gamma-ray spectroscopy - uniwersytet warszawski · gamma-ray spectroscopy radoslav marchevski...
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![Page 1: Gamma-ray Spectroscopy - Uniwersytet Warszawski · Gamma-ray Spectroscopy Radoslav Marchevski (University of Sofia) Angie Karina Orduz (University of Huelva) Osman Ağar (Akdeniz](https://reader033.vdocuments.us/reader033/viewer/2022042710/5f6442617bea20242f5643c0/html5/thumbnails/1.jpg)
Gamma-ray Spectroscopy
Radoslav Marchevski (University of Sofia)
Angie Karina Orduz (University of Huelva)
Osman Ağar (Akdeniz University)
Supervisors
M. Palacz - T. Abraham
International Workshop on Acceleration and Applications of Heavy Ions, Warszawa, 26.02 – 10.03.2012
![Page 2: Gamma-ray Spectroscopy - Uniwersytet Warszawski · Gamma-ray Spectroscopy Radoslav Marchevski (University of Sofia) Angie Karina Orduz (University of Huelva) Osman Ağar (Akdeniz](https://reader033.vdocuments.us/reader033/viewer/2022042710/5f6442617bea20242f5643c0/html5/thumbnails/2.jpg)
Agenda
● Introduction
● Setup
● Target preparation
● Calibration
-Energy calibration
-Efficiency calibration
● Data Analysis
-Identifying nuclei
-Relative population of different reaction channels
● Summary
![Page 3: Gamma-ray Spectroscopy - Uniwersytet Warszawski · Gamma-ray Spectroscopy Radoslav Marchevski (University of Sofia) Angie Karina Orduz (University of Huelva) Osman Ağar (Akdeniz](https://reader033.vdocuments.us/reader033/viewer/2022042710/5f6442617bea20242f5643c0/html5/thumbnails/3.jpg)
Introduction
We used a 2 0Ne beam with an energy of 54MeV at a target of 2 7Al to obtain a compound nucleus 4 7V. Various combinations of particles p, n, and α are emmited from CN leading to different residual nuclei.
20Ne 27Al
47V
We register the γ rays and in this way we determine properties of the excited states of the residual nuclei.
![Page 4: Gamma-ray Spectroscopy - Uniwersytet Warszawski · Gamma-ray Spectroscopy Radoslav Marchevski (University of Sofia) Angie Karina Orduz (University of Huelva) Osman Ağar (Akdeniz](https://reader033.vdocuments.us/reader033/viewer/2022042710/5f6442617bea20242f5643c0/html5/thumbnails/4.jpg)
Setup
We used 13 compton suppressed Ge detectors
EAGLE
![Page 5: Gamma-ray Spectroscopy - Uniwersytet Warszawski · Gamma-ray Spectroscopy Radoslav Marchevski (University of Sofia) Angie Karina Orduz (University of Huelva) Osman Ağar (Akdeniz](https://reader033.vdocuments.us/reader033/viewer/2022042710/5f6442617bea20242f5643c0/html5/thumbnails/5.jpg)
Target
2.3 mg/cm2
54MeV
2 mg/cm2
Stopping the residual nuclei Slowing down to Ec
Ec=37.2 MeV (Coulomb barrier)
Target thickness including safety margin : 5.4 mg/cm2
Target preparation using rolling method
20 µ m
Thanks to Anna Stolarz
27Al
![Page 6: Gamma-ray Spectroscopy - Uniwersytet Warszawski · Gamma-ray Spectroscopy Radoslav Marchevski (University of Sofia) Angie Karina Orduz (University of Huelva) Osman Ağar (Akdeniz](https://reader033.vdocuments.us/reader033/viewer/2022042710/5f6442617bea20242f5643c0/html5/thumbnails/6.jpg)
Energy Calibration
Energy calibration: translating channel numbers (from ADC)to true energy of gamma rays E= f(x) x-channel number
226Ra 156Eu
137Ba
Used sources
● Positions Xi of peaks corresponding to known γ-ray energies E
i are
determined
● A function E = f(x) is fitted to (Ei,X
i) points
![Page 7: Gamma-ray Spectroscopy - Uniwersytet Warszawski · Gamma-ray Spectroscopy Radoslav Marchevski (University of Sofia) Angie Karina Orduz (University of Huelva) Osman Ağar (Akdeniz](https://reader033.vdocuments.us/reader033/viewer/2022042710/5f6442617bea20242f5643c0/html5/thumbnails/7.jpg)
Energy Calibration-Deviation from linearity 226Ra source
[keV
]
[keV]
![Page 8: Gamma-ray Spectroscopy - Uniwersytet Warszawski · Gamma-ray Spectroscopy Radoslav Marchevski (University of Sofia) Angie Karina Orduz (University of Huelva) Osman Ağar (Akdeniz](https://reader033.vdocuments.us/reader033/viewer/2022042710/5f6442617bea20242f5643c0/html5/thumbnails/8.jpg)
