CATRiNA: Difference between revisions
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[[File:CATRiNA at Gamma Station beamline.png|600px|thumb|right|CATRiNA at Gamma Station beamline]] | [[File:CATRiNA at Gamma Station beamline.png|600px|thumb|right|CATRiNA at Gamma Station beamline]] | ||
= Introduction = | = Introduction = | ||
The '''C'''ompound '''A'''rray for '''T'''ransfer '''R'''eactions '''i'''n '''N'''uclear '''A'''strophysics (CATRiNA) <ref name="Perello2019">J. F. Perello et al. NIMA '''930''', 196 (2019) https://doi.org/10.1016/j.nima.2019.03.084 </ref> is a neutron detector array located at Florida State University. CATRiNA is composed of 32 deuterated-benzene (<math> \textrm{C}_6 \textrm{D}_6 </math>) liquid scintillators. The array consists of 16 "small" detectors | The '''C'''ompound '''A'''rray for '''T'''ransfer '''R'''eactions '''i'''n '''N'''uclear '''A'''strophysics (CATRiNA) <ref name="Perello2019">J. F. Perello et al. NIMA '''930''', 196 (2019) https://doi.org/10.1016/j.nima.2019.03.084 </ref> is a neutron detector array located at Florida State University. CATRiNA is composed of 32 deuterated-benzene (<math> \textrm{C}_6 \textrm{D}_6 </math>) liquid scintillators. The array consists of 16 "small" detectors each contained in a 2" x 2" (diameter x thickness) aluminum cell and 16 "large" detectors that are each contained in 4" x 2" aluminum cells. Due to the anisotropic light-output spectrum of of neutron-deuterium scattering, the light-output can be converted to the neutron energy without time-of-flight information in a process known as spectrum unfolding <ref name="Morelock2022">A. B. Morelock et al. NIMA '''1034''', 166759 (2022) https://doi.org/10.1016/j.nima.2022.166759 </ref>. Please refer [[https://fsunuc.physics.fsu.edu/wiki/index.php/Python_Iseg_HV_controller | here]] for setting up the HV source for CATRiNA. | ||
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|- | |- | ||
|4" x 2" || 0.6109 || 1.946 || 0.2625 | |4" x 2" || 0.6109 || 1.946 || 0.2625 | ||
|} | |||
= PMT Bias = | |||
The CATRiNA Photo-Multiplier Tubes (PMTs) require bias to function. The PMT channel number will be drawn in black ink on the PVC pipe covering the detector. Below is a table of optimized biases for the R7724 (2" x 2") PMTs: | |||
{|class='wikitable' | |||
! PMT Channel !! Bias (V) | |||
|- | |||
|0 || -1225 | |||
|- | |||
|1 || -1225 | |||
|- | |||
|2 || -1225 | |||
|- | |||
|3 || -1225 | |||
|- | |||
|4 || -1225 | |||
|- | |||
|5 || -1275 | |||
|- | |||
|6 || -1400 | |||
|- | |||
|7 || -1400 | |||
|- | |||
|8 || -1200 | |||
|- | |||
|9 || -1400 | |||
|- | |||
|10 || -1250 | |||
|- | |||
|11 || -1225 | |||
|- | |||
|12 || -1325 | |||
|- | |||
|13 || -1300 | |||
|- | |||
|14 || -1375 | |||
|- | |||
|15 || -1300 | |||
|} | |||
The 9821B (4" x 2") PMTs: | |||
{|class='wikitable' | |||
! PMT Channel !! Bias (V) | |||
|- | |||
|0 || -1725 | |||
|- | |||
|1 || -1700 | |||
|- | |||
|2 || -1675 | |||
|- | |||
|3 || -1800 | |||
|- | |||
|4 || -1700 | |||
|- | |||
|5 || -1750 | |||
|- | |||
|6 || -1650 | |||
|- | |||
|7 || -1725 | |||
|- | |||
|8 || -1750 | |||
|- | |||
|9 || -1725 | |||
|- | |||
|10 || -1725 | |||
|- | |||
|11 || -1800 | |||
|- | |||
|12 || -1700 | |||
|- | |||
|13 || -1725 | |||
|- | |||
|14 || -1885 | |||
|- | |||
|15 || -1735 | |||
|} | |} | ||
Latest revision as of 16:06, 8 October 2026
Introduction
The Compound Array for Transfer Reactions in Nuclear Astrophysics (CATRiNA) [1] is a neutron detector array located at Florida State University. CATRiNA is composed of 32 deuterated-benzene () liquid scintillators. The array consists of 16 "small" detectors each contained in a 2" x 2" (diameter x thickness) aluminum cell and 16 "large" detectors that are each contained in 4" x 2" aluminum cells. Due to the anisotropic light-output spectrum of of neutron-deuterium scattering, the light-output can be converted to the neutron energy without time-of-flight information in a process known as spectrum unfolding [2]. Please refer [| here] for setting up the HV source for CATRiNA.
