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[[Category:English]]
[[Category:Nuclear Physics]]

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= Introduction =

'''Nuclear physics''' studies atomic nuclei: how protons and neutrons are arranged, how nuclei change, why some nuclei are stable, and how nuclear reactions release or absorb energy. In this aiMOOC for Grades 11–13, you will connect experimental evidence, mathematical models, nuclear equations, energy calculations, radiation physics, and real-world applications.

By the end of the course, you should be able to use nuclide notation, explain nuclear stability, calculate mass defect and binding energy, model radioactive decay and half-life, balance nuclear equations, compare fission and fusion, interpret radiation data, and evaluate applications and risks using scientific evidence.

[[File:Rutherford Scattering.svg|500px|frameless|center]]

The Rutherford scattering experiment is a useful starting point because it showed that most of an atom is empty space and that nearly all positive charge and mass are concentrated in a tiny nucleus. Modern nuclear physics extends this picture by studying the forces, energy levels, transformations, and reactions of nuclei.

{{#ev:youtube|https://www.youtube.com/watch?v=lUhJL7o6_cA|500|center}}

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= The Atomic Nucleus =

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== Protons, Neutrons, and Nuclides ==

A nucleus contains '''protons''' and '''neutrons''', collectively called [[English:Nucleon|nucleons]]. The proton number or atomic number <math>Z</math> determines the chemical element. The neutron number is <math>N</math>, and the mass number is <math>A=Z+N</math>.

A nuclide is commonly written as <math>^{A}_{Z}X</math>, where <math>X</math> is the element symbol. For example, <math>^{14}_{6}\mathrm{C}</math> has six protons and eight neutrons. [[English:Isotope|Isotopes]] are nuclides of the same element with the same proton number but different neutron numbers.

The nucleus is extremely small compared with the entire atom. A useful empirical estimate for nuclear radius is <math>R \approx r_0 A^{1/3}</math>, with <math>r_0</math> about <math>1.2</math> femtometres. This scaling suggests that nuclear matter has approximately constant density over a wide range of nuclei.

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== Rutherford Scattering and Evidence ==

In the [[English:Geiger–Marsden experiment|Geiger–Marsden experiment]], alpha particles were directed at thin metal foil. Most passed through with little deflection, while a small fraction were scattered through large angles. The observations were inconsistent with a diffuse positive charge and supported a compact, positively charged nucleus.

When you interpret scattering, distinguish '''observation''' from '''model'''. The detector records particle directions and rates; the nuclear model is an explanation constructed from those measurements.

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= Nuclear Forces and Stability =

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== Strong Interaction and Electrostatic Repulsion ==

Protons repel one another through the electromagnetic interaction. At very short nuclear distances, an effective attractive nuclear interaction between nucleons can overcome this repulsion. In modern particle physics, the underlying strong interaction is described by quantum chromodynamics, while nuclear models often use an effective residual strong force between protons and neutrons.

Stable nuclei reflect a balance among several effects. Light stable nuclei often have similar numbers of protons and neutrons. Heavier stable nuclei generally require proportionally more neutrons because proton-proton electrostatic repulsion becomes more important as proton number increases.

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== Nuclear Energy Levels and Shell Ideas ==

Like electrons in atoms, nucleons occupy quantized states. The [[English:Nuclear shell model|Nuclear shell model]] explains important patterns in nuclear structure and helps account for unusually stable configurations associated with certain proton or neutron numbers. At Grades 11–13 level, the key idea is that nuclear stability is not determined by one simple rule: binding, proton-neutron ratio, shell structure, and available decay pathways all matter.

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= Mass Defect and Binding Energy =

The mass of a bound nucleus is less than the total mass of its separated protons and neutrons. This difference is the '''mass defect'''. The corresponding energy is the '''binding energy''':

<math>E_b = \Delta m c^2</math>

If mass is expressed in atomic mass units, the conversion <math>1\,\mathrm{u}\,c^2 \approx 931.5\,\mathrm{MeV}</math> is useful. Binding energy per nucleon, <math>E_b/A</math>, is especially helpful when comparing nuclear stability.