Energy calibration-deviation from linear
Detector 3 Detector 4
-All detectors have similar nonlinearity 226Ra source
![Page 9: Gamma-ray Spectroscopy - Uniwersytet Warszawski · Gamma-ray Spectroscopy Radoslav Marchevski (University of Sofia) Angie Karina Orduz (University of Huelva) Osman Ağar (Akdeniz](https://reader033.vdocuments.us/reader033/viewer/2022042710/5f6442617bea20242f5643c0/html5/thumbnails/9.jpg)
Energy Calibration
-Deviation from third order polynomial fit 226Ra source
[keV]
[keV
]
![Page 10: Gamma-ray Spectroscopy - Uniwersytet Warszawski · Gamma-ray Spectroscopy Radoslav Marchevski (University of Sofia) Angie Karina Orduz (University of Huelva) Osman Ağar (Akdeniz](https://reader033.vdocuments.us/reader033/viewer/2022042710/5f6442617bea20242f5643c0/html5/thumbnails/10.jpg)
Efficiency calibration
Energy [keV]
Relative Efficiency of EAGLE
400 800 1200 1600 2000 2400 2800
50
100
200
500
152Eu, 133Ba, 226Ra
ϵ(Eγ)=N detected
A k t d
![Page 11: Gamma-ray Spectroscopy - Uniwersytet Warszawski · Gamma-ray Spectroscopy Radoslav Marchevski (University of Sofia) Angie Karina Orduz (University of Huelva) Osman Ağar (Akdeniz](https://reader033.vdocuments.us/reader033/viewer/2022042710/5f6442617bea20242f5643c0/html5/thumbnails/11.jpg)
Total gamma-ray spectrum
Energy [keV]
30000
70000
3000
7000
11000
511
keV
- about 3 hours of data taking
![Page 12: Gamma-ray Spectroscopy - Uniwersytet Warszawski · Gamma-ray Spectroscopy Radoslav Marchevski (University of Sofia) Angie Karina Orduz (University of Huelva) Osman Ağar (Akdeniz](https://reader033.vdocuments.us/reader033/viewer/2022042710/5f6442617bea20242f5643c0/html5/thumbnails/12.jpg)
Gamma-gamma coincidences
400 800 1200 160085
1
708
1500
E [keV]
246
400 800E [keV]
1200 1600
708
151314
68
41k_a 41k_b 41k_c
![Page 13: Gamma-ray Spectroscopy - Uniwersytet Warszawski · Gamma-ray Spectroscopy Radoslav Marchevski (University of Sofia) Angie Karina Orduz (University of Huelva) Osman Ağar (Akdeniz](https://reader033.vdocuments.us/reader033/viewer/2022042710/5f6442617bea20242f5643c0/html5/thumbnails/13.jpg)
Reaction products - relative yields 20Ne (54 MeV) + 27Al ----> 47V (CN)
19 20 21 22 23 24 N/Z42V 43V 44V 45V 46V
47V CN
23
41Ti 42Ti 43Ti 44Ti4.3%p2n
45Ti11.6%pn
46Ti 22
40Sc 41Sc 42Sc1.2%αn/3n2p
43Sc 44Sc23.3%2pn
45Sc10.2%2p
21
39Ca 40Ca 41Ca7.8%αpn/3p3n
42Ca29.1%αp/3p2n
43Ca 44Ca0.7%3p
20
38K 39K4.6%2α/4p4n
40K 41K4.0%α2p/4p2n
42K 43K 19
37Ar 38Ar3.2%2αp/5p4n
39Ar 40Ar 41Ar 42Ar 18
![Page 14: Gamma-ray Spectroscopy - Uniwersytet Warszawski · Gamma-ray Spectroscopy Radoslav Marchevski (University of Sofia) Angie Karina Orduz (University of Huelva) Osman Ağar (Akdeniz](https://reader033.vdocuments.us/reader033/viewer/2022042710/5f6442617bea20242f5643c0/html5/thumbnails/14.jpg)
42Ca
Level Scheme
42ca_a 42ca_b 42ca_c 42ca_d 42ca_e
![Page 15: Gamma-ray Spectroscopy - Uniwersytet Warszawski · Gamma-ray Spectroscopy Radoslav Marchevski (University of Sofia) Angie Karina Orduz (University of Huelva) Osman Ağar (Akdeniz](https://reader033.vdocuments.us/reader033/viewer/2022042710/5f6442617bea20242f5643c0/html5/thumbnails/15.jpg)
Level Scheme
41Ca Shell Model orbitals
41ca_a 42ca_b
![Page 16: Gamma-ray Spectroscopy - Uniwersytet Warszawski · Gamma-ray Spectroscopy Radoslav Marchevski (University of Sofia) Angie Karina Orduz (University of Huelva) Osman Ağar (Akdeniz](https://reader033.vdocuments.us/reader033/viewer/2022042710/5f6442617bea20242f5643c0/html5/thumbnails/16.jpg)
Summary
● We used EAGLE setup to study 2 0Ne + 2 7Al → 4 7V (CN)
● Target preparation
● Energy and efficiency calibration
● Identified 11 different reaction products
● Relative yields determined
![Page 17: Gamma-ray Spectroscopy - Uniwersytet Warszawski · Gamma-ray Spectroscopy Radoslav Marchevski (University of Sofia) Angie Karina Orduz (University of Huelva) Osman Ağar (Akdeniz](https://reader033.vdocuments.us/reader033/viewer/2022042710/5f6442617bea20242f5643c0/html5/thumbnails/17.jpg)
Thank You for your
attention!