Light-Output Response
From page 570-571 of Radiation Detection and Measurement by Knoll, the recoil neutron energy is given as a function of the target recoil angle in the lab frame , incident neutron energy , and nucleon number of target nucleus
For maximum energy transfer, , and
For deuterium, which implies a maximum deposited neutron energy of .
From previous work, the light-output response of a given CATRiNA detector can be parameterized as a function of incident neutron energy and experimentally-extracted parameters:
Failed to parse (SVG with PNG fallback (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle LO = aE_{dep}-b(1-e^{-cE_{dep}}) }
The light output parameters are given by the following table [2]
| Size | a | b | c |
|---|---|---|---|
| 2" x 2" | 0.6193 | 2.036 | 0.2592 |
| 4" x 2" | 0.6109 | 1.946 | 0.2625 |
PMT Bias
The CATRiNA Photo-Multiplier Tubes (PMTs) require bias to function. The PMT channel number will be drawn in black ink on the PVC pipe covering the detector. Below is a table of optimized biases for the R7724 (2" x 2") PMTs:
| PMT Channel | Bias (V) |
|---|---|
| 0 | -1225 |
| 1 | -1225 |
| 2 | -1225 |
| 3 | -1225 |
| 4 | -1225 |
| 5 | -1275 |
| 6 | -1400 |
| 7 | -1400 |
| 8 | -1200 |
| 9 | -1400 |
| 10 | -1250 |
| 11 | -1225 |
| 12 | -1325 |
| 13 | -1300 |
| 14 | -1375 |
| 15 | -1300 |
The 9821B (4" x 2") PMTs:
| PMT Channel | Bias (V) |
|---|---|
| 0 | -1725 |
| 1 | -1700 |
| 2 | -1675 |
| 3 | -1800 |
| 4 | -1700 |
| 5 | -1750 |
| 6 | -1650 |
| 7 | -1725 |
| 8 | -1750 |
| 9 | -1725 |
| 10 | -1725 |
| 11 | -1800 |
| 12 | -1700 |
| 13 | -1725 |
| 14 | -1885 |
| 15 | -1735 |
Digitizer setup for coincident with RF
Digitizer 1 is the master, and received the RF-coin signal. Digitizer 2 and 3 are the slaves, connected to the neutron detectors
The TRG-OUT of digi-2 and -3 will be "on" when ever any channel is fired. To do so, the Local Shaped Trigs [G] must be OR.
also, the TRG-OUT Mode is Trigger (Mask) and the TRG-OUT Mask buttons are green for all channels.
Time sync
Digitizer 1 is SW controll and internal clock. The TRG-OUT mode is "RUN".
Digitizer 2 and 3 are S-IN and external clock.
Contact
Sergio Almaraz-Calderon mailto:salmarazcalderon@fsu.edu
References
- ↑ J. F. Perello et al. NIMA 930, 196 (2019) https://doi.org/10.1016/j.nima.2019.03.084
- ↑ 2.0 2.1 A. B. Morelock et al. NIMA 1034, 166759 (2022) https://doi.org/10.1016/j.nima.2022.166759