[[File:Binding energy curve of common isotopes.svg|600px|frameless|center]]

The binding-energy-per-nucleon curve rises steeply for light nuclei, reaches a broad maximum in the iron-nickel region, and then decreases gradually for very heavy nuclei. This explains why both '''fusion of light nuclei''' and '''fission of very heavy nuclei''' can release energy: the products can be more tightly bound per nucleon.

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== Worked Reasoning Pattern ==

When solving a binding-energy problem, identify the required masses, compute the mass defect, convert mass difference to energy, and only then divide by the number of nucleons if the question asks for binding energy per nucleon. Keep enough significant figures during intermediate calculations.

A high binding energy per nucleon usually indicates strong binding, but it does not by itself tell you the complete decay behavior of a nuclide. Decay also depends on which transformations are energetically allowed and on quantum-mechanical probabilities.

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= Radioactivity =

Radioactive decay is a spontaneous nuclear transformation. For a large collection of identical unstable nuclei, individual decay times are unpredictable, but the statistical behavior of the whole sample is highly regular.

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== Alpha Decay ==

In [[English:Alpha decay|Alpha decay]], a nucleus emits an alpha particle, which is a helium-4 nucleus with two protons and two neutrons. The parent mass number decreases by four and the atomic number decreases by two.

[[File:Alpha Decay.svg|450px|frameless|center]]

A general form is <math>^{A}_{Z}X \rightarrow ^{A-4}_{Z-2}Y + ^4_2\mathrm{He}</math>. Alpha decay is common among very heavy nuclei.

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== Beta Decay ==

In '''beta-minus decay''', a neutron in the nucleus transforms into a proton while an electron and an electron antineutrino are emitted. The mass number stays the same while the atomic number increases by one.

[[File:Beta-minus Decay.svg|450px|frameless|center]]

A simplified nuclear-level equation is <math>n \rightarrow p + e^- + \bar{\nu}_e</math>. The antineutrino is essential for conserving energy, momentum, and lepton number.

In '''beta-plus decay''', a proton transforms into a neutron while a positron and an electron neutrino are emitted. Electron capture is another process that can reduce the proton number by one.

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== Gamma Decay ==

In [[English:Gamma decay|Gamma decay]], an excited nucleus emits a high-energy photon and moves to a lower-energy nuclear state. The proton number and mass number do not change.

[[File:Gamma Decay.svg|450px|frameless|center]]

Gamma emission often follows alpha or beta decay because the daughter nucleus may initially be left in an excited state.

{{#ev:youtube|https://www.youtube.com/watch?v=P_SD5Rt6XMk|500|center}}

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= Decay Law, Activity, and Half-Life =

For a large number of identical radioactive nuclei,

<math>N(t)=N_0 e^{-\lambda t}</math>

where <math>N_0</math> is the initial number of undecayed nuclei and <math>\lambda</math> is the decay constant. The activity is

<math>\mathcal{A}=\lambda N</math>

and is measured in [[English:Becquerel|becquerels]], where one becquerel means one decay per second. The half-life is

<math>T_{1/2}=\frac{\ln 2}{\lambda}</math>.

[[File:Activity decay.svg|600px|frameless|center]]

After one half-life, half the original unstable nuclei remain on average; after two half-lives, one quarter remain; after three, one eighth remain. This exponential behavior is different from a linear decrease.

{{#ev:youtube|https://www.youtube.com/watch?v=IDkNlU7zKYU|500|center}}

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== Interpreting Decay Data ==

A measured count rate may include background radiation, so experimental analysis often requires subtracting an independently measured background count rate. Because nuclear decay is random, repeated counts fluctuate. Longer counting times generally reduce the relative statistical uncertainty.

A straight-line plot can also be obtained by plotting <math>\ln N</math> or <math>\ln \mathcal{A}</math> against time. The gradient is <math>-\lambda</math>, which allows the half-life to be calculated.

