Could the expansion of space tear us apart?

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Discussion Overview

The discussion revolves around the concept of the "big rip," a hypothetical scenario in cosmology where the expansion of the universe could eventually overcome the fundamental forces holding matter together. Participants explore the implications of dark energy and energy conditions in General Relativity, as well as the likelihood of such a scenario occurring.

Discussion Character

  • Debate/contested
  • Technical explanation
  • Conceptual clarification

Main Points Raised

  • Some participants propose that the forces behind the expansion of space could potentially overcome molecular forces, leading to the big rip scenario.
  • Others argue that while the big rip is a possibility, it does not appear likely based on current understanding.
  • A participant questions the feasibility of writing a sensible theory of gravity if energy conditions are violated, suggesting that such scenarios may be unphysical.
  • Another participant counters that dark energy does violate certain energy conditions but still allows for valid models in General Relativity.
  • Concerns are raised about the implications of negative mass and the stability of phantom fluids in the context of the big rip hypothesis.
  • Some participants clarify that the big rip scenario requires a specific relationship between dark energy pressure and density, indicating that if this ratio exceeds -1, the universe could eventually tear apart.
  • One participant references the latest Planck results, suggesting that measurements indicate the equation of state of dark energy is very close to -1, which aligns with the standard LambdaCDM model and contradicts the big rip scenario.

Areas of Agreement / Disagreement

Participants express differing views on the likelihood of the big rip scenario occurring. While some acknowledge it as a possibility, others emphasize that current evidence suggests it is unlikely, leading to an unresolved debate on the topic.

Contextual Notes

Participants note limitations regarding the assumptions underlying energy conditions and the implications of dark energy, as well as the need for further clarification on the stability of models that violate these conditions.

Ghostcrown
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Is it possible that the forces behind the expansion of space could at some point overcome the fundamental forces holding our molecules together?
 
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That idea is known as big rip. Possible, but it does not look likely.
 
mfb said:
That idea is known as big rip. Possible, but it does not look likely.
I think that may be overstating the situation a bit.

The big rip scenario requires a violation of some of the energy conditions of General Relativity. I'm not sure it's possible to write a sensible theory of gravity if those energy conditions are violated.

So we can't say for sure that it's impossible, but it's probably impossible.
 
Chalnoth said:
I'm not sure it's possible to write a sensible theory of gravity if those energy conditions are violated.

Sure it is. Dark energy violates energy conditions, but we have perfectly sensible models in GR that include dark energy. Solutions that violate one or more of the energy conditions don't have certain "nice" properties, but they're still valid solutions.
 
PeterDonis said:
Sure it is. Dark energy violates energy conditions, but we have perfectly sensible models in GR that include dark energy. Solutions that violate one or more of the energy conditions don't have certain "nice" properties, but they're still valid solutions.
Dark energy only violates the strong energy condition (a condition that is violated in other contexts as well), the "big rip" scenario violates them all. In particular, it violates the weak energy condition which requires that the observed mass density be non-negative for all observers. Negative mass can lead to all sorts of nasty consequences.
 
Chalnoth said:
Dark energy only violates the strong energy condition (a condition that is violated in other contexts as well), the "big rip" scenario violates them all.

Yes, agreed. Solutions that violate all of the energy conditions are most likely unphysical. But solutions that only violate some (like ordinary dark energy) can be physically reasonable. In post #3 you said "some", which was why I commented. :wink:
 
if my understanding is correct, the big rip hypothesis says that if the ratio between dark energy pressure and it's density is > -1 then the universe will eventually be pulled apart and that an instant before the end atoms will be destroyed
 
Vighnesh Nagpal said:
if my understanding is correct, the big rip hypothesis says that if the ratio between dark energy pressure and it's density is > -1 then the universe will eventually be pulled apart and that an instant before the end atoms will be destroyed
Yes, essentially. In the model, the cosmological horizon is constantly decreasing in size. Eventually the horizon will get so small that it will be impossible for atoms and even atomic nuclei to hold together.
 
  • #10
mfb said:
That idea is known as big rip. Possible, but it does not look likely.

Specifically, to judge for yourself how unlikely, look at the latest Planck results. The equation of state number w is measured to be WITHIN 5% of the value -1 which it has in the standard LambdaCDM model (cosmological curvature constant Lambda, no big rip)
The standard cosmic model has an INCREASING horizon distance that goes to an asymptotic value of 17.3 billion LY.
Not a DECREASING horizon distance that gets down to atom size. Huge difference.

Successive measurements keep nailing w down closer and closer to -1. So google [planck 2015 cosmological parameters] to get the report:

http://arxiv.org/abs/1502.01589
Planck 2015 results. XIII. Cosmological parameters
Planck Collaboration: ...
(Submitted on 5 Feb 2015...)
==abstract==
We present results based on full-mission Planck observations of temperature and polarization anisotropies of the CMB. These data are consistent with the six-parameter inflationary LCDM cosmology. ...
...
...The equation of state of dark energy is constrained to w = -1.006 +/- 0.045. Standard big bang nucleosynthesis predictions for the Planck LCDM cosmology are in excellent agreement with observations. We investigate annihilating dark matter and deviations from standard recombination, finding no evidence for new physics. The Planck results for base LCDM are in agreement with BAO data and with the JLA SNe sample. However the amplitude of the fluctuations is found to be higher than inferred from rich cluster counts and weak gravitational lensing. Apart from these tensions, the base LCDM cosmology provides an excellent description of the Planck CMB observations and many other astrophysical data sets.
==endquote==
 
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