In one day, a -kg mountain climber ascends from the -m level on a vertical cliff to the top at m. The next day, she descends from the top to the base of the cliff, which is at an elevation of m. What is her change in gravitational potential energy on the first day?
Table of contents
- 0. Math Review31m
- 1. Intro to Physics Units1h 29m
- 2. 1D Motion / Kinematics3h 56m
- Vectors, Scalars, & Displacement13m
- Average Velocity32m
- Intro to Acceleration7m
- Position-Time Graphs & Velocity26m
- Conceptual Problems with Position-Time Graphs22m
- Velocity-Time Graphs & Acceleration5m
- Calculating Displacement from Velocity-Time Graphs15m
- Conceptual Problems with Velocity-Time Graphs10m
- Calculating Change in Velocity from Acceleration-Time Graphs10m
- Graphing Position, Velocity, and Acceleration Graphs11m
- Kinematics Equations37m
- Vertical Motion and Free Fall19m
- Catch/Overtake Problems23m
- 3. Vectors2h 43m
- Review of Vectors vs. Scalars1m
- Introduction to Vectors7m
- Adding Vectors Graphically22m
- Vector Composition & Decomposition11m
- Adding Vectors by Components13m
- Trig Review24m
- Unit Vectors15m
- Introduction to Dot Product (Scalar Product)12m
- Calculating Dot Product Using Components12m
- Intro to Cross Product (Vector Product)23m
- Calculating Cross Product Using Components17m
- 4. 2D Kinematics1h 42m
- 5. Projectile Motion3h 6m
- 6. Intro to Forces (Dynamics)3h 22m
- 7. Friction, Inclines, Systems2h 44m
- 8. Centripetal Forces & Gravitation7h 26m
- Uniform Circular Motion7m
- Period and Frequency in Uniform Circular Motion20m
- Centripetal Forces15m
- Vertical Centripetal Forces10m
- Flat Curves9m
- Banked Curves10m
- Newton's Law of Gravity30m
- Gravitational Forces in 2D25m
- Acceleration Due to Gravity13m
- Satellite Motion: Intro5m
- Satellite Motion: Speed & Period35m
- Geosynchronous Orbits15m
- Overview of Kepler's Laws5m
- Kepler's First Law11m
- Kepler's Third Law16m
- Kepler's Third Law for Elliptical Orbits15m
- Gravitational Potential Energy21m
- Gravitational Potential Energy for Systems of Masses17m
- Escape Velocity21m
- Energy of Circular Orbits23m
- Energy of Elliptical Orbits36m
- Black Holes16m
- Gravitational Force Inside the Earth13m
- Mass Distribution with Calculus45m
- 9. Work & Energy1h 59m
- 10. Conservation of Energy2h 54m
- Intro to Energy Types3m
- Gravitational Potential Energy10m
- Intro to Conservation of Energy32m
- Energy with Non-Conservative Forces20m
- Springs & Elastic Potential Energy19m
- Solving Projectile Motion Using Energy13m
- Motion Along Curved Paths4m
- Rollercoaster Problems13m
- Pendulum Problems13m
- Energy in Connected Objects (Systems)24m
- Force & Potential Energy18m
- 11. Momentum & Impulse3h 40m
- Intro to Momentum11m
- Intro to Impulse14m
- Impulse with Variable Forces12m
- Intro to Conservation of Momentum17m
- Push-Away Problems19m
- Types of Collisions4m
- Completely Inelastic Collisions28m
- Adding Mass to a Moving System8m
- Collisions & Motion (Momentum & Energy)26m
- Ballistic Pendulum14m
- Collisions with Springs13m
- Elastic Collisions24m
- How to Identify the Type of Collision9m
- Intro to Center of Mass15m
- 12. Rotational Kinematics2h 59m
- 13. Rotational Inertia & Energy7h 4m
- More Conservation of Energy Problems54m
- Conservation of Energy in Rolling Motion45m
- Parallel Axis Theorem13m
- Intro to Moment of Inertia28m
- Moment of Inertia via Integration18m
- Moment of Inertia of Systems23m
- Moment of Inertia & Mass Distribution10m
- Intro to Rotational Kinetic Energy16m
- Energy of Rolling Motion18m
- Types of Motion & Energy24m
- Conservation of Energy with Rotation35m
- Torque with Kinematic Equations56m
- Rotational Dynamics with Two Motions50m
- Rotational Dynamics of Rolling Motion27m
- 14. Torque & Rotational Dynamics2h 5m
- 15. Rotational Equilibrium3h 39m
- 16. Angular Momentum3h 6m
- Opening/Closing Arms on Rotating Stool18m
- Conservation of Angular Momentum46m
- Angular Momentum & Newton's Second Law10m
- Intro to Angular Collisions15m
- Jumping Into/Out of Moving Disc23m
- Spinning on String of Variable Length20m
- Angular Collisions with Linear Motion8m
- Intro to Angular Momentum15m
- Angular Momentum of a Point Mass21m
- Angular Momentum of Objects in Linear Motion7m
- 17. Periodic Motion2h 9m
- 18. Waves & Sound3h 40m
- Intro to Waves11m
- Velocity of Transverse Waves21m
- Velocity of Longitudinal Waves11m
- Wave Functions31m
- Phase Constant14m
- Average Power of Waves on Strings10m
- Wave Intensity19m
- Sound Intensity13m
- Wave Interference8m
- Superposition of Wave Functions3m
- Standing Waves30m
- Standing Wave Functions14m
- Standing Sound Waves12m
- Beats8m
- The Doppler Effect7m
- 19. Fluid Mechanics4h 27m
- 20. Heat and Temperature3h 7m
- Temperature16m
- Linear Thermal Expansion14m
- Volume Thermal Expansion14m
- Moles and Avogadro's Number14m
- Specific Heat & Temperature Changes12m
- Latent Heat & Phase Changes16m
