How can anyone explain the universal equilibrium density problem

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Discussion Overview

The discussion centers around the concept of universal equilibrium density in the context of an expanding universe, particularly focusing on the roles of dark energy and dark matter. Participants explore theoretical implications, potential relationships, and the challenges in understanding these phenomena.

Discussion Character

  • Exploratory
  • Debate/contested
  • Technical explanation

Main Points Raised

  • Some participants note that NASA defines the equilibrium density at 9.9 x 10<30> gm/cm3, questioning how this density can remain steady as the universe expands.
  • Others propose that dark energy, which constitutes a significant portion of the stress-energy tensor, maintains a constant density during the universe's expansion, despite its accelerating nature.
  • A participant suggests that if dark energy is indeed increasing, it implies the generation of new dark energy, which raises questions about the constancy of density and contradicts basic scientific principles regarding volume expansion.
  • Another participant emphasizes the need for an explanation of the relationship between dark energy and dark matter, referencing findings such as galactic rotational curves and the challenges in identifying dark matter entities.
  • One participant asserts that dark matter and dark energy are unrelated, arguing that the confusion arises from their similar nomenclature and that there is no increase in dark matter corresponding to dark energy.
  • Another participant questions the ability to define dark matter and dark energy clearly, suggesting that without a proper understanding, the potential interactions between them remain uncertain.
  • A later reply mentions a lecture that could provide foundational elements for further discussion, although it does not directly address the original question.

Areas of Agreement / Disagreement

Participants express differing views on the relationship between dark energy and dark matter, with some arguing for a connection and others asserting they are distinct concepts. The discussion remains unresolved regarding the implications of dark energy's constancy and its relationship to the expanding universe.

Contextual Notes

There are limitations in the definitions and understanding of dark matter and dark energy, which may affect the discussion. The mathematical implications and the nature of their interactions remain unresolved.

Dr Aaron
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With NASA defining this equilibrium density at 9.9 x 10<30 gm/cm3, how can an increasingly expanding universe maintain a steady density as it expands?
 
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Dr Aaron said:
With NASA defining this equilibrium density at 9.9 x 10<30 gm/cm3, how can an increasingly expanding universe maintain a steady density as it expands?
"Dark Energy" is an unknown something that causes the expansion of the universe to accelerate. It makes up something like 70% of everything in the stress energy tensor, and for unknown reasons, it maintains a constant density as the universe expands.
 
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Doesn't that suggest that new dark energy is being generated within the universe for there to be an increasing rate of expansion? Then the density could not remain constant without new material to equilibrate the expanding volume. A fixed amount of "stuff" should drop in density when volume expands, yet this seems to contradict pretty basic scientific laws.
 
Dr Aaron said:
Doesn't that suggest that new dark energy is being generated within the universe for there to be an increasing rate of expansion? Then the density could not remain constant without new material to equilibrate the expanding volume. A fixed amount of "stuff" should drop in density when volume expands, yet this seems to contradict pretty basic scientific laws.
Yes, the fact that dark energy maintains a constant density as the universe expands does seem weird. If you can find an explanation for it, I guarantee you a Nobel Prize in physics.
 
If it is happening there must be an explanation. The increasing dark energy that expands the universe should be countered by the dark matter noted by findings such as galactic rotational curves, as described by Vera Rubin. I have heard discussions about this, but while we can identify increased dark matter by the expansion of space-time, as we try to identify the entities of dark matter we are having such difficulties in finding dark matter that the only way to measure dark matter is through functions such as evaluation of Einstein-Chowlson rings. Are these findings precise enough to recognize a similar increase for dark matter as we see with dark energy?
 
Dr Aaron said:
If it is happening there must be an explanation. The increasing dark energy that expands the universe should be countered by the dark matter noted by findings such as galactic rotational curves, as described by Vera Rubin. I have heard discussions about this, but while we can identify increased dark matter by the expansion of space-time, as we try to identify the entities of dark matter we are having such difficulties in finding dark matter that the only way to measure dark matter is through functions such as evaluation of Einstein-Chowlson rings. Are these findings precise enough to recognize a similar increase for dark matter as we see with dark energy?
Dark matter and dark energy have NOTHING to do with each other and the unfortunate use of the similar names has cause more wasted keystrokes here on PF that any other single topic. There is no increase in DM to correspond to the increasing amount of DE.
 
Dr Aaron said:
If it is happening there must be an explanation.
I agree, and again, if you can find it, I guarantee you a Nobel Prize.
 
If we cannot define dark matter and dark energy well, how could we assure ourselves that do not have a relationship? We cannot estimate exactly what dark matter is so whether it might interact with itself or with dark energy has not been confirmed to the positive or negative, to my knowledge. However, if you and I can figure it out, we can share the Nobel money! ;-)
 
Perhaps an interesting basic lecture, just for the pedagogy: arXiv:astro-ph/0703739v2, 14 Dec 2007, "Adventures in Friedmann cosmology: A detailed expansion of the cosmological Friedmann equations"; 32 pages. It doesn't give an answer to the initial question (of course) but it presents some basic elements with which a discussion can eventually start.
 

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