168-171 - Nuclear Radiation and Gamma Absorption (CP15)

168-171 - Nuclear Radiation and Gamma Absorption (CP15)

The thread running through this lesson is measurement: a detector counts radiation from the source and from the room around it, so good physics means separating the wanted signal from background, understanding what α\alpha, β\beta and γ\gamma can do in matter, and using lead-absorber data carefully. Radioactive decay laws and isotope half-life calculations belong to the next lesson; here, half-thickness means the thickness of lead that halves a γ\gamma count rate.

Background Counts

Put a Geiger-Muller tube on a bench, connect it to a counter, and leave the radioactive source in its store. The counter still clicks. That is not a broken detector: it is detecting background radiation.

Background radiation

Ionising radiation present in the surroundings from natural and artificial sources, detected whether or not a laboratory source is present.

Background radiation is ionising radiation already present in the surroundings. In a UK classroom it can come from natural sources such as radon from rocks and soil, γ\gamma radiation from the ground and building materials, cosmic radiation from space, and small amounts of radionuclides in food and drink. Artificial sources, especially diagnostic medical exposure, also contribute to population exposure, but the key laboratory point is simpler: the detector counts background whether or not your intended source is present.

A count is the number of detections in a time interval. A count rate is:

count rate=counttime\text{count rate} = \frac{\text{count}}{\text{time}}

The unit is count s−1\mathrm{count\,s^{-1}} or s−1\mathrm{s^{-1}}. In school radiation experiments, the useful source signal is usually the corrected count rate:

Corrected count rate

corrected count rate=measured count rate−background count rate \text{corrected count rate} = \text{measured count rate} - \text{background count rate}

Count rate = count ÷ counting time (s−1\mathrm{s^{-1}}). Subtract rates, not raw counts taken over different times.

Decision point: subtract rates, not raw counts measured over different times. If the background was counted for 300 s300\,\mathrm{s} and the source reading for 60 s60\,\mathrm{s}, the raw counts are not directly comparable until each is converted to a count rate.

Worked example:

The background count is 150150 counts in 300 s300\,\mathrm{s}.

background count rate=150300=0.50 count s−1\text{background count rate} = \frac{150}{300} = 0.50\,\mathrm{count\,s^{-1}}

With a γ\gamma source present, the detector records 18601860 counts in 60 s60\,\mathrm{s}.

measured count rate=186060=31.0 count s−1\text{measured count rate} = \frac{1860}{60} = 31.0\,\mathrm{count\,s^{-1}}

So:

corrected count rate=31.0−0.50=30.5 count s−1\text{corrected count rate} = 31.0 - 0.50 = 30.5\,\mathrm{count\,s^{-1}}

For Edexcel, a “calculate” answer should show the conversion to rates, the subtraction and the unit. A common wrong route is to subtract 150150 from 18601860 first; that mixes a five-minute count with a one-minute count and over-corrects the source reading.

Alpha, Beta And Gamma

Alpha, β\beta and γ\gamma are all ionising radiations, but they interact with matter in different ways.

RadiationNatureTypical chargeIonising abilityPenetration and range
α\alphahelium nucleus, 22 protons and 22 neutrons+2e+2ehighstopped by paper or skin; range of only a few cm in air
β\beta-minusfast electron emitted from the nucleus−e-emediumtypically travels up to metres in air; passes through paper, but is stopped by a few mm of aluminium or plastic
γ\gammahigh-energy electromagnetic photon from the nucleus00low per unit pathtravels long distances in air; reduced by thick lead or concrete, with no single sharp maximum range

The useful physical contrast is not "dangerous" against "safe". It is how often the radiation interacts while it travels. Alpha particles are massive and charged, so they interact strongly with nearby atoms. They cause many ionisations in a short distance, lose energy quickly, and therefore have low penetration. Gamma photons have no charge and no rest mass, so each photon has a lower chance of interacting over a small distance. That makes γ\gamma radiation weakly ionising per unit path but highly penetrating.

This contrast explains why α\alpha radiation can be serious if an α\alpha-emitting material is inside the body, even though α\alpha particles are easily stopped outside the body. It also explains why lead is used in the core practical: lead does not make γ\gamma radiation vanish at one magic thickness, but each extra thickness gives more chance for photons to interact and be removed from the beam.

