Wald General Relativity: On the homogenous cosmology, Page 178

In summary, Wald's statement in the picture has two contradictions. However, it is easy to find a solution that has two positive p_{\alpha} and one negative.
  • #1
qinglong.1397
108
1
Hi, everybody. I have some problem with Wald's statement shown in the picture. This is from the last paragraph in Page 178.

He claimed that there are only solutions with two of the [itex]p_{\alpha}[/itex] positive and one negative. But it's easy to find out that if two of the [itex]p_{\alpha}[/itex] are negative while the third positive, there is no contradiction.

Can you guys help me with this? Why should all the solutions have two positive [itex]p_{\alpha}[/itex] and one negative? Thank you:smile:

(The picture is from http://books.google.com/books?id=9S...ce=gbs_ge_summary_r&cad=0#v=onepage&q&f=false)
 

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  • #2
Well using (7.2.58) and (7.2.60) we have ##p_2^2 + p_1^2 - p_1 - p_2 + p_1p_2 = 0##. Now if ##p_3 < 0## then ##p_2 > 1 - p_1##. Plot these two and you will find that both ##p_1,p_2 > 0##. If ##p_3 >0## then ##1 - p_1> p_2##; plotting these two again you will find that ##p_1 > 0,p_2 < 0## or vice-versa. Finally if ##p_3 = 0## then either ##p_1 = 1## and ##p_2 = 0## or vice-versa which are just the trivial solutions.
 
  • #3
WannabeNewton said:
Well using (7.2.58) and (7.2.60) we have ##p_2^2 + p_1^2 - p_1 - p_2 + p_1p_2 = 0##. Now if ##p_3 < 0## then ##p_2 > 1 - p_1##. Plot these two and you will find that both ##p_1,p_2 > 0##. If ##p_3 >0## then ##1 - p_1> p_2##; plotting these two again you will find that ##p_1 > 0,p_2 < 0## or vice-versa. Finally if ##p_3 = 0## then either ##p_1 = 1## and ##p_2 = 0## or vice-versa which are just the trivial solutions.

Thanks! Never thought of this. Great!
 
  • #4
No problem! Make sure you do the problems at the end of that chapter; some of them are really fun (problems 7.1,7.4, and 7.5 in particular).
 
  • #5
WannabeNewton said:
No problem! Make sure you do the problems at the end of that chapter; some of them are really fun (problems 7.1,7.4, and 7.5 in particular).

Sure. I'll try to solve all of them before the end of the next week.
 
  • #6
Awesome, have fun with that!
 
  • #7
WannabeNewton said:
Awesome, have fun with that!

Hi WannabeNewton, I know it's been late, but I haven't been able to figure out how to solve the problem 7.4. Can you help me out? Thank you!
 

Related to Wald General Relativity: On the homogenous cosmology, Page 178

1. What is the concept of homogenous cosmology in Wald's General Relativity?

The concept of homogenous cosmology refers to the assumption that the universe is spatially homogeneous, meaning that the distribution of matter and energy is the same at every point in space. This assumption is based on the cosmological principle, which states that the universe is isotropic (the same in all directions) and homogeneous on large scales.

2. How does homogenous cosmology affect our understanding of the universe?

Homogenous cosmology is a key assumption in our current understanding of the universe and its evolution. It allows us to simplify the equations of general relativity and make predictions about the large-scale structure of the universe, such as the expansion rate and the formation of galaxies and clusters of galaxies.

3. What evidence supports the homogenous cosmology assumption?

Observations of the cosmic microwave background radiation, which is the leftover radiation from the early universe, show that the universe is highly homogeneous on large scales, with tiny variations in temperature. This supports the idea that the universe was once in a hot, dense, and uniform state and has since expanded and cooled.

4. Are there any exceptions to the homogenous cosmology assumption?

While homogenous cosmology is a useful assumption for understanding the overall structure of the universe, it is not always accurate on small scales or in regions with high concentrations of matter such as galaxies and galaxy clusters. In these cases, the distribution of matter is not completely uniform and can have significant effects on the local dynamics of the universe.

5. How does homogenous cosmology relate to the concept of dark energy?

Homogenous cosmology is closely related to the concept of dark energy, which is a hypothetical form of energy that is thought to be responsible for the accelerating expansion of the universe. The assumption of homogeneity, along with the principle of cosmic isotropy, is used in the mathematical models that attempt to explain the observed acceleration and the role of dark energy in the universe.

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