Lecture 2 - E. Wilson 16 Oct 2014 –- Slide 1 Lecture 2 - Overview of Accelerators II ACCELERATOR PHYSICS MT 2014 E. J. N. Wilson
Lecture 2 - E. Wilson 16 Oct 2014 –- Slide 2 Summary Lecture 1 - Overview of Accelerators I The history of accelerators Need for Accelerators The race to high energies Cockcroft and Walton - Electrostatic Van der Graaf Linear accelerator Wideroe’s Linac Fermilab linac (400MeV) Inside the Fermilab linac The Stanford Linear Accelerator The International Linear Collider (ILC) Cyclotrons –an inspired discovery Magnetic Rigidity Vertical Focusing Discovery of the Synchrotron Components of a synchrotron Phase stability Cosmotron Weak focusing in a synchrotron
Lecture 2 - E. Wilson 16 Oct 2014 –- Slide 3 Lecture 2 – Overview II - Contents The “n-value” Weak focusing in a synchrotron Cosmotron people Strong focussing CERN at BNL CERN 25 GeV PS CERNS RINGS SPS Center of mass v. Fixed target AdA - The first collider e-plus-minus ISR AND PS Luminosity SPS Physics of the electron v. protons LEP Inside LEP The Tevatron at FNAL The Large Hadron Collider (LHC) Superconducting magnets
Lecture 2 - E. Wilson 16 Oct 2014 –- Slide 4 Weak focusing in a synchrotron Vertical focussing comes from the curvature of the field lines when the field falls off with radius ( positive n-value) Horizontal focussing from the curvature of the path The negative field gradient defocuses horizontally and must not be so strong as to cancel the path curvature effect The Cosmotron magnet
Lecture 2 - E. Wilson 16 Oct 2014 –- Slide 5 As the C magnet saturates the n value – which is the rate of droop – increases The “n-value”
Lecture 2 - E. Wilson 16 Oct 2014 –- Slide 6 Cosmotron people FOURGUYS.pct E.Courant -Lattice DesignerStan Livingston - Boss Snyder -theorist Christofilos - inventor
Lecture 2 - E. Wilson 16 Oct 2014 –- Slide 7 Strong focussing
Lecture 2 - E. Wilson 16 Oct 2014 –- Slide 8 CERN at BNL Odd Dahl, Frank Goward, and Rolf Widerö (right hand trio) Fig.3(CERNVISITORS).pct
Lecture 2 - E. Wilson 16 Oct 2014 –- Slide 9 CERN 25 GeV PS
Lecture 2 - E. Wilson 16 Oct 2014 –- Slide 10 CERNS RINGS
Lecture 2 - E. Wilson 16 Oct 2014 –- Slide 11 SPS
Lecture 2 - E. Wilson 16 Oct 2014 –- Slide 12 Center of mass v. Fixed target
Lecture 2 - E. Wilson 16 Oct 2014 –- Slide 13 AdA - The first collider e-plus-minus
Lecture 2 - E. Wilson 16 Oct 2014 –- Slide 14 ISR AND PS ISR+PS.pct
Lecture 2 - E. Wilson 16 Oct 2014 –- Slide 15 Imagine a blue particle colliding with a beam of cross section area - A Probability of collision is For N particles in both beams Suppose they meet f times per second at the revolution frequency Event rate Luminosity LUMINOSITY Make small Make big
Lecture 2 - E. Wilson 16 Oct 2014 –- Slide 16 SPS
Lecture 2 - E. Wilson 16 Oct 2014 –- Slide 17 Physics of the electron v. protons When we collide Protons we collide complex assemblies of three quarks Only two quarks interact Their available energy is on average only 10% of the total centre of mass energy We do not know which quarks they are Hence in some ways 100 GeV LEP is as good as 1000 GeV TEVATRON HENCE THE RETURN TO LEP AFTER SPS AND THEN LHC AFTER LEP
Lecture 2 - E. Wilson 16 Oct 2014 –- Slide 18 LEP LEP(small).pct
Lecture 2 - E. Wilson 16 Oct 2014 –- Slide 19 Inside LEP
Lecture 2 - E. Wilson 16 Oct 2014 –- Slide 20 Superconducting magnets
Lecture 2 - E. Wilson 16 Oct 2014 –- Slide 21 Fermilab’s superconducting Tevatron can just be seen below the red and blue room temperature magnets of the 400 GeV main ring. The Tevatron at FNAL
Lecture 2 - E. Wilson 16 Oct 2014 –- Slide 22 The Large Hadron Collider (LHC)
Lecture 2 - E. Wilson 16 Oct 2014 –- Slide CERN Control Centre – LHC Startup
Lecture 2 - E. Wilson 16 Oct 2014 –- Slide 24 Lecture 2 – Overview II - Contents The “n-value” Weak focusing in a synchrotronCosmotron people Strong focussing CERN at BNL CERN 25 GeV PS CERNS RINGS SPS Center of mass v. Fixed target AdA - The first collider e-plus-minus ISR AND PS Luminosity SPS Physics of the electron v. protons LEP Inside LEP The Tevatron at FNAL The Large Hadron Collider (LHC) Superconducting magnets