Difference between revisions of "PAA Selenium"

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=Can one use plant material to measure the provenance of selenium?=
 
=Can one use plant material to measure the provenance of selenium?=
  
=Can one perform PAA measurements of Se-82 and Se-76?=
+
[[Se_Overview_PrevMeas]]
  
 +
As shown in the Figure below, the Se-82/Se-76 ratio varies from -1.2% to +0.2% for plant materials but remains relatively constant for other materials.  The variations in plant material has been described as being due to differences in the bacteria residing in the plant.  The question to investigate is whether or not these variations in the concentration can be used to determine the provenance of the sample.
  
==Neutron knockout of Se-82==
 
If you knock a neutron out of Se-82 you produce the unstable isotope Se-81 which Beta emitts with half life of 18 min and a meta-state that emmits a 103 keV gamma with a 57 minute half life.
 
  
<math>{82 \atop 34\; }Se (\gamma,n){81 \atop \; }Se</math>
 
  
Other prominent photons
 
  
260 & 276 keV for the 57 minute half life isotope
+
[[File:Krouse_Fig_1.png | 200 px]]
  
==Neutron knockout of Se-76==
+
== Below is a table listing the natural abundances of Selenium==
If you knock a neutron out of Se-76 you produce the unstable isotope Se-75 which has a half life of 119 days.
+
Natural abundance of selenium
  
<math>{76 \atop\; }Se (\gamma,n){75 \atop \; }Se</math>
+
{| border="3"  cellpadding="5" cellspacing="0"
 +
|  Isotope|| Abundance
 +
|-
 +
| Se-74  || 0.86%
 +
|-
 +
| Se-76 || 9.23%
 +
|-
 +
| Se-77 || 7.60%
 +
|-
 +
| Se-78 || 23.69%
 +
|-
 +
| Se-80 || 49.80%
 +
|-
 +
| Se-82 || 8.82%
 +
|}
  
The prominent photons emitted have the following energies
+
== Below are possible PAA reactions that may be used to observe specific Se isotopes==
  
136, 264, and 279 keV
+
{| border="3"  cellpadding="5" cellspacing="0"
 +
|  Reaction|| Half-life ||Relative activity ||Gamma-rays, keV (BR)
 +
|-
 +
| Se-74(gamma,n)Se-73  || 7.1 h || 1.5E-1 || 361 (100)
 +
|-
 +
| Se-74(gamma,n)Se-73m  || 39 m || 3.2 || 402 (4)
 +
|-
 +
| Se-74(gamma,np)As-72  || 26 h || 1.0E-3 || 834 (100)
 +
|-
 +
| Se-76(gamma,n)Se-75  || 120 d || 1.3E-2 || 265(29)
 +
|-
 +
| Se-77(gamma,p)As-76  || 26.4 h || 4.4E-2 || 559(44)
 +
|-
 +
| Se-78(gamma,p)As-77  || 38.8 h || 8.6E-2 || 239(2)
 +
|-
 +
| Se-80(gamma,n)Se-79m  || 3.9 m || 5.9 || 96(10)
 +
|-
 +
| Se-80(gamma,np)As-78 || 1.5 h || 2.2E-2 || 614(54)
 +
|-
 +
| Se-80(gamma,p)As-79  || 8.2 m || 1.3 || 96(9)
 +
|-
 +
| Se-80(gamma,<math>a</math>p)Ge-75  || 83 m || 2.8E-1 || 265(11)
 +
|-
 +
|}
  
 +
=Can one perform PAA measurements of Se-82 and Se-76?=
  
The article below describes how plant material and soil contain Se-76 to Se-82 ratios that differ from other natural samples by 1.5%.  They argue that it is due to the bacteria living in plant material. 
+
[[Se_PAA_Reactions]]
 
 
[[File:Krouse_CanJournChem_40_1962_p367.pdf]]
 
 
 
Plant material is a natural way to sample the selenium content to determine if there are difference isotopic ratios due to the impact of human activities on the environment.
 
  
 
=Experiments=
 
=Experiments=
  
==Chlorine==
+
==[[PAA_Selenium_ActivityCalc]]==
  
It looks like Cl-35 is abundant as you see photon energies of 146 keV and 2127 keV (you can barely see 1176 keV) from Cl-34's decay (neutron knocked out of Cl-35).
+
[[PAA Selenium/Soil Experiments]]
  
The half life is 32 minutes.
+
[[LB Se PAA Horse Feed Experiment]]
  
Should check the half life from the run AccOnAlInDetASe-AinDetD_001.root using the calibration
+
==Background Signals==
 +
[[PAA_BackGrd_Det_A]]
  
MPA->Draw("0.18063+0.960133*evt.Chan>> SeRun_008(8000,0.5,8000.5)","evt.ADCid==3");
+
==Nickel Normalization==
 +
[[LB PAA Nickel Investigation]]
  
== Irradiation of Horse Mineral Supplement==
+
== First Observation of Se lines==
  
=== Chlorine is a dominant signal===
+
Using the 44 Machine at 7 kW power and 44 meV incident electron energy to produce a bremsstrahlung spectrum with a mean energy of 15 meV.
  
