1 / 22

OMC rates in Sm and Kr for 2 b -decay

OMC rates in Sm and Kr for 2 b -decay. V.G. Egorov , A.V. Klinskih, R.V. Vasiliev , M.V.Shirchenko , D.R. Zinatulina 13 .0 6.200 7 MEDEX’07. OMC!. (n,p)-like charge- -exchange reactions. ?. . PSI 2006 :. 150 Sm 2 O 3 (solid target) nat Sm 2 O 3 (solid target)

aulii
Download Presentation

OMC rates in Sm and Kr for 2 b -decay

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. OMC rates in Sm and Kr for 2b-decay V.G. Egorov, A.V. Klinskih, R.V. Vasiliev, M.V.Shirchenko, D.R. Zinatulina 13.06.2007 MEDEX’07

  2. OMC! (n,p)-like charge- -exchange reactions ? 

  3. PSI 2006: • 150Sm2O3(solid target) • natSm2O3(solid target) • natKr (gas target) • 82Kr (gas target) • 12C4H10(gas target) • 232Th (calibration purpose) • 197Au (calibration purpose)

  4. Setup (solid target)

  5. Try to find a physicist! PSI,2006 An answer

  6. To deal with enriched 82Kr: • Keep noble gas (expensive! penetrating!) without loosing • Ensure μ-stops in gas (⇒ thickness of the entrance window be comparable with the “thickness” of gas) • Ensure detection of low-energy γ-rays without absorption in the target walls • ⇒Special construction was developed.

  7. Setup (gas target) Entrance window  C1 & C2 Vessel walls   plastic scintillator C3

  8. Gas vessel (C3) covered with black paper PSI,2006 PMT(C3) Gas inlet PMT(C1) Beam entrance PMC(C2)

  9. PSI,2006 physicist

  10. What do we observe?: • (Background) radiation not connected directly to muons (uncorrelated spectrum) • Cascade of muonic X-rays (prompt spectrum) • Nuclear g-rays following m-capture (delayed spectrum)

  11. Time [ns] Energy [keV]

  12. Spectra with 82Kr target

  13. Time evolution (method) The fragment number (each fragment corresponds to 10 ns time period)

  14. Muon life-time in Kr isotopes

  15. Our results for Kr and Sm:

  16. Dependence of λcapt.on(Z,A): • Total capture rate reflects the collective properties of the nucleus • Primakoff’s rule : λc=(Zeff)4 ∙ X1 · {1 - X2∙(A-Z)/2A} X1 = 120..170 X2 ≈ 3.0

  17. Effective Z-values and Huff factors taken from NP 35(1962)295

  18. Primakoff’s rule for different isotopes:

  19. Conclusions: • Some of our results contradict to theory Wrong measurement? Wrong interpretation? Wrong Primakoff rule? Wrong Zeff? • What can we do with this? Any ideas? • In any case, our L-values are necessary (and really are used) in extraction of partial capture rates – next talk.

  20. Thanks for your attention!

More Related