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= Ionizing Radiation and Matter =

Ionizing radiation has enough energy to remove electrons from atoms or molecules. Alpha particles are strongly ionizing and have short ranges in matter. Beta particles are more penetrating than alpha particles. Gamma rays are uncharged photons and are usually more penetrating. Neutrons are uncharged and interact mainly through nuclear collisions and reactions.

The effect of radiation depends on energy, type, exposure geometry, material, and biological context. Do not equate '''activity''' with '''dose''': activity describes nuclear transformations in a source, while dose describes energy deposited in matter and, for protection quantities, the biological weighting of that exposure.

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== Radiation Quantities and Protection ==

'''Absorbed dose''' is energy deposited per unit mass and is measured in grays. '''Equivalent dose''' and '''effective dose''' use sieverts and include weighting factors used in radiation protection.

General protection principles include reducing unnecessary exposure time, increasing distance from suitable external sources, and using appropriate shielding. Shielding depends on radiation type: dense materials can attenuate gamma radiation, low-atomic-number materials are often preferred for high-energy beta radiation to limit bremsstrahlung, and hydrogen-rich materials are useful for slowing many neutrons. Any work with real radioactive sources must follow local regulations and trained supervision.

[[File:Omega West Reactor Core showing Cherenkov Radiation.jpg|500px|frameless|center]]

The blue glow shown in some reactor pools is [[English:Cherenkov radiation|Cherenkov radiation]], produced when charged particles travel through a transparent medium faster than light can propagate through that medium. This does not mean that anything travels faster than the speed of light in vacuum.

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= Nuclear Fission =

[[English:Nuclear fission|Nuclear fission]] occurs when a heavy nucleus splits into lighter fragments, typically releasing neutrons and energy. A common example is neutron-induced fission of uranium-235. Energy appears mainly as kinetic energy of the fission fragments, with additional energy carried by neutrons and radiation.

[[File:Nuclear fission.svg|450px|frameless|center]]

If emitted neutrons cause further fissions, a '''chain reaction''' can develop.

[[File:Fission chain reaction.svg|450px|frameless|center]]

In a power reactor, the chain reaction is kept controlled. Reactor systems are designed to manage neutron behavior and remove heat safely. Depending on reactor design, components may include fuel, a moderator, control elements, coolant, shielding, and containment. The exact engineering differs among reactor types.

{{#ev:youtube|https://www.youtube.com/watch?v=D91T-B-PVE0|500|center}}

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== Energy and Reactor Reasoning ==

A single fission event releases energy on the order of hundreds of megaelectronvolts. The macroscopic energy available from nuclear fuel is large because enormous numbers of nuclei participate.

When comparing nuclear energy technologies, separate physical quantities from policy judgments. Useful evidence includes energy density, operational emissions, construction and decommissioning, waste management, accident risk, resource use, economics, proliferation concerns, and the reliability requirements of an electricity system.

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= Nuclear Fusion =

[[English:Nuclear fusion|Nuclear fusion]] combines light nuclei into heavier nuclei. A widely studied reaction is

<math>^2_1\mathrm{H}+^3_1\mathrm{H}\rightarrow ^4_2\mathrm{He}+^1_0n+17.6\,\mathrm{MeV}</math>.

[[File:Nuclear fusion illustration.svg|600px|frameless|center]]

Fusion can release energy because the products have greater binding energy per nucleon than the initial light nuclei. Positively charged nuclei repel each other, so fusion requires conditions that make close collisions sufficiently likely. In stars, gravity provides confinement and high temperature; laboratory research investigates magnetic and inertial confinement approaches.

{{#ev:youtube|https://www.youtube.com/watch?v=204l3wqs6OY|500|center}}

{{#ev:youtube|https://www.youtube.com/watch?v=X1SffRGMBEU|500|center}}

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= Applications of Nuclear Physics =

Nuclear physics supports medicine, energy, industry, archaeology, environmental science, astrophysics, and materials research.

In [[English:Nuclear medicine|Nuclear medicine]], radioactive tracers can reveal physiological processes. Positron emission tomography uses positron-emitting radionuclides; positron-electron annihilation produces pairs of gamma photons that can be detected to reconstruct images.