Misconception contrast: more penetrating does not mean more strongly ionising. Here, γ\gamma is the most penetrating of the three but the least ionising per unit path; α\alpha is the least penetrating but the most ionising.

The more strongly a radiation ionises, the faster it loses energy and the less it penetrates: α\alpha (stopped by paper) > β\beta (stopped by a few mm of aluminium) > γ\gamma (reduced gradually by lead).

For an “explain” response, Edexcel credit usually depends on linked reasoning. "Gamma is penetrating" is a statement. "Gamma has no charge, so it is less likely to interact with atoms over a short distance and can pass through more material" is an explanation.

Nuclear Equations

Nuclear equations track two conserved counts:

ZAX{}^{A}_{Z}\mathrm{X}

AA is the nucleon number, the total number of protons and neutrons. ZZ is the proton number, the number of protons. In a nuclear equation, the total AA values must balance and the total ZZ values must balance.

Useful particle symbols are:

Particle/radiationSymbol in equationsMeaning for AA and ZZ
α\alpha particleX24X2224He\ce{^{4}_{2}He} or X24X2224α\ce{^{4}_{2}\alpha}A=4A = 4, Z=2Z = 2
β\beta-minus particleX−10X2−120e\ce{^{0}_{-1}e} or X−10X2−120β\ce{^{0}_{-1}\beta}A=0A = 0, Z=−1Z = -1
γ\gamma radiationX00X2020γ\ce{^{0}_{0}\gamma}A=0A = 0, Z=0Z = 0

Worked example 1: α\alpha emission.

92238U→90234Th+24He{}^{238}_{92}\mathrm{U} \rightarrow {}^{234}_{90}\mathrm{Th} + {}^{4}_{2}\mathrm{He}

Check the nucleon numbers:

238=234+4238 = 234 + 4

Check the proton numbers:

92=90+292 = 90 + 2

Worked example 2: β\beta-minus emission.

614C→714N+−10e+00νˉe{}^{14}_{6}\mathrm{C} \rightarrow {}^{14}_{7}\mathrm{N} + {}^{0}_{-1}\mathrm{e} + {}^{0}_{0}\bar\nu_e

The nucleon number stays 1414. The proton number of the nucleus increases from 66 to 77, because the emitted electron has charge number −1-1 and the totals must still balance:

6=7+(−1)6 = 7 + (-1)

Gamma emission is different in this bookkeeping. It carries energy away from the nucleus but has A=0A = 0 and Z=0Z = 0, so it does not change the element:

4399mTc→4399Tc+00γ{}^{99m}_{43}\mathrm{Tc} \rightarrow {}^{99}_{43}\mathrm{Tc} + {}^{0}_{0}\gamma

The superscript mm just signals an excited nuclear state in this example; the key skill is that γ\gamma does not change AA or ZZ.

Decision point: do not balance nuclear equations by chemical valency. These are not electron-shell equations. Balance the top numbers and the bottom numbers.

In beta-minus decay a neutron changes into a proton, an electron and an electron antineutrino: n→p+e−+νˉen\rightarrow p+e^-+\bar\nu_e. The antineutrino has zero nucleon and charge numbers, so including it leaves the top and bottom number sums unchanged. The bottom number means proton number for a nucleus and charge in units of ee for an emitted particle; an electron does not contain minus one proton. When positron emission is specified, p→n+e++νep\rightarrow n+e^++\nu_e, so nuclear AA stays constant and ZZ decreases by one. Use the supplied particle symbols and include the neutrino where the full decay equation is requested.

Gamma Absorption Setup

Core Practical 15 investigates how lead reduces the count rate from a γ\gamma source. The apparatus needs a fixed geometry because count rate depends on more than the lead: it also depends on distance, alignment and detector position.

[DIAGRAM: asset_name: Gamma source, lead sheets, GM detector and counter at fixed distance with background and thickness controls; asset_slug: 049_background_radiation_gamma_absorption_core_practical__diagram_01; recommended_method: matplotlib; description: Gamma source, lead sheets, GM detector and counter at fixed distance with background and thickness controls.]
Diagram

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