1. Particle Physics at the Energy Frontier Tevatron → LHC & The Very Early Universe Tony LissAir Force Institute of TechnologyApril 10, 2008

2. Two Views of the Universe High energy physicists study the smallest, most fundamental objects and the forces between them. Cosmologists study what there is on the largest possible scales and try to understand how it got that way. But these two very different approaches address many of the same questions: What is the Universe made of & how does it behave?

3. ???? The High-Energy View The matter around us is made up of “quarks” and “leptons” And held together by four forces, each with a force carrier: A proton is made of U U D Add an electron to make a hydrogen atom Electromagnetic Strong Weak Gravity

4. Unification of the Forces Electric Magnetic Weak Strong Electromagnetic Electroweak “Low Energy” “High Energy” “Very (very)High Energy” Theory (“Standard Model”) works up to ~here … And you may notice that gravity isn’t in this picture… STRING THEORY ??? Part way to Einstein’s dream! Higgs Bosons born here

5. Cosmology, Particle Physics, the Universe and All That

7. Successes of Particle Physics + Big Bang Light elements (H to Li) were made in the early universe –And we can calculate how much! astron.berkeley.edu/~mwhite/darkmatter/bbn.html Predicted abundance depends on density of “baryons” – particles made of 3 quarks (like a proton or a neutron) About 1 He nucleus for every 10 protons (25% by mass) The grey band is where the measured & calculated abundances are.

8. But Wait! Most of the universe is not normal (“baryonic”) matter! Recent cosmological measurements put the density of the universe here.

9. Dark Matter (Not a New Idea) Speed of stuff out here Doesn’t match luminous matter in here! There’s DARK MATTER in Galaxies!!

10. Dark Matter In Between Galaxies Too! Motion of a galaxy out here Doesn’t agree with luminous matter in here The “Hydra” Galactic Cluster  matter ~ 0.3 from galactic clusters

11. Studying the Universe at Accelerators Accelerate particles to very high energies and smack them together. E=Mc 2 : Make new stuff and study how it behaves. This picture shows a proton and antiproton colliding to make a pair of top quarks. Top quarks were discovered 14 years ago at Fermilab Michael Goodman Fermi National Accelerator Laboratory

12. Hadron-Hadron Collisions Proton-antiproton (Tevatron) or proton-proton (LHC) collisions: Each collision (“event”) is between the hadron constituents. What can happen is…EVERYTHING

13. Cross Sections The total pp cross section is here at ~10 11 !

14. This happens only once in ~10 10 collisions

15. Data Taking (TeVatron) Protons & antiprotons collide at ~2.5 MHz 0.25Hz of W/Z production ~100 Hz of high E T jets ~100 Hz of b-quark production.0002 Hz of top quark production ?? Hz of new physics 1% “Acceptance” ~1% Analysis Mode ~10 -2 Hz for analysis 10% “Acceptance” ~40% Analysis Mode ~10 -5 Hz for analysis ?? “Acceptance” ?? Analysis Mode 20% “Acceptance” ~20% Analysis Mode ~10 -2 Hz for analysis Prescale/20 10% “Acceptance” 85% to analysis ~0.4 Hz for analysis

16. The CDF Detector at FNAL

17.  The Mass of the Top Quark  The Mass of the W Boson

18. Measuring the Top Mass There are many subtleties to improve S/B and resolution, but basically… Measure for each of the decay objects

20. Measuring the Top Mass

21. Measuring the W Boson Mass

22. A Window on the Higgs! Experimental bound (LEP) WW W H WW t b The result is marginally inconsistent with the SM… SUSY????

23. Making Higgs Bosons

24. Finding The Higgs The Higgs “couples to mass”, so it’s preferred decay channel depends on its (unknown) mass. As if life were not difficult enough…

25. Looking for Higgs (is hard)

26. No Higgs…yet

27. SUSY Every quark, lepton and force carrier has a SUSY partner (sparticles). –Sparticles would be made copiously in the early (HOT) universe. –They all decay away quickly, except for the lightest one (neutralino), which can’t. –The dark matter might be made up of neutralinos!! www.science.doe.gov/hep/EME2004/03-what-is.html Make SUSY particles at an accelerator: E=Mc 2 happening here!

28. Another Reason to Believe in SUSY? Einstein’s dream of a “Unified Field Theory”, now needs SUSY: Energy Strength of force No SUSY Energy Strength of force SUSY EM weak strong

29. Searching for SUSY – an example SUSY models come in many different flavors, but one characteristic of many of them is signatures with large “Missing E T ” – Undetectable particles whose momentum is unmeasured. In these diagrams “charginos” and “neutralinos” are produced. In their subsequent decay, the lightest “neutralino” is produced but remains undetected.

30. Searching for Charginos & Neutralinos What the signal would look like (if it were there) The data Backgrounds

31. No SUSY So Far Many searches, no sightings… The hunt continues… At LHC there is 7x more “reach” (E=Mc 2 ) for making SUSY particles. But maybe SUSY isn’t the right model… We can find it anyway if M<E/c 2 !

32. On to the LHC!

33. ATLAS Detector at CERN

34. ATLAS is VERY BIG

35. ATLAS

36. A (simulated) Higgs event in ATLAS

37. A Black Hole in ATLAS

38. The Universe as We Know It Dark Matter Dark Energy This is NOT what we thought as recently as 10 years ago!! Our fabulously successful “Standard Model of particle physics” explains only 4% of the universe… So far… Atoms 73% 4% 23%

39. Perspective Our theories of cosmology and particle physics are extremely successful, but leave significant open questions. As new phenomena are discovered, we adapt the theories and test them with experiments & observations. The next ten years of accelerator experiments and cosmological measurements are guaranteed to bring new insights and new surprises!