PHY 1020 – Chapter 4: Nuclei and Radioactivity

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34 question-and-answer flashcards summarizing key concepts, definitions, and quantitative facts from Chapter 4: Nuclei and Radioactivity.

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34 Terms

1
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What causes the sensation we identify as heat?

The molecular and atomic movement and vibrations of matter.

2
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At what temperature (in Kelvin) does all molecular motion theoretically stop?

0 K, absolute zero.

3
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Which three sub-atomic particles make up all atoms?

Protons, neutrons, and electrons.

4
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What uniquely defines an element on the periodic table?

The number of protons in its nucleus.

5
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What is an isotope?

Atoms of the same element that contain different numbers of neutrons.

6
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Name the three common isotopes of hydrogen.

¹H (protium), ²H (deuterium), and ³H (tritium).

7
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Why are many isotopes radioactive?

Because their nuclei are unstable and decay to reach a more stable configuration.

8
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What is nuclear fusion?

The process of two light nuclei combining to form a heavier nucleus, releasing energy.

9
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Where does natural fusion occur on a large scale?

In stars, including our Sun.

10
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Why isn’t Jupiter a fusion reactor like the Sun?

It is not massive enough to reach the pressures and temperatures required for sustained fusion.

11
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Describe alpha decay.

An unstable nucleus emits an alpha particle (2 protons and 2 neutrons), becoming a lighter element.

12
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What particle is emitted during beta-minus decay?

An electron (and an antineutrino), produced when a neutron converts into a proton.

13
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What particle is emitted during beta-plus decay?

A positron (and a neutrino), produced when a proton converts into a neutron.

14
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What are gamma rays?

High-energy photons (electromagnetic radiation) often emitted alongside alpha or beta decay.

15
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Why are gamma rays more dangerous to humans than alpha particles?

They have no mass or charge, allowing them to penetrate deeply and damage internal organs.

16
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What is cosmic radiation?

High-energy charged particles (mostly protons and electrons) from the Sun and other stars that continuously strike Earth.

17
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How long do free neutrons produced in nuclear reactions typically survive?

About 15 minutes before beta-decaying into a proton and electron.

18
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Rank alpha, beta, gamma, and neutron radiation by typical penetration, from least to greatest.

Alpha < Beta < Neutron < Gamma.

19
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What unit equals 0.01 Sievert of radiation dose?

1 rem (or 1000 mrem).

20
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What is the recommended maximum annual radiation exposure for the general public?

5000 mrem or 0.05 Sv (50 mSv).

21
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Approximately how much radiation does an average person receive yearly from natural sources?

About 300 mrem (3 mSv).

22
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Around what acute dose (in rem) can radiation poisoning begin in humans?

About 100 rem (1 Sv).

23
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State the linear hypothesis for radiation-induced cancer.

Cancer risk increases linearly with dose; e.g., 2.5 rem yields an extra 1-in-1000 chance.

24
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How many of the 134 emergency workers at Chernobyl died from acute radiation sickness?

28 workers.

25
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What discrepancy was observed between predicted and actual cancer rates after Hiroshima?

Predicted ~0.8 % extra cancers versus ~2 % observed, suggesting incomplete understanding of radiation effects.

26
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Why does Denver challenge simple radiation-risk models?

Despite higher background radiation (~0.1 rem more per year), Denver’s cancer rate is lower than the U.S. average.

27
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Define half-life.

The time required for half of a radioactive sample to decay.

28
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After two half-lives, what fraction of the original radioactive material remains?

One-quarter (25 %).

29
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What is nuclear fission?

The splitting of a heavy nucleus into two lighter nuclei, releasing energy and neutrons.

30
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What isotope powers most Radioisotope Thermoelectric Generators (RTGs)?

Plutonium-238.

31
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How does a household smoke detector use radioactivity?

An alpha emitter ionizes air; smoke disrupts the ionization, triggering the alarm.

32
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What is the half-life of carbon-14 used in radiocarbon dating?

5730 years.

33
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Why is radiocarbon dating limited to objects younger than about 60,000 years?

After ~10 half-lives, too little ¹⁴C remains to measure accurately.

34
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Which radioactive isotope is used for dating very old rocks via its decay to ⁴⁰Ca and ⁴⁰Ar?

Potassium-40, with a half-life of 1.248 × 10⁹ years.