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Nuclear Spectroscopy

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E X P E R I M E N T 1<br />

Energy Calibration<br />

INTRODUCTION<br />

When a gamma ray (that is emitted during a change<br />

in an atom’s nucleus) interacts with your sodium<br />

iodide crystal, NaI(Tl), the gamma will frequently<br />

give all its energy to an atomic electron via the photoelectric<br />

effect (photoeffect). This electron travels a<br />

short, erratic path in the crystal, converting its energy<br />

into photons of light by colliding with many atoms in<br />

the crystal. The more energy the gamma ray has, the<br />

more photons of light that are created.<br />

The photomultiplier tube (PMT) converts each photon<br />

into a small current, and since the photons arrive<br />

at the PMT at about the same time, the individual<br />

currents combine to produce a larger current pulse.<br />

This pulse is converted into a voltage pulse whose size<br />

is in proportion to the gamma ray’s energy.<br />

The voltage pulse is amplified and measured by an<br />

Analog to Digital Conversion (ADC) process. The<br />

result of this measurement is an integer between 0<br />

and 1023 for a 10-bit ADC. Zero is the measure for a<br />

voltage pulse less than a hundredth of a volt, and<br />

1023 is the measure for a pulse larger than about 8<br />

volts (or the largest voltage pulse accepted by your<br />

ADC). Pulses between 0 V and 8 V are proportionately<br />

given an integer measure between 0 and 1023.<br />

This measure is called the channel number. The<br />

analog to digital conversion process is performed by<br />

your interface board. Your computer records and<br />

displays these measurements as the number of gamma<br />

rays observed for each integer measure, or channel<br />

number. Your screen displays the number of gamma<br />

rays as a function of the channel number.<br />

Calibration with sources of known energies allows<br />

you to correlate the channel number with the gamma<br />

energy. The result is a graph of the gamma frequency<br />

(counts) as a function of gamma-ray energy (channel<br />

number). Figure 1.1 is a calibrated spectrum. The<br />

photopeaks are marked; other structures in the data<br />

will be discussed in later experiments.<br />

511<br />

1274<br />

Sum<br />

Figure 1.1 Gamma Spectrum of 22 Na source with a 3.8 cm x 2.5 cm NaI(Tl) scintillation detector.<br />

7

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