Revisiting WMAP Data Reveals Significant Changes in CMB Power Spectrum

  • Thread starter nicksauce
  • Start date
  • Tags
    Data
In summary, a recent study has found that the temperature maps of the cosmic microwave background (CMB) published by the WMAP team may have a systematic error. The study developed its own map-making and power spectrum estimation software and found significant differences between their maps and the official WMAP maps. These differences resulted in changes to the best-fit cosmological parameters, indicating the need for further revision in the current cosmological model. However, some skeptics have pointed out that the study lacks details and rigor, and it is unlikely that multiple independent groups would have made the same mistake in their map-making.
  • #1
nicksauce
Science Advisor
Homework Helper
1,271
7
This is interesting: http://arxiv.org/abs/0907.2731 ... Apparently there could have been a systematic error in the WMAP temperature maps.

The cosmic microwave background (CMB) temperature maps published by the Wilkinson Microwave Anisotropy Probe (WMAP) team are found to be inconsistent with the differential time-ordered data (TOD), from which the maps are reconstructed. The inconsistency indicates that there is a serious problem in the map making routine of the WMAP team, and it is necessary to reprocess the WMAP data. We develop a self-consistent software package of map-making and power spectrum estimation independently of the WMAP team. Our software passes a variety of tests. New CMB maps are then reconstructed, which are significantly different with the official WMAP maps. In the new maps, the inconsistency disappeared, along with the hitherto unexplained high level alignment between the CMB quadrupole and octopole components detected in released WMAP maps. An improved CMB cross-power spectrum is then derived from the new maps which better agrees with that of BOOMRANG. Two important results are hence obtained: the CMB quadrupole drops to nearly zero, and the power in multiple moment range between 200 and 675 decreases on average by about 13%, causing the best-fit cosmological parameters to change considerably, e.g., the total matter density increases from 0.26 up to 0.32 and the dark energy density decreases from 0.74 down to 0.68. These new parameters match with improved accuracy those of other independent experiments. Our results indicate that there is still room for significant revision in the cosmological model parameters.
 
Space news on Phys.org
  • #2
Well, I was looking over this with a friend last week, and we generally agree: the paper is very light on details, not well-written, and generally lacking in overall rigor. It leaves the impression that they didn't put enough work into the research to really show what they claim to show.

And the thing that worries me is that I'm pretty sure that a number of independent groups have done map making on the WMAP timelines, and it seems rather unlikely to me that they all would have made the same mistake (this paper claims that the error isn't in the algorithm, as they claim to replicate the WMAP team's mapmaking algorithm, but rather in the implementation).
 

Related to Revisiting WMAP Data Reveals Significant Changes in CMB Power Spectrum

1. What is WMAP data and what does it reveal?

WMAP (Wilkinson Microwave Anisotropy Probe) is a satellite mission launched in 2001 to measure the temperature and polarization of the cosmic microwave background (CMB) radiation. The data from WMAP has revealed significant changes in the power spectrum of the CMB, providing valuable insights into the early universe.

2. What is the CMB power spectrum and why is it important?

The CMB power spectrum is a plot of the temperature fluctuations in the CMB as a function of angular scale. It is important because it contains information about the distribution of matter and energy in the early universe, and can help us understand the processes that shaped the universe.

3. What are the significant changes in the CMB power spectrum revealed by the WMAP data?

The WMAP data has shown that the CMB power spectrum is not a simple, smooth curve as previously thought. It has significant fluctuations and anomalies, such as a lack of power at large angular scales and an excess of power at small angular scales, which challenge our current understanding of the universe.

4. What implications do these changes in the CMB power spectrum have for cosmology?

The changes in the CMB power spectrum suggest that there may be new physics at play in the early universe that we do not yet understand. This could lead to revisions of current cosmological models and a deeper understanding of the fundamental laws of the universe.

5. How can we further study and confirm these changes in the CMB power spectrum?

Further analysis of the WMAP data and future observations from other experiments, such as the Planck satellite, will help us confirm and better understand the changes in the CMB power spectrum. Additionally, new theoretical models and simulations can be developed to explain these findings and guide future research.

Similar threads

Replies
4
Views
4K
Replies
13
Views
2K
Replies
2
Views
3K
  • Cosmology
Replies
11
Views
5K
Replies
8
Views
3K
Replies
1
Views
1K
Replies
2
Views
2K
Back
Top