Gravitating Matter in LQG & String: How Critical is the Density?

In summary, Gravitating matter is needed for our universe to be as it is, and LQG and String theories are not sufficiently developed to provide a figure for the critical density. However, ordinary 1915 Gen. Rel. does provide a basis for calculating the critical density. The usual estimate is that this 0.83 joules is broken down between 73 percent dark energy and 27 percent matter (of which most is dark matter). So if you want to know how much "matter" (dark and baryonic combined) then it is 27 percent of 0.83 joules. This is about 0.22 joules per cubic kilometer.
  • #1
wolram
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I think this is the right place to ask, how much "gravitating", matter
is needed, in LQG and String, for our universe to be as it is. and how
critical is this "density".
 
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  • #2
wolram said:
I think this is the right place to ask, how much "gravitating", matter
is needed, in LQG and String, for our universe to be as it is. and how
critical is this "density".

wolram, I do not think that either LQG or stringy theories are sufficiently well-developed to provide a figure for the critical density

however, ordinary 1915 Gen. Rel. does provide a basis for calculating the critical density
the formula for calculating it basically just the Friedmann equation and it gives a figure of about

0.83 joules per cubic kilometer.

the usual estimate is that this 0.83 joules is broken down between 73 percent dark energy and 27 percent matter (of which most is dark matter)

so if you want to know how much "matter" (dark and baryonic combined) then it is 27 percent of 0.83 joules

this is about 0.22 joules per cubic kilometer. (baryonic and dark matter combined)


the word "density" just means so-and-so much of something per unit volume
and there is no certain total volume, one can only guess about whether it is finite or infinite and what it is if it is finite.
so one is better off just talking about density----so and so much per cubic km or cubic lightyear.
besides, it is the density at each point that determines the curvature at that point. So the density is the relevant thing, not the total.

the density, whether it is measured or inferred, turns out to be amazingly sparse by human standards. 0.22 joules is a small amount of energy already and it would seem even more tiny if expressed as a mass equivalent (miniscule fraction of a nanogram)---but all that means is that space, on average, is extraordinarily empty and if it were not so empty then it would not appear flat

what they mean by "critical density" is the value which is necessary for the universe to be flat
and since it appears to be flat (people keep checking this in everyway they can think of) the actual density is believed to be at or close to the critical level.
 
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  • #3
This is disappointing i thought that at least LQG or STRING could
predict a value for cosmological constants, if it cannot what is reason of pursing them?
 
  • #4
wolram said:
This is disappointing i thought that at least LQG or STRING could
predict a value for cosmological constants, if it cannot what is reason of pursing them?

LQG is still working hard on showing from first principles that four dimensional time-space exists. String theory isn't much better off. Both are working hard to show that what they predict resembles GR. THe reason to pursue them is the hope that someday you will have a theory that gives you the source code for the universe.
 

Related to Gravitating Matter in LQG & String: How Critical is the Density?

1. What is LQG and how does it relate to gravitating matter?

LQG stands for Loop Quantum Gravity and is a theory that attempts to reconcile general relativity with quantum mechanics. In this theory, space and time are quantized, meaning they are made up of discrete units rather than being continuous. LQG proposes that gravitating matter is made up of tiny loops or strings, which interact with each other to create the force of gravity.

2. How does string theory contribute to our understanding of critical density?

String theory is another attempt to reconcile general relativity and quantum mechanics. It proposes that the fundamental building blocks of the universe are not particles, but tiny, one-dimensional strings. In this theory, critical density refers to the minimum amount of matter needed for the universe to maintain a stable, flat shape. String theory helps us understand this critical density by providing a framework for calculating the effects of gravitating matter on the curvature of space.

3. What is the significance of critical density in the study of gravitating matter?

Critical density is important because it determines the fate of the universe. If the amount of gravitating matter in the universe is less than critical density, the universe will continue to expand indefinitely. If the amount of matter is greater than critical density, gravity will eventually cause the expansion to slow down and the universe may eventually collapse in a "Big Crunch." Understanding the critical density of gravitating matter is crucial in predicting the future of our universe.

4. How do scientists measure the density of gravitating matter in the universe?

Scientists use various methods to measure the density of gravitating matter in the universe. One method is to observe the rotation of galaxies and measure the amount of mass needed to keep the galaxies from flying apart. Another method is to study the cosmic microwave background radiation, which is leftover radiation from the Big Bang. By analyzing the fluctuations in this radiation, scientists can determine the density of matter in the early universe.

5. What are some current research efforts focused on understanding the critical density of gravitating matter?

Scientists are currently conducting various experiments and observations to improve our understanding of the critical density of gravitating matter. This includes studying the properties of dark matter, which makes up a significant portion of the universe's mass but is still largely unknown. Other research efforts involve studying the large-scale structure of the universe, such as galaxy clusters and superclusters, to gather more evidence on the distribution of matter. Additionally, scientists are using advanced mathematical models and computer simulations to better understand the effects of gravitating matter on the evolution of the universe.

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