[[File:PET-MIPS-anim.gif|400px|frameless|center]]

Radiotherapy uses ionizing radiation to damage cancer cells while treatment planning aims to limit dose to healthy tissue. Industrial applications include thickness measurement, non-destructive testing, process monitoring, and tracer studies. In archaeology and Earth science, radiometric dating uses known decay behavior to estimate ages under appropriate assumptions.

Nuclear astrophysics explains how nuclear reactions power stars and how nucleosynthesis produces chemical elements. Heavy-element production involves environments such as stellar explosions and neutron-star mergers.

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= Scientific Evidence, Uncertainty, and Responsible Use =

Nuclear physics combines models with measurements. Good scientific reasoning means stating assumptions, using units consistently, estimating uncertainty, checking whether results are physically plausible, and distinguishing measured data from interpretation.

Radiation topics can be emotionally and politically charged. Evaluate claims by asking what quantity was measured, which units were used, what comparison is being made, what uncertainty is reported, and whether the source is scientifically credible.

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= Reliable Background Sources =

For further reading, consult [https://www.energy.gov/science/doe-explainsnuclei DOE Explains: Nuclei], [https://www.energy.gov/science/doe-explainsthe-strong-force DOE Explains: The Strong Force], [https://www.nrc.gov/about-nrc/radiation/health-effects/radiation-basics U.S. Nuclear Regulatory Commission: Radiation Basics], and [https://www.iaea.org/topics/radiation-protection International Atomic Energy Agency: Radiation Protection].

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= Interactive Tasks =

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== Quiz: Test Your Knowledge ==

{{MC}}

'''Which quantity identifies the chemical element of a nucleus?'''
(Proton number)
(!Neutron number)
(!Mass defect)
(!Half life)

{{E}}
<br>

{{MC}}

'''What happens to the mass number in alpha decay?'''
(It decreases by four)
(!It increases by four)
(!It stays unchanged)
(!It decreases by one)

{{E}}
<br>

{{MC}}

'''What is emitted in gamma decay?'''
(A photon)
(!A proton)
(!A helium nucleus)
(!A neutron only)

{{E}}
<br>

{{MC}}

'''What does binding energy represent?'''
(Energy needed to separate a nucleus)
(!Energy of atomic electrons only)
(!Energy stored in chemical bonds)
(!Energy required to ionize one atom)

{{E}}
<br>

{{MC}}

'''Which law describes the number of undecayed nuclei over time?'''
(Exponential decay)
(!Linear growth)
(!Constant increase)
(!Quadratic decay)

{{E}}
<br>

{{MC}}

'''What is the unit of activity?'''
(Becquerel)
(!Gray)
(!Sievert)
(!Tesla)

{{E}}
<br>

{{MC}}

'''Why can fission of very heavy nuclei release energy?'''
(Products can be more tightly bound)
(!Electrons become heavier)
(!Charge is not conserved)
(!Neutrons disappear completely)

{{E}}
<br>

{{MC}}

'''Which process powers ordinary stars for most of their lifetimes?'''
(Nuclear fusion)
(!Nuclear fission)
(!Chemical combustion)
(!Radioactive shielding)

{{E}}
<br>

{{MC}}

'''What happens to atomic number in beta minus decay?'''
(It increases by one)
(!It decreases by one)
(!It decreases by two)
(!It remains unchanged)

{{E}}
<br>

{{MC}}

'''Which statement best describes radioactive decay?'''
(Individual decays are random)
(!Every nucleus decays at a fixed age)
(!Activity always decreases linearly)
(!Half life depends on sample size)

{{E}}
<br>

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== Memory Game ==

<div class="memo-quiz">
{|
|-
| Nuclide || A specific nucleus defined by proton number and neutron number
|-
| Isotope || A member of one element with a particular neutron number
|-
| Nucleon || A proton or neutron inside a nucleus
|-
| Activity || The rate of nuclear decays in a radioactive sample
|-
| Fission || Splitting of a heavy nucleus into lighter fragments
|-
| Fusion || Combining light nuclei into a heavier nucleus
|-
| Becquerel || The unit equal to one nuclear decay per second
|-
| Sievert || A unit used for radiation protection dose quantities
|}
{{E}}
<br>

