Physics HL
Physics HL
5
Chapters
329
Notes
Theme A - Space, Time & Motion
Theme A - Space, Time & Motion
Theme B - The Particulate Nature Of Matter
Theme B - The Particulate Nature Of Matter
Theme C - Wave Behaviour
Theme C - Wave Behaviour
Theme D - Fields
Theme D - Fields
Theme E - Nuclear & Quantum Physics
Theme E - Nuclear & Quantum Physics
Unveiling Atoms: From Plücker's Discovery to Modern Models
Understanding Nuclear Notation: Dive Into Atomic Structure
The Groundbreaking Geiger-Marsden-Rutherford Gold Foil Experiment
Unlocking Nuclear Density: From Nucleons to Rutherford's Discoveries
Unveiling Sunlight's Mysteries: The Story Of Emission & Absorption Spectra
Unraveling The Atom: Bohr's Revolution Beyond Rutherford's Model
Unraveling the Bohr Model: Insights into Hydrogen's Energy Levels
Unlocking the Secrets: Bohr Model & Spectra Insights
The Ultraviolet Catastrophe: Planck’s Revolutionary Breakthrough
Unraveling Einstein's Explanation of The Photoelectric Effect
Unlocking Einstein's Photoelectric Equation Secrets
Unraveling the Mystery: Millikan's Photoelectric Experiment & Wave-Particle Duality
Unraveling Compton's Pioneering X-ray Experiments
Unveiling Photon-Matter Interactions: Beyond Compton & Photoelectric Effects
De Broglie Hypothesis: Matter Waves and Quantum Revelations
Unraveling The Davisson-Germer Experiment: Nobel-Prize Worthy Discoveries
Unveiling Radioactivity: Serendipity in Science's Evolution
Isotopes & Isotones: Understanding Chemical Properties
Understanding Radioactive Decay: From Parent To Daughter Nuclide
Unlocking Radioactive Decay: Alpha, Beta, Gamma Explained!
Understanding Alpha Decay: From Uranium-232 To Radon-222
Beta (β) Decay: Understanding Its 3 Types and Importance
Gamma-Photon Emission: Insights Into Cobalt-59 Decay
Discrete Nuclear Energy Levels: Understanding Gamma Emission
Continuous Beta Decay Spectra vs. Alpha Decay Energy
Ionizing Radiation Properties: Understanding Alpha, Beta & Gamma
Understanding The Strong Nuclear Force: Beyond Gravitational & Electromagnetic Interactions
Understanding Mass Defect & Nuclear Binding Energy
Understanding Nuclear Mass: From Atomic Units To Energy
Understanding Binding Energy Per Nucleon: Key To Nuclear Stability
Unraveling the Strong Nuclear Force: The Rutherford Revelation
Understanding Nuclear Stability: Insights from Binding Energy & Decay
Understanding Radioactive Half-Life: From Basics To Applications
Unlocking Radioactivity: Instruments & Intricacies Explained
Understanding Activity Vs. Count Rate In Radioactivity
Unlocking The Mysteries Of Background Radiation
Unlocking Time's Secrets: The Science Of Radioactive Dating
Unlocking The Power: Radioactive Nuclides In Medical Diagnosis & Therapy
Unlocking Industrial Uses Of Radioactive Materials
Understanding Radioactive Decay: The Fundamental Law & Implications
Understanding Decay Constant: The Nuance Of Nuclear Decay Probability
Decoding Half-Life: Dive Into Phosphorus-32 Decay Analysis
Unveiling The Secrets: Long Half-Lives & Thorium-232 Explained
Discovering Half-Life: Lab Methods & Radioactive Decay Analysis
Decay Chains & Radioactive Dating: From Uranium To Lead
Elise Meitner: The Unsung Pioneer Of Nuclear Fission
Nuclear Fission: Spontaneous Vs. Induced Processes
Unlocking Nuclear Energy: The Uranium-235 Fission Process
Chain Reactions: The Heart of Nuclear Energy Production
Unlocking Nuclear Secrets - The PWR Reactor Explained!
Understanding Neutron Moderation In Power Stations
Control Rods: Key To Regulating Reactor Power Output
Understanding Heat Exchangers In Nuclear Power Stations
Safeguarding Nuclear Reactors: Key Protective Measures
Unlocking The Complexities Of Nuclear Waste Management
Sun's Energy Secret: The Role of Fusion in Stellar Power
Unraveling The Proton-Proton Cycle: Stellar Nuclear Fusion
Unlocking The Secrets Of Stars: The Hertzsprung–Russell Diagram Explored
Stellar Evolution: The Role of Interstellar Medium & Mass
Evolution Of Moderate Mass Stars: Unveiling The Mysteries Of White Dwarfs
Stellar Evolution: The Journey From Massive Stars To Black Holes
Unlocking Space: Understanding Astrophysics Distance Units
Stellar Parallax: Unlocking Secrets of Star Distances
Unlocking Stellar Secrets: How Black-Body Radiation Defines Star Properties
IB Resources
Theme E - Nuclear & Quantum Physics
Physics HL
Physics HL

Theme E - Nuclear & Quantum Physics

Unveiling The Secrets: Long Half-Lives & Thorium-232 Explained

Word Count Emoji
674 words
Reading Time Emoji
4 mins read
Updated at Emoji
Last edited on 5th Nov 2024

Table of content

What are half-lives?

Imagine you have a heap of candy, and every hour, half of that candy magically disappears. The time it takes for half the candy to disappear is its "half-life". Now, replace candy with radioactive atoms, and you get the idea! 😁

Types of Half-lives

Long Half-lives: Imagine a magical candy that takes a year for just half of it to disappear! This is what long half-lives are like. It's when the half-life is much longer than the time we measure.

How to determine half-lives?

For long half-lives

  • Direct Method: Use the equation A = λN
  • Substitution & Rearrangement Method: T1/2​= \(\frac {0.693}{A} × N\)

Glossary

  • A: Activity of the sample (kinda like how active or hyper the candy is in disappearing!)
  • λ (lambda): Decay constant (how fast our atoms are decaying)
  • N: Total number of atoms

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IB Resources
Theme E - Nuclear & Quantum Physics
Physics HL
Physics HL

Theme E - Nuclear & Quantum Physics

Unveiling The Secrets: Long Half-Lives & Thorium-232 Explained

Word Count Emoji
674 words
Reading Time Emoji
4 mins read
Updated at Emoji
Last edited on 5th Nov 2024

Table of content

What are half-lives?

Imagine you have a heap of candy, and every hour, half of that candy magically disappears. The time it takes for half the candy to disappear is its "half-life". Now, replace candy with radioactive atoms, and you get the idea! 😁

Types of Half-lives

Long Half-lives: Imagine a magical candy that takes a year for just half of it to disappear! This is what long half-lives are like. It's when the half-life is much longer than the time we measure.

How to determine half-lives?

For long half-lives

  • Direct Method: Use the equation A = λN
  • Substitution & Rearrangement Method: T1/2​= \(\frac {0.693}{A} × N\)

Glossary

  • A: Activity of the sample (kinda like how active or hyper the candy is in disappearing!)
  • λ (lambda): Decay constant (how fast our atoms are decaying)
  • N: Total number of atoms

Unlock the Full Content! File Is Locked Emoji

Dive deeper and gain exclusive access to premium files of Physics HL. Subscribe now and get closer to that 45 🌟

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