion Overview

The discussion revolves around the concept of vacuum energy and its implications for unifying quantum field theory (QFT) and general relativity (GR). Participants explore the nature of vacuum energy, its potential scale invariance, and its gravitational effects, as well as the challenges posed by the cosmological constant problem.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • One participant expresses curiosity about vacuum energy, questioning its scale invariance and its role in connecting phenomena across different length scales.
  • Another participant notes that vacuum energy is typically set to zero in calculations, as only energy differences are relevant, but highlights that this changes when considering gravity.
  • A third participant references an article on vacuum energy, suggesting uncertainty about its true nature and existence.
  • Participants discuss the cosmological constant problem, where the predicted vacuum energy from QFT significantly exceeds the observed value, raising questions about the validity of current theories.
  • There is a reiteration of the importance of gravity in discussions of vacuum energy, emphasizing that the energy tensor affects curvature in GR.

Areas of Agreement / Disagreement

Participants generally express uncertainty about the nature of vacuum energy and its implications, with no consensus on its properties or the resolution of the cosmological constant problem. There are competing views on how vacuum energy should be treated in the context of gravity.

Contextual Notes

Limitations include the dependence on definitions of vacuum energy and the unresolved nature of the cosmological constant problem, which remains a significant challenge in theoretical physics.

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I often wonder about how little I understand vacuum, and only recently I've been paying attention to this "vacuum energy" hypothetical.

I see it being associated with things as small as spontaneous emissions to things as large as the expansion of the universe. This is a huge range of length scales. I know of no other force (or energy or whatever) with that kind of reach.

What could this potentially mean?

As far as we can observe, is it reasonable to hypothesize that "vacuum energy" is scale invariant (does it make sense to say that energy or energy potential is scale invariant?), hereby enabling the coupling of physical phenomena from different length scales, and maybe even holding the key to the unification of QFT with GR?

Or am I smoking crack?

Have to say that it looks like a promising concept, even though I don't really understand what/how it is yet. Hence, I defer the title question to the experts.
 
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I also need to learn a lot about vacuum energy and QFT in general. But from what I know vacuum energy is associated with the vacuum diagrams of a given theory. Usually one sets the vacuum energy to zero, which is equivalent to normal ordering quantum fields. We do this because we only care about energy differences.

All this is fine until we consider gravity. Gravity couples to energy, so the vacuum energy will have a gravitational effect. Supposedly the vacuum energy of all fields in the universe should add up to give a value for the cosmological constant, and this calculaton was done by S. Weinberg (he may have been the first, not too sure on that). Yet, the experimental value of the cosmological constant is order of magnetudes smaller than the predicted value accoding to QFT. This calculation, which may be dubbed the worst prediction in physics, is the cosmological constant problem.
 
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Lucas SV said:
We do this because we only care about energy differences.

You can only care about energy difference as long as you ignore gravity and work in flat Minkovski space. With GR, energy tensor itself, not the difference, affects curvature.
 
nikkkom said:
You can only care about energy difference as long as you ignore gravity and work in flat Minkovski space. With GR, energy tensor itself, not the difference, affects curvature.
Yes, of course. This is why I said "All this is fine until we consider gravity" ...
 
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