Colloquium by Jonathan Feng - Fermilab Center for Particle ...

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STRONGLY-INTERACTING MASSIVE PARTICLES • The big picture 23 Mar 11 Mack, Beacom, Bertone (2007) • SIMP window is now essentially closed Albuquerque, de los Heros (2010) Feng 18
LOWER LIMIT ON DIRECT DETECTION • Solar, atmospheric, and diffuse supernova background neutrinos provide an “irreducible background” • The limits of background-free, non-directional direct detection searches (and also the metric prefix system!) will be reached by ~10 ton experiments probing σ ~ 1 yb (10 -12 pb,10 -48 cm 2 ) Strigari (2009); Gutlein et al. (2010) 23 Mar 11 Feng 19
Page 1 and 2: WIMP PARADIGM: CURRENT STATUS FNAL
Page 3 and 4: THE COSMIC CONNECTION, c. 1977 “O
Page 5 and 6: DARK MATTER Known DM properties •
Page 7 and 8: 23 Mar 11 THE WEAK MASS SCALE • F
Page 9 and 10: 23 Mar 11 THE WIMP MIRACLE 10-3 σ0
Page 11 and 12: LEP’S COSMOLOGICAL LEGACY Gauge H
Page 13 and 14: INDIRECT DETECTION Dark Matter anni
Page 15 and 16: ARE THESE DARK MATTER? • Energy s
Page 17: DIRECT DETECTION • Can look for n
Page 21 and 22: LOW MASS FRONTIER Collision rate sh
Page 23 and 24: SPIN-DEPENDENT SCATTERING 23 Mar 11
Page 25 and 26: CURRENT BOUNDS FOR SUSY Yellow: pre
Page 27 and 28: 23 Mar 11 THE SIGNIFICANCE OF 10 -4
Page 29 and 30: BEYOND WIMPS • Does the WIMP para
Page 31 and 32: FREEZE OUT WITH SUPERWIMPS WIMPs fr
Page 33 and 34: WARM SUPERWIMPS • SuperWIMPs are
Page 35 and 36: • In SUSY, however, there may be
Page 37: CONCLUSIONS • Particle Dark Matte

Colloquium by Jonathan Feng - Fermilab Center for Particle ...

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