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Hierarchy in the phase space and dark matter detection

Hierarchy in the phase space and dark matter detection. Niayesh Afshordi. Collaborators. Roya Mohayaee (IAP, Paris) Ed Bertschinger (MIT) Hierarchical Phase Space Structure of Dark Matter Haloes: Tidal debris, Caustics, and Dark Matter annihilation: arXiv:0812.2244

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Hierarchy in the phase space and dark matter detection

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  1. Hierarchy in the phase space and dark matter detection Niayesh Afshordi

  2. Collaborators • Roya Mohayaee (IAP, Paris) Ed Bertschinger (MIT) • Hierarchical Phase Space Structure of Dark Matter Haloes: Tidal debris, Caustics, and Dark Matter annihilation: arXiv:0812.2244 • Hierarchy in the Phase Space and Dark Matter Detection: in preparation

  3. Dark Matter detection • 22% of density of Universe consist of DM • No clear non-gravitational detection • Tentative anomalies may come from WIMP’s: • PAMELA, positron excess • ATIC e+-e-excess • WMAP haze at Galactic center • INTEGRAL 511 keV excess • DAMA/LIBRA direct detection signal • ?????

  4. WIMPs: from gravity to detection • Gravitational evidence for DM comes from potential: sd3x½(x)/|x-x’| • Direct detection: ½(x) at solar system • Indirect detection (annihilation): sd3x½(x)2 WIMP detection is much more sensitive to DM sub-structure: Boost ´h½2i/h½i2-1

  5. Hierarchy in the Phase space • CDM is really cold • vCDM» 10-11c • Phase space density remains constant in lieu of collisions (Liouville Theorem): • At CDM freeze out: • Within our Galaxy:  Most of the phase space is empty!

  6. Conclusions • Phase space of CDM haloes is mostly empty, and has a rich structure: • Hierarchy of tidal debris and subn-haloes • Fundamental discreteness • Boost in DM annihilations • DM direct detection can show signs of sub-structure

  7. Three types of phase structures • Bound sub-haloes (cluster in real/phase space) • Tidal debris (cluster in initial conditions) • Fundamental discreteness  analogous to galaxy shot noise Kuhlen, Diemand, et al. NGC 3923

  8. Hierarchical Micro-Structure of the Phase Space

  9. Phase mixing in action-angle space • Evolution of tidal debris is simple in action-angle space

  10. Lattices in action space • Distribution in action space is a lattice which becomes finer in time Afshordi et al. 08 McMilllan & Binney 08

  11. Catastrophes in the CDM Structure • Discrete/cold structures in action space project into catastrophes into real space Catastrophes of light ray distribution cusp fold Catastrophes in stellar distribution NGC 3923

  12. Annihilation Boost in DM haloes • Tidal debris: hf(J1)f(J2)i/|J1-J2|-1.6 • Fundamental discreteness: hf(J1)f(J2)i/±3(J1-J2) • Boost = h½2i/h½i2-1 » O(1) + 3x105 (½/½crit)-3/2 tidal debris discreteness

  13. Local vs. Total Boost in NFW haloes Total boost Local Boost

  14. sub-haloes and stable clustering • Stable clustering in phase space can be used to describe bound subn-halo hierarchy within virial radius Boost »106 (½crit,0/½) at solar system Kuhlen, Diemand, et al. Afshordi et al. in prep.

  15. sub-haloes in Direct Detection! • Temporal auto-correlation of DM detection in several years… Afshordi et al. in prep.

  16. Conclusions • Phase space of CDM haloes is mostly empty, and has a rich structure: • Hierarchy of tidal debris and subn-haloes • Fundamental discreteness • Boost in DM annihilations • DM direct detection can show signs of sub-structure

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