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Frank Linde, Philips meets particle physics , 31 January 2012

Frank Linde, Philips meets particle physics , 31 January 2012. 1946. 1965. first silicon strip detector Philips & IKO. 1954. What is the Universe made of? We barely know 4%!. Where is all the antimatter? Universe ought to be symmetric!.

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Frank Linde, Philips meets particle physics , 31 January 2012

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  1. Frank Linde, Philips meets particle physics, 31 January 2012

  2. 1946 1965 first silicon strip detector Philips & IKO 1954

  3. What is the Universe made of? We barely know 4%! Where is all the antimatter? Universe ought to be symmetric! How did the Universe lookdirectly after the Big Bang? Observe it! Origin of particle masses? Newton didn’t know – neither do we …

  4. natural source: cosmic rays, •••

  5. natural source: cosmic rays, •••

  6. PS ISR SPS SppS LEP LHC CLIC 1959 1971 1976 1981 1989 2025? 2009 500 fellows & associates 2500 staff 6500 users 1 G€/year CERN

  7. man-made source: accelerator

  8. man-made source: accelerator

  9. tracking detector: silicon pixels

  10. tracking detector: silicon pixels

  11. particle hunting: Higgs

  12. particle hunting: Higgs

  13. HiggsZZ?     no simulation i.e. real!

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