  
First, look at the peak around 146 keV
+
All runs lasting less than 214 seconds have time stamp that gives real time if you divide by clock frequency of 20 MHz. The first 32 bits are used for a real time measurement.
https://wiki.iac.isu.edu/index.php/File:146_keV.png
 
  
Next I plotted the counts as a function of time to get an exponentially decaying graph. When doing an exponential fit here, the parameter "b" given by root will be the decay constant.
 
  
https://wiki.iac.isu.edu/index.php/File:Counts_vs_time_146kev.png
+
== MDA and Se mass Calculations ==
 +
[[LB MDA/Se Mass Calculations]]
  
Root gives a value b = 3.83655x10^-4, which yields a half life of 30.11 minutes.
+
==IAC Detector Efficiencies ==
  
 +
[[LB PAA IAC Detector Efficiencies]]
  
Now do the same for the 2127 keV line
+
==IAC Detector Calibrations==
https://wiki.iac.isu.edu/index.php/File:2127_keV.png
 
  
Here are the counts plotted as a function of time
+
[[LB April DetB DetA Calibration]]
https://wiki.iac.isu.edu/index.php/File:Counts_vs_time_2127keV.png
 
  
Root gives b = 3.31508x10^-4, which yields a half life of 34.8 minutes.
+
==Runlists==
 +
[[LB PAA Runlist 4/01/16 - 06/02/16]]
  
===Possible Yb-167 in the Sample===
+
[[LB March 2017 Runlist]]
  
Yb-167 has a half life of 17.5 minutes and can be produced by knocking a neutron out of Yb-168, which is stable.
+
[[LB_May_2017_Irradiation_Day]]
  
I looked at the horse feed spectrum and compared the spectral lines for Yb-167, below is a table of those results:
+
=Data Analysis=
  
  
 +
[[LB_Feb2017_Se_Investigations]]
  
{| border="3"  cellpadding="5" cellspacing="0"
+
=References=
| Energy (keV) || Spectrum Energy (keV) || Half life (min)
 
|-
 
| 90.84 || 89 || 18.23
 
|-
 
| 106.18 || 105 || 18.0
 
|-
 
| 112.88 || 113 || 18.86
 
|-
 
| 132.02 || 137 || 19.2 
 
|-
 
| 161.29 || 161 || 17.3 
 
|-
 
| 203.75 || 204 || 17.27
 
|-
 
| 280.5 || 281 || 17.0
 
|-
 
| 290.89|| 289 || 16.7 
 
|-
 
| 323.5|| 322 || 16.6
 
|-
 
| 354.0 || 354|| 16.7 
 
|-
 
| 375.9 || 378|| 15.5
 
|-
 
| 387.0 || 388.4|| 19.1
 
|-
 
| 398.1 || 402||  16.1
 
|-
 
|688.5 || 691 || 15.6
 
|-
 
|733.2 || 736 || 17.1
 
|-
 
|920.32 || 922 || 16.6
 
|-
 
|977.9 || 980 || 16.9
 
|-
 
|1025.9 || 1028 || 16.9
 
|-
 
|1242 || 1245 || 17.5
 
|-
 
|1340.1 || 1341 || 16.5
 
|-
 
|1410.4 || 1413 || 18.6
 
|-
 
|1433.4 || 1437 || 16
 
|-
 
|1631.7 || 1630 || 19.6
 
|-
 
|}
 
  
The average of these half lives is 17.22 minutes. Also the relative intensity for the 106.18 and the 112.88 lines is about 2. Below are some histograms to verify this is indeed the case.
 
  
== First Observation of Se lines==
+
[[User_talk:Brenleyt]]
  
Using the 44 Machine at 7 kW power and 44 meV incident electron energy to produce a bremsstrahlung spectrum with a mean energy of 15 meV.
 
  
 +
<references/>
  
All runs lasting less than 214 seconds have time stamp that gives real time if you divide by clock frequency of 20 MHz.  The first 32 bits are used for a real time measurement.
+
[[File:Krouse_CanJournChem_40_1962_p367.pdf]]
  
+
Goryachev, A. M., & Zalesnyy, G. N. (n.d.). The studying of the photoneutron reactions cross sections in the region of the giant dipole resonance in zinc, germanium, selenium, and strontium isotopes. Retrieved September 16, 2016, from http://www-nds.indcentre.org.in/exfor/servlet/X4sSearch5?EntryID=220070
  
[[SeRun_01-11-16]]
+
Goryachev, B. I., Ishkhanov, B. S., Kapitonov, I. M., Piskarev, I. M., Piskarev, V. G., & Piskarev, O. P. (n.d.). Giant Dipole Resonance on Ni Isotopes. Retrieved October 26, 2016, from http://www-nds.indcentre.org.in/exfor/servlet/X4sGetSubent?reqx=119235&subID=220597006&plus=1
  
[[SeRun_03-07-16]]
 
  
=References=
 
  
<references/>
+
Handbook on Photonuclear data for applications, cross sections, and spectra. (2000, October). Retrieved November 4, 2016, from http://www-pub.iaea.org/MTCD/Publications/PDF/te_1178_prn.pdf
  
 
=MSDS=
 
=MSDS=

Latest revision as of 22:10, 17 May 2019

Using PAA ro measure Selenium concentrations.

