Dark Matter Detection Experiment Results?

In summary, the latest LUX results show that the experiment is still active and looking for dark matter, but there is some doubt about the results.
  • #1
secur
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In 2011 Dr. Gerald Guralnik of Brown University was involved in an ongoing Dark Matter Detection experiment, perhaps LUX? It was an international collaboration involving underground detectors. He was certain DM would be detected in 5 years - i.e., now. I was dubious, so we bet "bragging rights" on it.

Tragically, Jerry passed away in 2014. He was a great physicist and a great guy as well.

Now, I'm wondering what the status of that experiment is. Obviously nothing dramatic or I would have seen it in the news; and don't see up-to-date info on the net (if it was LUX). Can anyone tell me how it's doing, whether work is ongoing, and whether I would have won my bet?
 
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  • #3
thanks Orodruin, that's exactly what I needed. I'd noticed this before on the net: "We present constraints on WIMP-nucleus scattering from the 2013 ... LUX"); 2013 is a long time ago. But the crucial information I was missing is: "last revised 26 Jan 2016". It's pretty clear what's happened between 2013 and 2016 ...
 
  • #4
As far as I know, only the DAMA/LIBRA and DAMA/NaI experiments have made claims of a direct detection, by way of an annual modulation in signal around 40 keV. These results are in tension with the other direct detection experiments. There is a new experiment called SABRE that will have active background suppression (http://www.pa.ucla.edu/sites/default/files/webform/jingke_xu.pdf ) that will test the DAMA/LIBRA claims. Happily, there will be a southern hemisphere component that should deal with seasonal background contributions.
 
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  • #6
e.bar.goum said:
... There is a new experiment called SABRE that will have active background suppression (http://www.pa.ucla.edu/sites/default/files/webform/jingke_xu.pdf ) that will test the DAMA/LIBRA claims. ...
Chapter 2 of Emily Shields thesis is very informative and pedagogical, it doesn't need a high level of prior knowledge. She has worked with Jing ke Xu and they use some of the same graphs. You may have seen it.
https://www.princeton.edu/physics/graduate-program/theses/theses-from-2015/Shields-Thesis.pdf

She seems to be part of the group working on SABRE.
 
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  • #7
Thanks for responses, e.bar.goun, Chronos, marcus

Just to clarify, I mainly wanted to know if I'd won my bet re. LUX. I made one other bet with Dr. Guralnik, that the Higgs boson wouldn't be found by LHC! Of course I lost. As you probably know he was one of the people, as well as Peter Higgs, who helped work out the Higgs symmetry-breaking mechanism back in 1964, and deserved the Nobel as much as anyone. So it's great that he lived long enough to see the July 4, 2012 announcement.

marcus, Emily Shields thesis is great for getting up to speed on DM detection, very readable and covers all the bases. Having looked at it all of a sudden I'm much more interested in the whole question.

I'm afraid the DAMA work is not too convincing yet, but let's hope SABRE backs it up. DAMA is obviously very difficult and subject to uncertainties, and of course I know little about it (just this thesis). But one thing I can say, Dr. Guralnik worked on LUX, and it seems to conflict with DAMA. Just as a general rule, if his work disagrees with anyone at all - I'll put my money on him. (If he told me God made a mistake, I'd believe him.)

Can't help making a comment ... The thesis contains 10 pages (!) of acknowledgments, including this: "I thank you. Words cannot express how much you mean to me, but fortunately I think you already know. I love you, and I can’t wait to meet our next adventure together." - to Jason. I shudder to think what would have happened, back in the day, if I'd included 10 pages of such acknowledgments. The world has changed.

The following is not Ms. Shield's statistic, but some other worker's; she's just summarizing results:

"The Planck results are the most statistically significant evidentiary results for non-baryonic dark matter to-date, constituting a 42σ result for the existence of cold dark matter."

42 sigma is meaningless statistically, and surely is due to the 6-parameter model used for fitting a pretty simple power curve - you can fit almost anything with 6 fudge factors. Anything over 6-8 sigma or thereabouts shouldn't even be mentioned. It's like having a result with 4 significant digits, say 1.000, dividing it by 3, and reporting your answer as .333333...recurring for 42 digits.

As I said, excellent, comprehensive survey, thanks for pointing it out; I'm just addicted to picking nits.
 

1. What is dark matter and why is it important to study?

Dark matter is a form of matter that makes up about 85% of the total matter in the universe. It does not interact with light, making it invisible to telescopes, and its composition is still unknown. Studying dark matter is important because it plays a crucial role in the formation and evolution of galaxies, and understanding it can help us better understand the universe.

2. How do scientists detect dark matter?

Scientists use a variety of methods to detect dark matter, including indirect detection through observations of its effects on visible matter, and direct detection through experiments that look for interactions between dark matter particles and normal matter.

3. What is the latest progress in dark matter detection experiments?

The latest progress in dark matter detection experiments includes the use of more sensitive detectors and new technologies, such as the use of liquid xenon or argon as detection mediums. These experiments have also been able to rule out certain theories and narrow down the possible mass and properties of dark matter.

4. Have we found any evidence of dark matter yet?

While there is strong evidence for the existence of dark matter based on its gravitational effects, there has been no direct detection of dark matter particles yet. Scientists continue to search for evidence through experiments and observations.

5. What are some challenges in detecting dark matter?

One of the main challenges in detecting dark matter is its elusive nature and the fact that it does not interact with light. This makes it difficult to observe and study directly. Additionally, dark matter particles are expected to have very low interaction rates with normal matter, making it challenging to detect them in experiments. Other challenges include background noise and the need for highly sensitive and precise equipment.

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