What impact on QG if the CMB map is revised?

In summary, the paper found that the Cosmic Microwave map will have to be revised with even less quadrupole and octopole power. This could have a major impact on the Standard Model of Cosmology. If Bojowald is correct, then the LQG signature may be able to be found in the CMB. However, this is still a mystery and more research is needed.
  • #1
marcus
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A paper just came out this month that makes it more certain that the Cosmic Microwave map will have to be revised, with even less quadrupole and octopole power.

http://www.arxiv.org/abs/astro-ph/0508047/
On the large-angle anomalies of the microwave sky

I opened a thread on this paper in the Astronomy section
https://www.physicsforums.com/showthread.php?t=86191
where it may be of general interest, since the Standard Model of cosmology will have to be made over if there is substantial revision of the CMB map. (that thread has reference to earlier papers about this by the same people, the issue has been around for a couple of years)

what I want to know in this thread is if anyone has some idea as to the impact on quantum gravity. or even just explain some basics to us.

According to some work by Bojowald, and by Singh (I think also perhaps Maartens, Tsujikawa) Loop Quantum Cosmology is near the point of being able to predict some LQG signature to be looked for in the CMB.
This because the LQG big bang and the LQG inflation picture is slightly different from classical. Parampreet Singh gave a series of seminar talks on this at Penn State that is online and that I listened to the first two of.

So if the CMB map is going to be radically revised, what happens to the LQG signature that people like Parampreet Singh were hoping to find in the CMB map? Do they have the rug pulled out from under? That depends on a lot of stuff I don't know. Does anybody else know something about this?
If he is the only person who understands the situation, maybe we should write to Parampreet.
 
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  • #2
Hi Marcus

One of the authors is Starkman whom we discussed once previously because there was a New Scientist article about this.

Summarising the conclusions: the authors pretty well rule out (a) systematic error and (b) statistical flukes. This leaves two possibilities:

1) an unexpected foreground astrophysical source
2) a cosmological explanation

Either of these possibilities means a very serious reinterpretation of the WMAP data. Cool! This has to be the most astonishing observational conundrum around. :smile:
 
  • #3
I think that the relations between the CMB and quantum gravity should not be considered too strong. As you say, there are LQG (and maybe string)-inspired models modifying the low-l CMB spectrum, but it is important to note that these 'explanations' for the observational discrepancies are not at all unique. I recall cosmologists having a rather large list of relatively mundane explanations that make the same predictions (at least to the observational precision acheivable in the forseeable future).

As this paper points out, there are also a lot of systematic issues with measuring the lower multipole moments. It is an interesting thing to study, though. In my personal opinion, the assumptions used in the standard cosmological model are likely to have problems in this regime.
 
  • #4
  • #5
Kea said:
Hi Marcus

One of the authors is Starkman whom we discussed once previously because there was a New Scientist article about this.

Summarising the conclusions: the authors pretty well rule out (a) systematic error and (b) statistical flukes. This leaves two possibilities:

1) an unexpected foreground astrophysical source
2) a cosmological explanation

Either of these possibilities means a very serious reinterpretation of the WMAP data. Cool! This has to be the most astonishing observational conundrum around. :smile:
Hi Kea! I vote for both possibilities. There is more than ample evidence for each. Modern cosmology is more exciting than texas holdem [except on Tuesdays].
 

1. What is the CMB map and how is it related to QG?

The CMB map, or cosmic microwave background map, is a map of the oldest light in the universe, which was emitted about 380,000 years after the Big Bang. This map provides valuable information about the early universe and is used to study theories of quantum gravity (QG), which aim to unify quantum mechanics and general relativity.

2. How often is the CMB map revised?

The CMB map is constantly being revised as new data is collected from various experiments and telescopes. However, major revisions to the map typically occur every few years as more data is analyzed and technology improves.

3. What impact does a revised CMB map have on QG theories?

A revised CMB map can have a significant impact on QG theories as it provides new information and constraints on the early universe. This can challenge existing theories and lead to the development of new ones.

4. How do scientists revise the CMB map?

The CMB map is revised through a process called data analysis. This involves collecting data from various experiments and telescopes, removing any noise or interference, and then analyzing the data to create an updated map. This process is repeated as new data becomes available.

5. Can a revised CMB map disprove current QG theories?

A revised CMB map can certainly challenge and potentially disprove current QG theories, but it is not the only factor that determines the validity of these theories. Other experiments and observations must also be considered in order to fully understand the implications of a revised CMB map on QG.

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