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Published byMaría Isabel Benítez Gómez Modified over 6 years ago
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Search for Dark Matter physics 805 fall 2008
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WIMP search strategies
Direct detection Indirect detection: – neutrinos from the Earth/Sun – antiprotons from the galactic halo – positrons from the galactic halo – gamma rays from the galactic halo – gamma rays from external galaxies/halos – synchrotron radiation from the galactic center / galaxy clusters – ...
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direct detection - general principles
WIMP + nucleus WIMP + nucleus Measure the nuclear recoil energy Suppress backgrounds c c c Search for an annual modulation due to the Earth’s motion around the Sun December June
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present limits
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DAMA result (> 8 sigma)
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WIMP Capture and Annihilation
nm DETECTOR c + c W + W n + n
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7 IceCube + 18 AMANDA strings
Inner Core Detector Inner Core (same region as AMANDA) 7 IceCube + 18 AMANDA strings 225 DOMs OMs
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neutralino capture and annihilation
rc velocity distribution sscatt Gcapture Gannihilation n interactions n int. m int. c sun nm m Freese, ’86; Krauss, Srednicki & Wilczek, ’86 Gaisser, Steigman & Tilav, ’86 Silk, Olive and Srednicki, ’85 Gaisser, Steigman & Tilav, ’86
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indirect detection for cyclists
e.g. 104 m2 n-telescope searches for 500 GeV WIMP 300 km/s > LHC limit 1. - flux 2. solar cross section
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Nsun = capture rate = annihilation rate
_ c c WW 250 GeV 500 GeV mnm 3. Capture rate by the sun 4. Number of muon-neutrinos 0.1 is the leptonic branching ratio
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5.5 x 1023 cm-3 104 m2 _ ~ # events = 10 per year
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WIMP search Limits on muon flux from Earth
PRELIMINARY Limits on muon flux from Earth Limits on muon flux from Sun AMANDA 180d Antares 3 years 1km3 (IceCube) SK New solar system WIMP diffusion model -> more realistic neutralino velocity distribution (Lundberg&Edsjoe) Detection threshold (mu): ~50GeV (extrapolate to get limits for E>1 GeV) Cuts optimized for each mass independently Disfavored by direct search (CDMS II)
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IceCube 22 strings
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Status indirect search
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IceCube Direct Detection vs Black: out Green: yes Blue: no
(Zeppelin4/Genius) Black: out Green: yes Blue: no
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