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== Drag and Drop ==

<div class="lueckentext-quiz">

{| class="wikitable"
! Match the correct terms.
! Topic
|-
| '''Alpha emission'''
| Mass number falls by four and atomic number by two
|-
| '''Beta minus emission'''
| A neutron changes into a proton with an electron and antineutrino emitted
|-
| '''Gamma emission'''
| An excited nucleus releases a high energy photon
|-
| '''Nuclear fission'''
| A heavy nucleus separates into lighter nuclear fragments
|-
| '''Nuclear fusion'''
| Light nuclei combine to form a heavier nucleus
|}
{{E}}

<br>
Match every process with the description that best preserves the relevant conservation laws.
<br />

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== Crossword Puzzle ==

<div class="kreuzwort-quiz">
{|
|-
| Isotope || What name is given to a nuclide of the same element with a different neutron number?
|-
| Nucleon || What single word describes either a proton or a neutron in a nucleus?
|-
| Fission || What process splits a heavy nucleus into lighter nuclear fragments?
|-
| Fusion || What process combines light nuclei into a heavier nucleus?
|-
| Activity || What quantity measures the rate of radioactive decays?
|-
| Neutrino || What neutral lepton is emitted in beta decay?
|}
{{E}}
<br>

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== LearningApps ==

<iframe> https://learningapps.org/index.php?s=Nuclear+Physics </iframe>

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== Cloze Text ==

<quiz display=simple>
{'''Complete the text.'''<br>
|type="{}"}
A nucleus is made of protons and { neutrons }. The total number of nucleons is the { mass number }. Isotopes have the same proton number but different { neutron numbers }. The energy required to separate a nucleus is its { binding energy }. Radioactive decay follows an { exponential } law for a large sample. The time for half of the original unstable nuclei to remain is the { half-life }. Alpha decay emits a { helium nucleus }. Beta-minus decay emits an electron and an electron { antineutrino }. Heavy nuclei can release energy through { fission }. Light nuclei can release energy through { fusion }.
</quiz>

<br>

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= Open-Ended Tasks =

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=== Easy ===
# [[English:Nuclear notation card set|Nuclear notation card set]]: Create a one-page visual guide that explains proton number, neutron number, mass number, isotope notation, and two worked examples.
# [[English:Decay dice model|Decay dice model]]: Use dice or a digital random-number tool to model radioactive decay, graph the number of undecayed objects after each round, and explain why the curve is approximately exponential.
# [[English:Radiation comparison poster|Radiation comparison poster]]: Design an image that compares alpha, beta, gamma, and neutron radiation by charge, ionizing behavior, penetration, and typical shielding.
# [[English:Nuclear physics explainer video|Nuclear physics explainer video]]: Produce a two-minute video that explains one key idea from this course using your own diagram and one numerical example.

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=== Standard ===
# [[English:Half-life data investigation|Half-life data investigation]]: Analyze a supplied or simulated count-rate dataset, subtract background where appropriate, estimate the half-life, and discuss statistical fluctuations.
# [[English:Binding energy spreadsheet|Binding energy spreadsheet]]: Calculate binding energy per nucleon for several selected nuclides using published mass data, graph the results, and interpret the trend.
# [[English:Nuclear medicine interview|Nuclear medicine interview]]: Interview a qualified medical professional or use an approved recorded interview to investigate how nuclear physics is used in diagnosis or treatment, then summarize the physics and safety controls.
# [[English:Science museum or virtual laboratory visit|Science museum or virtual laboratory visit]]: Visit a science museum, university outreach laboratory, reactor information centre, or virtual research facility and document three examples of nuclear physics in practice.

