Content deleted Content added
m clean up, typo(s) fixed: ie → i.e., add reflist |
|||
Line 6:
PAC goes back to a theoretical work by Donald R. Hamilton <ref>Donald R. Hamilton: On Directional Correlation of Successive Quanta. In: Physical Review. Band 58, Nr. 2, 15. Juli 1940, S. 122–131, doi:10.1103/PhysRev.58.122</ref> from 1940. The first successful experiment was carried out by Brady and Deutsch <ref>Edward L. Brady, Martin Deutsch: Angular Correlation of Successive Gamma-Ray Quanta. In: Physical Review. Band 72, Nr. 9, 1. November 1947, S. 870–871, doi:10.1103/PhysRev.72.870</ref> in 1947. Essentially spin and parity of nuclear spins were investigated in these first PAC experiments. However, it was recognized early on that electric and magnetic fields interact with the nuclear moment, providing the basis for a new form of material investigation: nuclear solid-state spectroscopy.
After Abragam and Pound <ref>A. Abragam, R. V. Pound: Influence of Electric and Magnetic Fields on Angular Correlations. In: Physical Review. Band 92, Nr. 4, 15. November 1953, S. 943–962, doi:10.1103/PhysRev.92.943</ref> published their work on the theory of PAC in 1953, many studies with PAC were carried out afterwards. In the 1960s and 1970s, interest in PAC experiments sharply increased, focusing mainly on magnetic and electric fields in crystals into which the probe nuclei were introduced. In the mid-1960s, ion implantation was discovered, providing new opportunities for sample preparation. The rapid electronic development of the 1970s brought significant improvements in signal processing. From the 1980s to the present, PAC has emerged as an important method for the study and characterization of materials
While until about 2008 PAC instruments used conventional high-frequency electronics of the 1970s, in 2008 Christian Herden and Jens Röder et al. developed the first fully-digitized PAC instrument that enables extensive data analysis and parallel use of multiple probes.
==Measuring principle ==
Line 36:
== Sample preparation ==
The amount of suitable PAC isotopes required for a measurement is between about 10 to 1000 billion atoms (10<sup>10</sup>-10<sup>12</sup>). The right amount depends on the particular properties of the isotope. 10 billion atoms are a very small amount of substance. For comparison, one mol contains about 6.22x10<sup>23</sup> particles. 10<sup>12</sup> atoms in one cubic centimeter of beryllium give a concentration of about 8 nmol/L (nanomol=10<sup>
How the PAC isotopes are brought into the sample to be examined is up to the experimenter and the technical possibilities. The following methods are usual:
Line 52:
=== Added during synthesis ===
PAC probes may also be added during the synthesis of sample materials to achieve the most uniform distribution in the sample. This method is particularly well suited if, for example, the PAC probe diffuses only poorly in the material and a higher concentration in grain boundaries is to be expected. Since only very small samples are necessary with PAC (about 5
=== Neutron activation ===
Line 67:
</math>
For a <math>\gamma</math>-<math>\gamma</math>-cascade, <math>k</math> is due to the preservation of [[
▲For a <math>\gamma</math>-<math>\gamma</math>-cascade, <math>k</math> is due to the preservation of [[parity_(physics)|parity]]:
:<math>0<k<\textrm{min}(2I_S, I_i+I'_i)
</math>
Where <math>I_S</math> is the spin of the intermediate state and <math>I_i</math> with <math>i=1;2</math> the [[
<math>A_ {kk}</math> is the anisotropy coefficient that depends on the [[angular momentum]] of the intermediate state and the multipolarities of the transition.
The radioactive nucleus is built into the sample material and emits two <math>\gamma</math>-quanta upon decay. During the lifetime of the intermediate state,
:<math>W(\Theta)=\sum^{k_{max}}_{k}A_{kk}G_{kk}
Line 95 ⟶ 94:
</math>
<math>g</math> is the [[
With <math>N=M-M'</math> follows:
Line 153 ⟶ 152:
In cubic crystals, the axis parameters of the unit cell x, y, z are of the same length. Therefore:
:<math>V_{zz}=V_{yy}=V_{xx}</math> and <math>\eta=0</math>
In axisymmetric systems is <math>\eta=0</
For axially symmetric electric field gradients, the energy of the substates has the values:
Line 201 ⟶ 200:
For half integer spins applies:
:<math>\omega_0=6\cdot\omega_Q</math> und <math>n=\frac{1}{2}|M^2-M'^2|</math>
The perturbation factor is given by:
Line 288 ⟶ 286:
</math>
==References==
[[de:Gestörte_Gamma-Gamma-Winkelkorrelation]]▼
{{Reflist}}
|