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Observational Evidence for Extra Dimensions from Dark Matter

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Presentation on theme: "Observational Evidence for Extra Dimensions from Dark Matter"— Presentation transcript:

1 Observational Evidence for Extra Dimensions from Dark Matter
Bo Qin National Astronomical Observatories, CAS Bo Qin, Ue-Li Pen & Joseph Silk, PRL, submitted (astro-ph/ )

2 Main results Astronomical observations of systems of dark matter in recent years suggest that dark matter particles may have considerable self-interaction. We find that the properties of this self-interaction are precisely the consequences of a gravity of the r-5 law at r<~1nm, corresponding to a world of 3 large extra dimensions of size R~1nm.

3 String Theory: Extra Dimensions: --- Have never been tested
How to test? ---From gravitational behavior at small distance scales r<R Size of extra dimensions: Planck scale ~10-33 cm Large Extra Dimensions: Arkani-Hamed, Dimopoulos & Dvali (ADD) 1998, Phys. Lett. B Gravity: F ~ r-(2+n) at r<R, R~10(30/n)-17 cm (for n=2, R~1mm) Opens New Window: Experimental test of string theory + Searches for extra dimensions, by precise measurement of gravity at submm scales

4 Gravity has only been accurately measured
at ~1cm and beyond But was extrapolated for 33 orders of magnitude down to ~10-33cm Does Newton’s Inverse Square Law still hold--- 1. At very small distance scales? 2. In very weak regimes? a ~10-8 cm s-2 Modified Newtonian Dynamics (MOND?) Milgrom 1983

5 Experimental tests of Newton’s law at sub-mm scales & Searches for large extra dimensions
e.g.: Long et al., Nature (2003) Hoyle et al., PRL (2001); PRD (2004) Chiaverini et al. PRL (2003) ( & e.g. hep-ph/ for a review ) No deviation from Newtonian has been found from ~1cm down to ~1μm

6 Potential challenge to CDM model
 Collisionless Cold Dark Matter (CCDM) Very successful in explaining the origin and evolution of cosmic structure on large scales, but may have problems on galactic and sub-galactic scales Theory vs. Observation  Conflict (Crisis?) Cuspy core problem of DM \rho ~r^-1 (NFW) ~r^-0.5 (Obs.) Solutions---Modify CCDM Self-Interacting DM (Spergel & Steinhardt, 2000, PRL) Warm Dark Matter (not favored by WMAP, early reionization)

7 xx/mx  810-(25-22) cm2/GeV DM self-interaction cross section:
(Spergel & Steinhardt 2000, PRL) Nature of this self-interaction is unknown: Introduce a new interaction beyond the Standard Model? SIMPs? (Strongly Interacting Massive Particles) Wandelt et al., astro-ph/ Starkman et al., 1990, PRD Qin & Wu, 2001, PRL

8 Further studies of SIDM
In galaxy clusters: ( X-ray / strong lensing / weak lensing )  xx is much smaller In galaxies: still room to argue xx may not be constant, but varies with mass of the system--- more massive systems (clusters) have smaller xx, while less massive systems (like dwarf galaxies) have larger xx

9 xx Maybe velocity dependant
Nature of SIDM xx Maybe velocity dependant Firmani et al. (2000): xx/mx  410-25(100kms/v) cm2/GeV v DM self-interaction m1 Long-range forces? m2

10 Why Extra Dimensions? DM self-interaction  some Variant of Gravity?
If n extra dimensions, gravity would be F~r-(2+n), greatly enhanced at r<R. May naturally provide the DM self-interaction. Advantages: (of attributing DM self-interaction to extra dimensions) 1. Using the existing framework 2. Without introducing any new or fine-tuned interaction 3. Link string scenarios with observable/astronomical phenomena

11 At small scales gravity takes the general form:
where =Rn , from the boundary condition that at r=R, The gravitational scattering cross section (1) And the DM self-interaction cross section from observations: (2)

12 The results  The only solution is n=3 R~1nm mx~3×10-16GeV (axions?)
Combining Eq (1) and (2):  The only solution is n=3 R~1nm mx~3×10-16GeV (axions?) Speculative?


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