Cosmological Constant and the like

In summary, the conversation discusses the impact of the cosmological constant on various calculations and theories related to dark energy. It also explores the relationship between dark energy and the Higgs field, and the implications of dark energy on the overall fate of the universe. There are different theories and uncertainties surrounding these topics, leading to ongoing discussions and debates in the scientific community.
  • #1
blumfeld0
148
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I have a few questions that have been piling up.

1.
Einstein introduced the cosmoligical constant to demand a static universe like so, G + (Lambda * metric tensor) = T
If you were to calculate the perihelion precession of mercury, bending of starlight etc. with this additional term would you get the same results or would you get significantly different numbers in the end?
I suspect they would be different but hardly noticeable in the final numbers but I am not sure. Has anyone tried to do this? If so, what does it mean for the cosmological constant lamba.


2. Is dark energy the physial manifestation of the cosmological constant? Is dark energy the same as the higgs field (not the electroweak or grand unified higgs field, responsible for giving particles mass) but the higgs field responsible for Inflation in the early universe?
I thought the answer to the first question was yes but the consensus seems to change every month

Lastly,
3. What implications does dark energy have on the overall curvature and fate of the universe? Doesnt it throw everything we know into panic mode? We know the vast majority of the universe is composed of dark energy so what implications does that have?



blumfeld0
 
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  • #2
Perhaps you've seen it already, but if not, check out my brief review of dark energy https://www.physicsforums.com/showpost.php?p=893482&postcount=82".


blumfeld0 said:
If you were to calculate the perihelion precession of mercury, bending of starlight etc. with this additional term would you get the same results or would you get significantly different numbers in the end?
I suspect they would be different but hardly noticeable in the final numbers but I am not sure.

You're correct. There's some detailed discussion of the impact of dark energy on orbits in this thread:

https://www.physicsforums.com/showthread.php?t=103450"


2. Is dark energy the physial manifestation of the cosmological constant?

In the simplest model, yes. However, there are many reasonable theories in which the dark energy density is not a constant (w != -1). These are generally referred to as "quintessence" models.


Is dark energy the same as the higgs field (not the electroweak or grand unified higgs field, responsible for giving particles mass) but the higgs field responsible for Inflation in the early universe?

No, it most probably isn't related to the scalar field that caused inflation.


3. What implications does dark energy have on the overall curvature and fate of the universe? Doesnt it throw everything we know into panic mode? We know the vast majority of the universe is composed of dark energy so what implications does that have?

The end fate of the universe is something we can only speculate about because there is always the possibility some other "dark" component will become dominant in the far future. If the current cosmological model is the whole picture (unlikely), then the universe will suffer a heat death, just as in the open universe model. Lots more information here:

http://math.ucr.edu/home/baez/end.html"
 
Last edited by a moderator:

1. What is the cosmological constant?

The cosmological constant is a term in Einstein's theory of general relativity that represents the energy density of the vacuum of space. It was originally introduced by Einstein to account for a static universe, but later it was found that the universe is expanding and the cosmological constant is responsible for this expansion.

2. How does the cosmological constant affect the expansion of the universe?

The cosmological constant is a positive energy density that acts as a repulsive force, causing the expansion of the universe to accelerate. This acceleration was first observed in 1998 and has since been confirmed by other experiments.

3. Can the value of the cosmological constant change over time?

According to current theories, the value of the cosmological constant is a constant and does not change over time. However, some theories suggest that it may slowly decrease over time, which would eventually lead to a reversal of the universe's expansion.

4. How does the cosmological constant relate to dark energy?

The cosmological constant is the leading explanation for dark energy, the mysterious force that is causing the expansion of the universe to accelerate. It is believed that the cosmological constant makes up about 70% of the total energy density of the universe, with the remaining 30% being dark matter and regular matter.

5. What does the value of the cosmological constant tell us about the fate of the universe?

The value of the cosmological constant is directly related to the fate of the universe. If the value is positive and large enough, the expansion of the universe will continue to accelerate and eventually lead to a "big rip" where the universe is torn apart. If the value is smaller, the expansion may eventually slow down and stop, resulting in a "big crunch" where the universe collapses back in on itself. If the value is zero or negative, the universe will continue to expand at a constant rate.

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