{{BR}}
=== Advanced ===
# [[English:Decay curve model comparison|Decay curve model comparison]]: Fit exponential and linear models to the same radioactive-decay dataset, compare residuals, and justify which model is physically appropriate.
# [[English:Fission and fusion evidence brief|Fission and fusion evidence brief]]: Produce an evidence-based briefing that compares fission and fusion in terms of nuclear reactions, binding energy, engineering challenges, waste, safety, and present technological maturity.
# [[English:Radiation risk communication study|Radiation risk communication study]]: Compare how three credible institutions communicate radiation quantities and risk, identify possible sources of misunderstanding, and redesign one explanation for a school audience.
# [[English:Nuclear astrophysics research project|Nuclear astrophysics research project]]: Create a research poster or narrated presentation explaining how nuclear reactions build elements in stars and explosive astrophysical events, including a clear chain from nuclear process to observational evidence.

{{:Open Task - Create a MOOC}}

{{BR}}
= Learning Assessment =

# [[English:Conservation in nuclear equations|Conservation in nuclear equations]]: Complete and justify a set of unfamiliar nuclear equations by applying conservation of nucleon number, charge, energy, and relevant emitted particles.
# [[English:Binding energy transfer problem|Binding energy transfer problem]]: Use mass data for an unfamiliar reaction to determine whether energy is released or absorbed and explain the result using the binding-energy curve.
# [[English:Half-life inference|Half-life inference]]: Interpret noisy count-rate measurements, account for background radiation, estimate a half-life, and state the main sources of uncertainty.
# [[English:Radiation protection scenario|Radiation protection scenario]]: Compare two realistic exposure scenarios and recommend proportionate protection measures using radiation type, distance, shielding, and exposure time.
# [[English:Fission fusion comparison|Fission fusion comparison]]: Explain why both fission and fusion can release energy even though one splits nuclei and the other combines them.
# [[English:Evidence evaluation|Evidence evaluation]]: Critique a public claim about nuclear power, radiation, or nuclear medicine by checking units, evidence quality, uncertainty, and the distinction between physical data and value judgments.

<br>
<br>

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= Evidence of Learning =

'''Knowledge:''' You can explain nuclear structure, nuclide notation, nuclear forces, binding energy, radioactive decay, half-life, fission, fusion, radiation interactions, and major applications.

'''Skills:''' You can balance nuclear equations, calculate energy from mass defect, use exponential models, interpret graphs, work with units, estimate uncertainty, and distinguish activity from dose.

'''Products:''' Strong evidence may include a decay model, annotated diagrams, a binding-energy calculation, a data analysis, a scientific poster, a short video, an interview summary, or a research briefing.

'''Transfer:''' You can apply nuclear physics to unfamiliar contexts such as medical imaging, reactor questions, dating methods, radiation protection, astrophysics, and public claims about nuclear technology.

<br>
<br>

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= OERs on the Topic =

<iframe> https://en.m.wikipedia.org/wiki/Nuclear_physics </iframe>

<br>

{{BR}}
= Linked Learning Areas =

{| align=center
{{:D-Tab}}
'''[[English:Nuclear Physics|Nuclear Physics]]'''
# [[English:Atomic nucleus|Atomic nucleus]]
# [[English:Isotope|Isotope]]
# [[English:Radioactive decay|Radioactive decay]]
# [[English:Half-life|Half-life]]
# [[English:Binding energy|Binding energy]]
# [[English:Nuclear fission|Nuclear fission]]
# [[English:Nuclear fusion|Nuclear fusion]]
# [[English:Nuclear medicine|Nuclear medicine]]
# [[English:Radiation protection|Radiation protection]]
# [[English:Nuclear astrophysics|Nuclear astrophysics]]
|}

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= aiMOOC Projects =
[[Category:English]]
[[Category:Nuclear Physics]]
[[Category:Physics]]
[[Category:Science]]
[[Category:STEM]]
[[Category:Grades 11-13]]
[[Category:Upper Secondary Education]]
[[Category:Radioactivity]]
[[Category:Nuclear Energy]]
[[Category:AI_MOOC]]
[[Category:GPT aiMOOC]]
{{MT}}

English:Nuclear Physics - Versionsgeschichte

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