PLato said,"Look to the perfection of the heavens for truth," while Aristotle said "look around you at what is, if you would know the truth" To Remember: Eskesthai
Model of the Cryogenic Dark Matter Search which translates actual data into sound and light. We have not yet had a dark matter interaction, but we have lots of particles hitting the detectors and that is what you are watching. A downloadable version is at my webpage http://www.hep.umn.edu/~prisca More info on our experiment can be found at http://cdms.berkeley.edu and http://www.soudan.umn.edu
There is current data that deals with this topic that has been transformed in how we look at this issue. I leave that up to viewers to think about all the other bloggers that have already spoken to this. I wll give one link below for consideration.
So far no WIMP interaction has been observed, so the sensitivity needs to be improved further. This will be achieved by increasing the total detector mass (and with this the probability that a WIMP interacts in the detector) and at the same time reducing the background and improving the discrimination power. This effort started in 2009 under the name SuperCDMS.
The first set of new detectors has been installed in the experimental setup at Soudan and is operating since summer 2009. First tests show that the background levels are in the expected range. Over the course of the next year all CDMS detectors will be replaced by the new larger detectors. The active mass will increase by more than a factor of three to about 15 kg.See:CDMS and SuperCDMS Experiments
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It is known since the 1930's that a significant part of the mass of the universe is invisible. This invisible material has been named Dark Matter. Weakly Interacting Massive Particles (WIMPs) are considered as one of the most convincing explanation for this phenomenon.See:SuperCDMS Queen's Home
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SNOLAB is an underground science laboratory specializing in neutrino and dark matter physics. Situated two km below the surface in the Vale Inco Creighton Mine located near Sudbury Ontario Canada, SNOLAB is an expansion of the existing facilities constructed for the Sudbury Neutrino Observatory (SNO) solar neutrino experiment. SNOLAB follows on the important achievements in neutrino physics achieved by SNO and other underground physics measurements. The primary scientific emphasis at SNOLAB will be on astroparticle physics with the principal topics being: Low Energy Solar Neutrinos; Neutrinoless Double Beta Decay; Cosmic Dark Matter Searches; Supernova Neutrino Searches.
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The Sudbury Neutrino Laboratory, located two kilometres below the surface, is the site of groundbreaking international research.
The 17-metre-wide SNO detector in Vale Inco’s Creighton Mine. Ernest Orlando, Lawrence Berkeley National Laboratory
If dark matter can pull gravitationally, it has mass
So here is an article of 2006 with some interesting information. Now these experimental procedures are always interesting to me because of the type of detectors that were dreamt up in which to measure some aspect of the reality supposed, and realized, by noise in the background.
For scientists to "hear" a dark matter particle, it must hit an atom in one of the crystals at the heart of the CDMS detectors. The crystals are kept cold—close to absolute zero—to reduce atomic movement, keeping the crystals quiet. The detectors "listen" for vibrations inside the crystal, like ears listening for vibrations in the air.
The detectors contain two kinds of crystals, germanium and silicon. A germanium atom is larger than a silicon one: Its nucleus has 73 protons and neutrons compared to silicon's 28. This size difference helps CDMS sort out yet another source of background—neutrons. High-energy cosmic rays and radioactive decays in the matter surrounding the detectors can produce neutrons. Hitting atoms in the crystals, these neutrons cause a "sound" in the detectors similar to the one made by the predicted dark matter particles.See: Listening for whispers of dark matter
Model of the Cryogenic Dark Matter Search which translates actual data into sound and light. We have not yet had a dark matter interaction, but we have lots of particles hitting the detectors and that is what you are watching. A downloadable version is at my webpage http://www.hep.umn.edu/~prisca More info on our experiment can be found at http://cdms.berkeley.edu and http://www.soudan.umn.edu
So lets mover forward here to Dec 10, while waiting to hear on Dec 17 for more news.
The CDMS collaboration has completed the analysis of the final CDMS-II runs, which more than doubled the total data from all previous runs combined. The collaboration is working hard to complete the first scientific publication about these new results and plans to submit the manuscript to arXiv.org before the two primary CDMS talks scheduled for Thursday, Dec. 17, at Fermilab and at SLAC. See:The search for dark matter:has CDMS found something?
