1. DARK MATTER Jonathan Feng University of California, Irvine University of Colorado, Boulder 21 June 2011 Credit: John Kormendy

2. 21 June 11Feng 2 PHYSICS: TRADITIONAL VIEW smalllarge Particle Physics Nuclear Physics Atomic Physics Condensed Matter Physics Biophysics Astrophysics Cosmology

3. 21 June 11Feng 3 Particle Physics Condensed Matter Physics Biophysics Astrophysics Cosmology Nuclear Physics Atomic Physics PHYSICS: UPDATED VIEW

4. 21 June 11Feng 4

5. 21 June 11Feng 5 THE LARGE FRONTIER clusters of galaxies 10 12 meters solar systemgalaxy 10 17 meters 10 23 meters > 10 26 meters universe

6. 21 June 11Feng 6 EVIDENCE FOR DARK MATTER: CLUSTERS OF GALAXIES In the 1930’s Fritz Zwicky observed the Coma cluster and found that the galaxies were moving too fast to be contained by the visible matter

7. 21 June 11Feng 7 EVIDENCE FOR DARK MATTER: INDIVIDUAL GALAXIES In the 1970’s Vera Rubin and collaborators and Albert Bosma found that stars in galaxies were rotating too fast to be contained by the visible matter

8. THE STANDARD MODEL OF COSMOLOGY Atoms make up only 4% of the Universe The rest of the matter is dark matter, which does not shine or reflect light –Not atoms –Cold –Stable Also, 73% of the Universe isn’t even matter 21 June 11Feng 8

9. 21 June 11Feng 9 THE SMALL FRONTIER electron 10  10 meters (thickness of human hair ~ 10 -5 m) up quark down quark atom nucleus proton neutron 10  14 meters 10  15 meters < 10  8 meters

10. Strong Weak 4 FORCES OF NATURE Gravity Electromagnetism 21 June 11Feng 10

11. 21 June 11Feng 11 STANDARD MODEL OF PARTICLE PHYSICS Atoms

12. 21 June 11Feng 12 Known DM properties WHICH PARTICLE IS DARK MATTER? Not atoms The extraordinarily successful standard models of cosmology and particle physics are inconsistent Cold Stable

13. In 1821 Alexis Bouvard found anomalies in the path of Uranus and suggested they could be caused by unseen matter In 1845-46 Urbain Le Verrier determined where this matter should be. With this guidance, Johann Galle discovered the unseen matter at the Berlin Observatory in 1846 21 June 11Feng 13 Le Verrier wanted to call it Le Verrier, but this matter is now known as Neptune, the farthest known planet (1846-1930, 1979- 1999, 2006-present) WHAT SHOULD WE DO?

14. Strong Weak WHICH FORCES DOES DARK MATTER FEEL? Gravity Electromagnetism 21 June 11Feng 14 ?

15. OPTION 1: WIMPS Dark matter feels the weak force DM = WIMPs: weakly-interacting massive particles Why WIMPs? Looking under the lamp post 21 June 11Feng 15

16. THE WIMP MIRACLE But there’s more to it than that Many theories predict WIMPs that are around 100 times heavier than the proton Feng 16 DM q q time Such particles are present just after the Big Bang, but then annihilate in pairs. Assuming they annihilate through the weak force, calculations show that they should be ~ 10% of the Universe now. This is what is required to be dark matter! 21 June 11

17. WIMP DETECTION If WIMPs annihilated in the early Universe, they should also be doing that now We can look for rare forms of matter and anti-matter created in these collisions Feng 17 DM q q time 21 June 11

18. ICECUBE IN ANTARCTICA Looking for neutrinos produced by WIMP annihilation in the Sun Feng 18 21 June 11

19. ALPHA MAGNETIC SPECTROMETER Carried by Space Shuttle to the International Space Station Feng 19 21 June 11

20. Feng 20 WIMP PRODUCTION If WIMPs annihilated in the early Universe, we should also be able to run time backwards We can collide two normal particles at high velocities to create dark matter, which we detect as missing energy Feng 20 DM q q time 21 June 11

21. Feng 21 LARGE HADRON COLLIDER Colliding protons at 99.999999% the speed of light Feng 2121 June 11

22. Feng 22 Billion collisions per second; dark matter is a needle in the haystack 21 June 11 CMS

23. WIMP RECOILS If WIMPs annihilated in the early Universe, we should also be able to run time sideways We can watch for normal matter recoiling from a WIMP collision. At any given time, there is roughly 1 WIMP per coffee cup, but their interactions are weak and recoils are rare Feng 23 DM q q time 21 June 11

24. CRYOGENIC DARK MATTER SEARCH Colliding protons at 99.999999% the speed of light Operating at milli-Kelvin temperatures in a mine in Minnesota Feng 2421 June 11

25. Collision rate should change as the Earth goes around the Sun: annual modulation (1986) 21 June 11Feng 25 DAMA/LIBRA signal with period ≈ 1 year, maximum ≈ June 2 DAMA/LIBRA IN ITALY DAMA/LIBRA (2010)

26. OPTION 2: SUPERWIMPS Dark matter does not feel the weak force DM = SuperWIMPs: superweakly- interacting massive particles Seemingly a lost cause Feng 2621 June 11

27. GRAVITINOS Feng 27 An example: gravitinos proposed by Pagels and Primack in 1982 Gravitinos feel only gravity But they may be created by decaying particles that have dramatic implications for the LHC Long-lived progenitor (charge and mass) q (charge) SuperWIMP (mass) 21 June 11

28. GRAVITINOS AT THE LHC D. Akerib Feng 2821 June 11

29. SUMMARY We now have two extraordinarily successful theories of the large and small, but they don’t match A quarter of the Universe is dark matter, but we don’t know what it is We have some ideas, though, and many interesting search experiments underway Feng 2921 June 11