According to Krouse<ref name="Krous1962"> H.R. Krause and H.G. Thode,"Thermodynamic Properties and Geochemistry of Iosotopic Compounds of Selenium",.Can. J. Chem., vol 40, pg 367</ref> , the fractional concentration of Se-82/Se-76 in plant material is observed to be less than from primordial (meteoric) concentrations by as much as 1.2%. Anaerobic bacteria are known to reduce selenates and senelites in biological systems. This may be the reason plant material has fractionation of selenium isotopes. They also observe excess concentrations of up to 0.4% in soil.


Plant material appears to detect environmental selenium.

Can one use plant material to measure the provenance of selenium?

Se_Overview_PrevMeas

As shown in the Figure below, the Se-82/Se-76 ratio varies from -1.2% to +0.2% for plant materials but remains relatively constant for other materials. The variations in plant material has been described as being due to differences in the bacteria residing in the plant. The question to investigate is whether or not these variations in the concentration can be used to determine the provenance of the sample.



Krouse Fig 1.png

Below is a table listing the natural abundances of Selenium

Natural abundance of selenium

Isotope Abundance
Se-74 0.86%
Se-76 9.23%
Se-77 7.60%
Se-78 23.69%
Se-80 49.80%
Se-82 8.82%

Below are possible PAA reactions that may be used to observe specific Se isotopes

Reaction Half-life Relative activity Gamma-rays, keV (BR)
Se-74(gamma,n)Se-73 7.1 h 1.5E-1 361 (100)
Se-74(gamma,n)Se-73m 39 m 3.2 402 (4)
Se-74(gamma,np)As-72 26 h 1.0E-3 834 (100)
Se-76(gamma,n)Se-75 120 d 1.3E-2 265(29)
Se-77(gamma,p)As-76 26.4 h 4.4E-2 559(44)
Se-78(gamma,p)As-77 38.8 h 8.6E-2 239(2)
Se-80(gamma,n)Se-79m 3.9 m 5.9 96(10)
Se-80(gamma,np)As-78 1.5 h 2.2E-2 614(54)
Se-80(gamma,p)As-79 8.2 m 1.3 96(9)
Se-80(gamma,[math]a[/math]p)Ge-75 83 m 2.8E-1 265(11)

Can one perform PAA measurements of Se-82 and Se-76?

Se_PAA_Reactions

Experiments

PAA_Selenium_ActivityCalc

PAA Selenium/Soil Experiments

LB Se PAA Horse Feed Experiment

Background Signals

PAA_BackGrd_Det_A

Nickel Normalization

LB PAA Nickel Investigation

First Observation of Se lines

Using the 44 Machine at 7 kW power and 44 meV incident electron energy to produce a bremsstrahlung spectrum with a mean energy of 15 meV.


All runs lasting less than 214 seconds have time stamp that gives real time if you divide by clock frequency of 20 MHz.  The first 32 bits are used for a real time measurement.


MDA and Se mass Calculations

LB MDA/Se Mass Calculations

IAC Detector Efficiencies

LB PAA IAC Detector Efficiencies

IAC Detector Calibrations

LB April DetB DetA Calibration

Runlists

LB PAA Runlist 4/01/16 - 06/02/16

LB March 2017 Runlist

LB_May_2017_Irradiation_Day

Data Analysis

LB_Feb2017_Se_Investigations

References

User_talk:Brenleyt


<references/>

File:Krouse CanJournChem 40 1962 p367.pdf

Goryachev, A. M., & Zalesnyy, G. N. (n.d.). The studying of the photoneutron reactions cross sections in the region of the giant dipole resonance in zinc, germanium, selenium, and strontium isotopes. Retrieved September 16, 2016, from http://www-nds.indcentre.org.in/exfor/servlet/X4sSearch5?EntryID=220070

Goryachev, B. I., Ishkhanov, B. S., Kapitonov, I. M., Piskarev, I. M., Piskarev, V. G., & Piskarev, O. P. (n.d.). Giant Dipole Resonance on Ni Isotopes. Retrieved October 26, 2016, from http://www-nds.indcentre.org.in/exfor/servlet/X4sGetSubent?reqx=119235&subID=220597006&plus=1


Handbook on Photonuclear data for applications, cross sections, and spectra. (2000, October). Retrieved November 4, 2016, from http://www-pub.iaea.org/MTCD/Publications/PDF/te_1178_prn.pdf

MSDS

Selenium shot, amorphous, 2-6 mm, Puratronic, 99.999% Alfa Aesar product # 10603 File:AlphaAesarSelenium MDSD.pdf

Informative links

http://www.deq.idaho.gov/regional-offices-issues/pocatello/southeast-idaho-phosphate-mining/southeast-idaho-selenium-investigations/

https://inldigitallibrary.inl.gov/sti/3169894.pdf

http://giscenter.isu.edu/research/Techpg/sisp/index.htm


PAA_Research