1 / 17

Interactions of muons with atoms & nuclei

Interactions of muons with atoms & nuclei. BNL Muon Storage Ring. Introduction of muons m + , m - (Leptons, electro-weak interactions)  a major component of natural radioactive background produced by “cosmic rays” in upper atmosphere.

yazid
Download Presentation

Interactions of muons with atoms & nuclei

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. Interactions of muons with atoms & nuclei Weak Beta/Muon Interactions BNL Muon Storage Ring

  2. Introduction of muons m+, m- (Leptons, electro-weak interactions) a major component of natural radioactive background produced by “cosmic rays” in upper atmosphere. Application: Demonstration of relativistic time dilatation; Nuclear structure,…., radiography (?). Energy loss by Coulomb interactions with matter. (biomed/radio-imaging application). Kinematics of muon decay. Nuclear capture of negative muons. The ANSEL cosmic muon experiment, counters & electronics. Today’s Agenda Weak Beta/Muon Interactions

  3. Muons from Cosmic Ray Showers Muons produced in energetic p-induced reactions.Cosmic ray shower in the upper atmosphere generated by primary protons from solar system (Sun etc.) Weak Beta/Muon Interactions Muon momentum spectrum at sea level. Solid line: parameterization of high momentum spectrum. 30% m-, 70% m+

  4. Direct measurement of the muon lifetime. Images from the 1962 documentary “Time Dilation”. Measure survival of energetic muons, compare to stopped muon decay. Stopper Decay products. Weak Beta/Muon Interactions Decay Product Muon Stop Frisch and Smith, AJP 31, 342 (1963).

  5. Demonstration of Time Dilatation Weak Beta/Muon Interactions Frisch & Smith, AJP 31, 342 (1963) t = (2.2 ± 0.2) µs.

  6. Properties of Electrons and Muons Weak Beta/Muon Interactions Electromagnetic interactions via charge and magnetic moment. Weak muonic interactions: m± decay and m- capture (EC)

  7. Electronic Interactions of Muons with Matter Stronger electric + weaker magnetic interactions of muon Bethe-Bloch Formula Energetic muons are minimum ionizing particles (“mips”). Lose most of their energy near the end of trajectory. mips Weak Beta/Muon Interactions

  8. Electronic Interactions of Muons with Matter Plastic Target: Monitored in experiment Expect a line E/DE spectrum for traversing muons. Stop, Decay following Transmitted Plexiglas Plastic: CnHmpolymer ([H]/[C]≈1.11), rT=1.03 g/cm3IE=64.7 eV. Cosmic ray muons = mostly minimum ionizing particles (mips) For plastic: DE=2MeV/cm Weak Beta/Muon Interactions

  9. Weak Interactions: Muon Decay Configuration of maximum pe Rest mass Maximum

  10. Muon Decay: Electron Energy Spectrum Less than maximum momentum transfer to electron Electron Momentum x

  11. Cosmic-Muon Disappearance Rates Partial muon life times and disappearance rates (branching decay) m+ , m- decay m-Capture Light nuclei (Li, Be, …C, O,..): long partial capture muon life times (tc~ 100 ms » td) Random Background Heavy nuclei (Cu,..W,..Pb,..): short partial capture muon life times (tc ~ 50 ns « td)

  12. Exotic (Muonic) m- Atoms Negative muonm- captured by (electronic) atom, ejects 1 e-, cascades down to 1sm Muonic X rays  muonic atom formed with m- in 1s 1sm (Z, N) decay capture Heavy m atom: Muon mostly inside nucleus shielding of Z  effective Zeff < Z Isomeric shift, magnetic HF splitting nuclear levels

  13. Negative Muon K-Capture Negative muonm- in K shell (1sm) is captured by proton (analog to EC process) 1sm (Z, N) Isotopic effect in capture rates due to differences in n, n phase space n Strength factor K=272 s-1 (A-1,Z-1)+n p n

  14. Neutrino momentum transfer depends on Nucleonic momentum distribution influencedby correlations (m*)  Spectrum I(E*) of Nuclear excitations can be broad, emission of neutrons, charged particles, g-rays m-Capture Nuclear Excitation Function Q = excitation energy E* Theoretical n Multiplicity Distribution (Singer Model) Evaporation Non-Equilibrium Curves to guide the eye and to illustrate evaporative and pre-equilibrium n components

  15. The ANSEL Cosmic Muon Telescope ExtendedActual version Weak Beta/Muon Interactions

  16. Electronics for ANSEL Muon Experiment Active target AT= plastic scintillator Placed between telescope counters #3 and #4 Muon transmission Muon stop in AT Measure energy deposit in both modes Active target AT= plastic scintillator between #3 and #4 stops muon  decay Measure decay lifetime in plastic AT (negligible capture) Weak Beta/Muon Interactions

  17. The END (For Now) Weak Beta/Muon Interactions

More Related