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Deep Core Proposal
Handle: Document-49410
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Wednesday, April 29, 2009 10:33:19 AM CDT
Thursday, March 18, 2010 04:28:51 PM CDT
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  • With seven of the neighboring conventional IceCube strings they will form the DeepCore detector with a neutrino energy threshold of E? ? 10 GeV, to be compared with 100 GeV for IceCube.
  • The past and future of IceCube string deployments is shown in Table 1.
  • 2 IceCube DeepCore The IceCube DeepCore sub-array will replace the original AMANDA detector and provide the IceCube Neutrino Observatory [2] with sensitivity to neutrinos at energies over an order of magnitude lower than originally envisioned.
  • The higher efficiency for low energy neutrinos in DeepCore translates into an IceCube effective volume for neutrinos from WIMP annihilations which is significantly larger than it would be ...
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Appears In: 05. Other Reference Materials
Preferred Version: Deep Core Proposal