CATRiNA: Difference between revisions

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The 9821B (4" x 2") PMTs:
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Revision as of 15:02, 8 October 2026

CATRiNA at Gamma Station beamline

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 (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 \textrm{C}_6 \textrm{D}_6 } ) liquid scintillators. The array consists of 16 "small" detectors which has 2" x 2" aluminum cell each and 16 "large" detectors that has a 4" x 2" aluminum cell each. 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 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 \theta } , incident neutron energy 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 E_n } , and nucleon number of target nucleus 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 A }

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 E_{recoil} = \frac{4A}{(1+A)^2}cos^2\theta E_n }

For maximum energy transfer, 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 \theta = 0 } , and

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 E_{recoil} = \frac{4A}{(1+A)^2} E_n }

For deuterium, 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 A = 2 } which implies a maximum deposited neutron energy of 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 E_{recoil}/E_n = \frac{8}{9} } .

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. 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

CATRiNA cable connection

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.

Local shaped trigger setting for CATRiNA.png

also, the TRG-OUT Mode is Trigger (Mask) and the TRG-OUT Mask buttons are green for all channels. CATRiNA TRG-OUT setting.png

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

  1. ↑ J. F. Perello et al. NIMA 930, 196 (2019) https://doi.org/10.1016/j.nima.2019.03.084
  2. ↑ 2.0 2.1 A. B. Morelock et al. NIMA 1034, 166759 (2022) https://doi.org/10.1016/j.nima.2022.166759