The CP-violating inert-doublet model - Scalars 2011

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Scales Gravity explored down to here Unknown Other interactions explored down to here Planck scale Particle physics Atomic physics You are here Solar system Galaxies Clusters of galaxies light year 10 -36 m 10 -24 m 10 -12 m 1 m 10 12 m 10 24 m
Ambition: •Problem at scales of 10 20 m •Solution: new physics at scales below 10 -18 m !!!
Page 1 and 2: Scalar dark matter work with Bohdan
Page 3 and 4: Dark Matter Astrophysical evidence:
Page 5: footnote: scales 1 light year ≈ (
Page 9 and 10: The Big Picture 10 -40 cm 2 mass cr
Page 11 and 12: Simple estimate MPl Density of dark
Page 13 and 14: Scalar DM • “Inert (Scalar) Dou
Page 15 and 16: Motivation (Barbieri et al) May all
Page 18 and 19: Allowed regions LEP (PDG) LEP, Lund
Page 20 and 21: (standard) Coupling: (most general)
Page 22 and 23: “Dark democracy”
Page 24 and 25: Positivity Define: Plus additional
Page 26 and 27: Annihilation in the Early Universe
Page 28 and 29: Allowed regions in MS IDM LOW MEDIU
Page 30 and 31: Light DM: coupling to Higgs, can no
Page 32 and 33: forbidden, coannihilation too fast
Page 34 and 35: Allowed regions in MS, M1 3 10 Allo
Page 36 and 37: Allowed regions High region: Allowe
Page 38 and 39: CP violation Measured in terms of i
Page 40 and 41: CP violation: electron edm Unit: (~
Page 42 and 43: Direct detection S nucleus ionizes
Page 44 and 45: Compare CDMS-II and XENON100 ] 2 [
Page 46 and 47: Md charged abundance scalars in tha
Page 48 and 49: Cross sections pp +, -, j M s=75 [

The CP-violating inert-doublet model - Scalars 2011

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