1 / 11

Introduction to particle physics Part V

Physics 129, Fall 2010; Prof. D. Budker . Introduction to particle physics Part V. The Weak Interactions. Responsible for -decay Mediated by heavy ( 80-90 GeV /c 2 ) bosons Discovered in 1983 at CERN ( UA1 ) 1984 Nobel Prize to . Stochastic cooling.

teenie
Download Presentation

Introduction to particle physics Part V

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. Physics 129, Fall 2010; Prof. D. Budker Introduction to particle physicsPart V

  2. The Weak Interactions • Responsible for -decay • Mediated by heavy (80-90 GeV/c2) bosons • Discovered in 1983 at CERN (UA1) • 1984 Nobel Prize to Stochastic cooling Simon van der Meer Carlo Rubia Accelerator Detector Physics 129, Fall 2010, Prof. D. Budker; http://budker.berkeley.edu/Physics129_2010/Phys129.html

  3. The Wand Z propagators • Does not reduce to photon case for M0 • Polarization vector has threeindep. comp. The metric Physics 129, Fall 2010, Prof. D. Budker; http://budker.berkeley.edu/Physics129_2010/Phys129.html

  4. The W vertex • Weak Coupling Constant: • Numerical factors are conventional •  --- vector coupling (as in QED) •  5 --- axial-vector coupling • “V-A” interaction Physics 129, Fall 2010, Prof. D. Budker; http://budker.berkeley.edu/Physics129_2010/Phys129.html

  5. p2 p4 p3 p1 • Amplitude according to the rules: • What are the units here? • Remember normalization: • Proper averaging over polarizations gives (neglecting lepton masses): Physics 129, Fall 2010, Prof. D. Budker; http://budker.berkeley.edu/Physics129_2010/Phys129.html

  6. Cross-section • The cross-section formula reads: • No dependence on angles! •  Isotropic cross-section! • Cross-section goes E2 (typical for weak processes) Physics 129, Fall 2010, Prof. D. Budker; http://budker.berkeley.edu/Physics129_2010/Phys129.html

  7. Muon Decay p1 p3 p2 • Amplitude according to the Rules: • Calculation of the muon lifetime (see Griffiths) yields: • Note scaling with muon mass: = -1 (m)5 Not quite how Griffiths would draw this p4 Physics 129, Fall 2010, Prof. D. Budker; http://budker.berkeley.edu/Physics129_2010/Phys129.html

  8. Muon Decay andFermi Theoryof weak interactions • Note that coupling comes together with W mass • Historically, the Fermi coupling constant was used: • The largest coefficient “of order unity” • With =c=1, F Physics 129, Fall 2010, Prof. D. Budker; http://budker.berkeley.edu/Physics129_2010/Phys129.html

  9. The week coupling is LARGE • Weak interactions are weak because gauge bosons are heavy Physics 129, Fall 2010, Prof. D. Budker; http://budker.berkeley.edu/Physics129_2010/Phys129.html

  10. Island Physics… • Why are numerical coefficients (usually) ~1? • (The 1923 exception “proves” the rule…) • The answer is unexpected: this is due to… • 3 dimensions of space • Unit sphere (R=1) in N dimensions: Physics 129, Fall 2010, Prof. D. Budker; http://budker.berkeley.edu/Physics129_2010/Phys129.html

  11. Island Physics… • How to calculate muon lifetime… • with no Griffiths and no internet • Remember that this is an allowed weak decay • Rate goes as |M|2 (GF)2 • What else can enter ?  m • That’s it! (Neglecting light-lepton masses) • With =c=1, []=Energy=Mass Physics 129, Fall 2010, Prof. D. Budker; http://budker.berkeley.edu/Physics129_2010/Phys129.html

More Related