SPT-SZ Survey Results: New Neutrino Species Suggested

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In summary: No particularly shocking revelations, however, the suggestion of new neutrino species is interesting.
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Results from the spt-sz survey are in - http://arxiv.org/abs/1212.6267. No particularly shocking revelations, however, the suggestion of new neutrino species is interesting.
 
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There was an earlier report in October (Story et al) that discussed the curvature estimate in more detail. This new paper basically just refers the reader to the October one.

==quote http://arxiv.org/pdf/1212.6267v1.pdf page 9==
5. CURVATURE
The SPT+WMAP7 constraint on the mean curvature of the universe has been presented by Story et al. (2012). ...
...
...
...Better constraints on curvature are possible by including low-redshift probes. For instance, CMB+BAO+H0 leads to a constraint on curvature of Ωk = −0.0061 ± 0.0040. Even with low-redshift datasets included, SPT data remains important. Without the SPT bandpowers (and lensing information therein), the uncertainty would be roughly 15% larger: Ωk = −0.0019 ± 0.0047 for WMAP7+BAO+H0.
==endquote==

So without the new SPT data you have the WMAP7+BAO+H0 result. Including the SPT data you have what they denote CMB+BAO+H0 which I highlighted in blue. This bounds the average curvature away from zero (i.e. flat) at 2σ or 95% confidence.

Since they begin by referring to the Story et al paper, which gave a longer more detailed treatment with essentially the same bottom line, I'll quote equation (21) in that Story et al.

==quote http://arxiv.org/pdf/1210.7231.pdf page 14==
The tightest constraint on the mean curvature that we consider comes from combining the CMB, H0 , and BAO datasets:
Ωk =−0.0059±0.0040. (21)
==endquote==

So the central value in the new paper, -0.0061, is just slightly more negative than the one in the October paper, -0.0059.

The way Ωk is defined, a negative value corresponds to positive mean curvature and
Ωtotal = 1 - Ωk
So a central value of -0.006 corresponds to Ωtotal = 1.006.

We still can't say anything with much assurance because if you do not include SPT data and make different choice of data set---e.g. just use WMAP, or some other combination--you get a wider errorbar and the central values are all over the place.

It just happens that for some reason the SPT in conjunction with the other main data gives this comparatively tight constraint of ±0.0040 that both papers report, and a positive curvature which translates to a finite spatial volume universe with a finite circumference.

The 95% confidence smallest positive curvature with Ωk = -0.006 + 0.004 = -0.002
would lead to the largest estimated circumference. Basically 2π time Hubble distance (say 14 Gly) divided by sqrt(.002)
That is, 88 billion lightyears divided by sqrt(.002) = 1968 billion light years.

The 95% confidence largest positive curvature with Ωk = -0.006 - 0.004 = -0.01
would lead to the smallest estimated circumference. Again 2π time Hubble distance (say 14 Gly) or 88 Gly, but this time divided by sqrt(.01)
That is, 88 billion lightyears divided by sqrt(.01) = 880 billion light years.

So although it's still very much undecided, one of the things about the SPT reports that continues to fascinate me is that it appears to be excluding a spatially flat, spatially infinite universe at 2 sigma or 95% confidence.

Assume that the piece of it we can observe is representative, curvature-wise.
 
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  • #3
New neutrino species? Where would it fit in at in the standard model? (Am I understanding that right?)
 
  • #4
This is another potential indicator favoring the existence of sterile neutrinos, which could be a significant fraction of dark matter. It would constitute new physics beyond the standard model.
 
  • #5
Nice.
 

1. What is the SPT-SZ survey and how does it relate to neutrino research?

The SPT-SZ survey, or South Pole Telescope-Sunyaev Zel'dovich survey, is a large-scale project that uses a telescope located at the South Pole to study cosmic microwave background radiation. This radiation is a remnant of the early universe and can provide important insights into the properties of neutrinos, which are subatomic particles with very little mass. The SPT-SZ survey specifically focuses on the search for new neutrino species, which could help us better understand the fundamental building blocks of the universe.

2. What are the main findings of the SPT-SZ survey results regarding new neutrino species?

The main finding of the SPT-SZ survey results is the suggestion of a new neutrino species. This is based on the detection of a specific pattern in the cosmic microwave background radiation, known as the "neutrino bump." This pattern is consistent with the presence of an additional type of neutrino with a mass of around 0.1 electron volts. However, further research and confirmation are needed to fully establish the existence of this new neutrino species.

3. How significant is the discovery of a new neutrino species in the SPT-SZ survey results?

The suggestion of a new neutrino species in the SPT-SZ survey results is a significant finding in the field of particle physics. If confirmed, it would be the first new type of neutrino discovered since the 1990s and could provide important insights into the properties of neutrinos, such as their mass and interaction with other particles. It could also have implications for our understanding of the early universe and the formation of galaxies.

4. What are the potential implications of the SPT-SZ survey results for future research?

The SPT-SZ survey results could have significant implications for future research in the field of neutrino physics. If the existence of a new neutrino species is confirmed, it could open up new avenues for studying the properties of neutrinos and their role in the universe. It could also lead to the development of new technologies and experiments to further investigate this new particle and its potential impact on our understanding of the universe.

5. What are the next steps in confirming the existence of a new neutrino species suggested by the SPT-SZ survey results?

The next steps in confirming the existence of a new neutrino species suggested by the SPT-SZ survey results involve further research and collaboration among scientists in the field. This could include conducting additional experiments and observations, as well as analyzing data from other sources to see if they support the findings of the SPT-SZ survey. It could also involve developing new theories and models to explain the potential properties and behavior of this new neutrino species. Ultimately, the confirmation of its existence will require multiple lines of evidence and the consensus of the scientific community.

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