Radioactive decay and stability

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Knowledge and terms for radioactive decay spec 3.8.1.3 AQA A-level physics.

18 Terms

1

What does the inverse-square law demonstrate?

Radiation spreads out uniformly as a sphere. When an EM wave spreads out, the area over which it spreads is (inversely) proportional to the radius squared.

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2

What is λ?

The decay constant, the probability of a nucleus decaying per unit time.

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3

Definition of the half-life?

The time taken for the number of particles/activity in a source to halve.

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4

How to determine half-life from a nuclei-time graph?

Measure time taken for sample size to halve. Do this across several half-lives and find a mean.

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5

How to determine half-life no with nuclei-time graph?

Plot ln (N) against time. This forms a straight line. Modulus of the gradient is the decay constant. Substitute into half-life formula.

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6

When can the decay constant be used to model the decay of nuclei? Why?

When there is a large number of nuclei in the sample, because the decay constant models the number of nuclei statistically; decay is a random process.

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7

Applications of nuclei with short half-life.

Radioactive tracers in medical diagnosis. Needs to be long enough for tests, but short enough to reduce exposure to the healthy tissue of a patient.

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8

Applications of nuclei with long half-life.

Dating of objects; carbon-dating for organic objects. Achieved by measuring the current amount of carbon-14 and comparing it to the initial amount, the percentage of which is approximately equal in all living things.

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9

Prove the modulus of the gradient of a ln(N0) - time graph is the decay constant.

??

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10

What is I in the inverse square law?

Intensity of the gamma radiation, Wm-2

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11

What is k in the inverse square law?

Constant of proportionality.

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12

What is x in the inverse square law?

distance from the source, m

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13

Equation for radiation at two different points.

knowt flashcard image
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14

What makes some nuclei unstable?

The larger nuclei are more unstable. Attractive range of strong nuclear force is 0.5fm-3fm so for nuclei large than this, the electrostatic force of repulsion is greater than the strong nuclear force holding nucleons together.

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15

What type of radiation uses inverse square law?

only gamma radiation

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16

What is electron capture? And equation?

when an atomic electron is absorbed by a proton on the nucleus. A neutron and electron neutrino are released. Mediated by the W+ boson.

p + e- = n + ve

<p>when an atomic electron is absorbed by a proton on the nucleus. A neutron and electron neutrino are released. Mediated by the W+ boson. </p><p>p + e<sup>-</sup> = n + v<sub>e</sub></p>
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17

What is electron-proton collision (decay)? And equation?

when an electron collides with a proton, a neutron and an electron neutrino are emitted. Mediated by the W- boson.

p + e- —> n + ve

<p>when an electron collides with a proton, a neutron and an electron neutrino are emitted. Mediated by the W- boson.</p><p>p + e<sup>-</sup> —&gt; n + v<sub>e</sub></p>
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18

A (large) nucleus has more neutrons than protons. Explain why there is an imbalance of proton and neutrons numbers.

  • Strong nuclear force (SNF) affects nucleons or protons and neutrons.

  • SNF attraction extends up to 3 fm (allow 1–4 fm)

  • The SNF is repulsive below about 0.8 fm (allow 0.3 to 1 fm and prevents the nucleus totally collapsing)

  • Electromagnetic/electrostatic repulsive force (only) acts between protons

  • EM forces are long range/infinite/acts across whole nucleus/acts on all protons(so increases as proton number increases)

  • More neutrons are needed to hold nucleus together/add to binding force/increase instability/reduce stability

  • Fewer protons are required so as to reduce the repulsion/reduce instability/increase stability

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