Can Cosmological Constant contract (negative)?

In summary, the cosmological constant may not be able to contract or have a negative value equal to 120 magnitude, which would warp spacetime after the Big Bang.
  • #1
cube137
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Hello...

Can the cosmological constant become so rigid as to resist the 120 magnitude quantum contribution? Where is the mathematical terms for it in GR EFEs? is the effect like contraction instead of expansion? Because the 120 magnitude quantum contribution should immediately warp spacetime after Big Bang.. but it is somehow cancelled.. maybe the cosmological constant can contract or negative value equal to 120 magnitude too?
 
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  • #2
Hi cube137,

As I understand it the problem of 120 oom is not within GR to explain but it is a problem in QFT.
QFT vacuum energy is much higher than the measured cosmological one.
 
  • #3
Yes, and it's really the most enigmatic problem of contemporary physics. The isssue is still more or less in the same status as is written in Weinberg's famous review on it:

The cosmological constant problem. Steven Weinberg. Rev. Mod. Phys. 61, 1 – Published 1 January 1989.
http://dx.doi.org/10.1103/RevModPhys.61.1
http://www.itp.kit.edu/~schreck/general_relativity_seminar/The_cosmological_constant_problem.pdf
 
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  • #4
vanhees71 said:
Yes, and it's really the most enigmatic problem of contemporary physics. The isssue is still more or less in the same status as is written in Weinberg's famous review on it:

The cosmological constant problem. Steven Weinberg. Rev. Mod. Phys. 61, 1 – Published 1 January 1989.
http://dx.doi.org/10.1103/RevModPhys.61.1
http://www.itp.kit.edu/~schreck/general_relativity_seminar/The_cosmological_constant_problem.pdf

I read them.. but something I still can't understand. In the Anthropic argument.. how come they just stated the cosmological constant is small in our universe.. why didn't they consider the 120 magnitude quantum contributions.. what is the exactly formula of the cosmological constant.. where is the variable that is negative or the one where you plug the negative 120 magnitude (to the quantum contributions) and still making the cosmological constant small?
 
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  • #5
You are misunderstanding.

We go out and measure the cosmological constant by looking at the redshift of supernovae and applying the equations of general relativity. The result is that the cosmological constant is very, very small.

Then we go and look at quantum theory and calculate the energy of the vacuum, which we think ought to be the same as the cosmological constant. The answer is very, very big - 120 orders of magnitude bigger than the GR-based measurements.

There is no way to make the large value into the small one. These two results just contradict each other. There is something we don't understand going on here. Hopefully quantum gravity will explain it all - but we don't have that theory yet.
 
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  • #6
Ibix said:
You are misunderstanding.

We go out and measure the cosmological constant by looking at the redshift of supernovae and applying the equations of general relativity. The result is that the cosmological constant is very, very small.

Then we go and look at quantum theory and calculate the energy of the vacuum, which we think ought to be the same as the cosmological constant. The answer is very, very big - 120 orders of magnitude bigger than the GR-based measurements.

There is no way to make the large value into the small one. These two results just contradict each other. There is something we don't understand going on here. Hopefully quantum gravity will explain it all - but we don't have that theory yet.

But that's the point. In the Anthropic multiverse arguments.. there are billions of universes with different values of the constants.. we just happened to be in a universe with small constant.. but still it doesn't take into account the 120 magnitude quantum contributions.. so what is the point of the Anthropic argument.. it is supposed to solve what happened to the 120 magnitude quantum contributions and why is the cosmological constant small in spite of it.
 

1. Can the cosmological constant contract or become negative?

Yes, it is possible for the cosmological constant to contract or become negative. In fact, some theories suggest that the cosmological constant may have changed over time, leading to the expansion of the universe.

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

A negative cosmological constant would have the opposite effect of a positive one, causing the universe to contract rather than expand. This could potentially lead to a collapse of the universe.

3. Can a negative cosmological constant explain the accelerated expansion of the universe?

While a negative cosmological constant can cause the universe to contract, it cannot fully explain the accelerated expansion of the universe. Other factors, such as dark energy, are also believed to play a role in the expansion.

4. How is the cosmological constant related to dark energy?

The cosmological constant is a term in Einstein's equations of general relativity that describes the energy density of empty space. It is often used interchangeably with the term "dark energy," which refers to the unknown force causing the accelerated expansion of the universe.

5. Are there any ongoing studies or experiments related to the cosmological constant?

Yes, there are ongoing studies and experiments to better understand the nature of the cosmological constant and its role in the universe. For example, the Dark Energy Survey and the European Space Agency's Euclid mission are both dedicated to studying dark energy and its effects on the expansion of the universe.

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