High-energy neutrinos from IceCube

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In summary, this paper reports on a search for high-energy neutrino events at the IceCube detector, which observed 26 additional events beyond what was expected from atmospheric backgrounds. These events have properties consistent with predictions for an extraterrestrial origin, leading to excitement among physicists. Further analysis may provide insight on the theoretical explanation of these results and potential questions that can be answered by IceCube.
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http://arxiv-web3.library.cornell.edu/abs/1311.5238

"Evidence for High-Energy Extraterrestrial Neutrinos at the IceCube Detector"

We report on results of an all-sky search for high-energy neutrino events interacting within the IceCube neutrino detector conducted between May 2010 and May 2012. The search follows up on the previous detection of two PeV neutrino events, with improved sensitivity and extended energy coverage down to approximately 30 TeV. Twenty-six additional events were observed, substantially more than expected from atmospheric backgrounds. Combined, both searches reject a purely atmospheric origin for the twenty-eight events at the 4σ level. These twenty-eight events, which include the highest energy neutrinos ever observed, have flavors, directions, and energies inconsistent with those expected from the atmospheric muon and neutrino backgrounds. These properties are, however, consistent with generic predictions for an additional component of extraterrestrial origin.

Judging from newspaper accounts, a lot of physicists seem very excited by this paper. Can anyone offer any further insight? Are the present results hard to explain theoretically? Are there specific questions that can be answered by IceCube?
 
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There was some discussion earlier in this thread. I will have to look at the present paper to see if there's any evidence for deviation from the expected known-physics background for extraterrestrial neutrinos that was discussed in that thread.
 

Related to High-energy neutrinos from IceCube

1. What is IceCube and how does it detect high-energy neutrinos?

IceCube is a neutrino observatory located at the South Pole. It consists of a cubic kilometer of ice that is instrumented with thousands of optical sensors. When a high-energy neutrino interacts with the ice, it produces a cascade of particles, which emit light that is then detected by the sensors.

2. Why are high-energy neutrinos important to study?

High-energy neutrinos can provide information about the most extreme and energetic processes in the universe, such as black holes and supernovae. They can also help us understand the properties of neutrinos, which are fundamental particles with very little mass.

3. How are high-energy neutrinos detected by IceCube?

IceCube detects high-energy neutrinos through a process called Cherenkov radiation. When a neutrino interacts with the ice, it produces a charged particle that travels faster than the speed of light in the ice, creating a shockwave of light called Cherenkov radiation. This light is then detected by the sensors in IceCube.

4. How do scientists determine the direction and energy of high-energy neutrinos?

By analyzing the pattern and timing of the Cherenkov light detected by IceCube, scientists can determine the direction of the high-energy neutrino. The energy of the neutrino is calculated based on the amount of light produced in the interaction, which is proportional to the energy of the neutrino.

5. What have we learned from the detection of high-energy neutrinos by IceCube?

IceCube has detected a number of high-energy neutrinos, providing valuable insights into the most energetic processes in the universe. It has also confirmed the existence of high-energy astrophysical neutrinos, which was a major breakthrough in the field. Additionally, IceCube has helped us better understand the properties of neutrinos, such as their masses and oscillation behavior.

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