- Intro to Calorimetry21m
- Calorimetry with Temperature and Phase Changes15m
- Advanced Calorimetry: Equilibrium Temperature with Phase Changes9m
- Phase Diagrams, Triple Points and Critical Points6m
- Heat Transfer44m
- 21. Kinetic Theory of Ideal Gases1h 50m
- 22. The First Law of Thermodynamics1h 26m
- 23. The Second Law of Thermodynamics3h 11m
- 24. Electric Force & Field; Gauss' Law3h 42m
- 25. Electric Potential1h 51m
- 26. Capacitors & Dielectrics2h 2m
- 27. Resistors & DC Circuits3h 8m
- 28. Magnetic Fields and Forces2h 23m
- 29. Sources of Magnetic Field2h 30m
- Magnetic Field Produced by Moving Charges10m
- Magnetic Field Produced by Straight Currents27m
- Magnetic Force Between Parallel Currents12m
- Magnetic Force Between Two Moving Charges9m
- Magnetic Field Produced by Loops andSolenoids42m
- Toroidal Solenoids aka Toroids12m
- Biot-Savart Law (Calculus)18m
- Ampere's Law (Calculus)17m
- 30. Induction and Inductance3h 38m
- 31. Alternating Current2h 37m
- Alternating Voltages and Currents18m
- RMS Current and Voltage9m
- Phasors20m
- Resistors in AC Circuits9m
- Phasors for Resistors7m
- Capacitors in AC Circuits16m
- Phasors for Capacitors8m
- Inductors in AC Circuits13m
- Phasors for Inductors7m
- Impedance in AC Circuits18m
- Series LRC Circuits11m
- Resonance in Series LRC Circuits10m
- Power in AC Circuits5m
- 32. Electromagnetic Waves2h 14m
- 33. Geometric Optics2h 57m
- 34. Wave Optics1h 15m
- 35. Special Relativity2h 10m
10. Conservation of Energy
Intro to Conservation of Energy
Problem 25
Textbook Question
In which of the following reactions or decays is strangeness conserved? In each case, explain your reasoning.
(a)
(b)
(c)
(d)

1
Step 1: Understand the concept of strangeness conservation. Strangeness is a quantum number associated with the presence of strange quarks in particles. In strong and electromagnetic interactions, strangeness is conserved. However, in weak interactions, strangeness can change by ±1.
Step 2: Analyze reaction (a): K⁺ + μ⁺ + ν_μ. The K⁺ meson contains a strange quark (s) and an up antiquark (u̅). The muon (μ⁺) and neutrino (ν_μ) are leptons and do not carry strangeness. This reaction involves the weak interaction (due to the presence of neutrinos), so strangeness may not be conserved. Check the initial and final states to confirm.
Step 3: Analyze reaction (b): n + K⁺ → p + π⁰. The neutron (n) and proton (p) are baryons, while K⁺ and π⁰ are mesons. The K⁺ meson has a strangeness of +1, while the neutron, proton, and π⁰ have a strangeness of 0. Since the initial state has a total strangeness of +1 and the final state has a total strangeness of 0, strangeness is not conserved. This reaction likely involves the weak interaction.
Step 4: Analyze reaction (c): K⁺ + K⁻ → π⁰ + π⁰. The K⁺ meson has a strangeness of +1, and the K⁻ meson has a strangeness of -1. The π⁰ mesons have a strangeness of 0. The total strangeness in the initial state is 0 (+1 + -1), and the total strangeness in the final state is also 0. Strangeness is conserved, so this reaction likely occurs via the strong interaction.
Step 5: Analyze reaction (d): p + K⁻ → Λ⁰ + π⁰. The proton (p) has a strangeness of 0, the K⁻ meson has a strangeness of -1, the Λ⁰ baryon has a strangeness of -1, and the π⁰ meson has a strangeness of 0. The total strangeness in the initial state is -1 (0 + -1), and the total strangeness in the final state is also -1 (-1 + 0). Strangeness is conserved, so this reaction likely occurs via the strong interaction.

This video solution was recommended by our tutors as helpful for the problem above
Play a video:
Was this helpful?
Key Concepts
Here are the essential concepts you must grasp in order to answer the question correctly.
Strangeness
Strangeness is a quantum number that reflects the presence of strange quarks in a particle. It is defined as the negative of the number of strange quarks minus the number of anti-strange quarks. In particle interactions, strangeness is conserved in strong and electromagnetic processes, but can change in weak interactions. Understanding how strangeness behaves in different reactions is crucial for determining whether it is conserved.
Recommended video:
Guided course
Time Dilation
Conservation Laws in Particle Physics
Conservation laws are fundamental principles in physics that state certain properties of isolated systems remain constant over time. In particle physics, key conservation laws include those for energy, momentum, charge, baryon number, and strangeness. These laws help predict the outcomes of particle interactions and decays, guiding physicists in analyzing which reactions can occur and under what conditions.
Recommended video:
Guided course
Conservation of Charge
Types of Interactions
In particle physics, interactions can be classified into three main types: strong, weak, and electromagnetic. Strong interactions govern the behavior of quarks and gluons, while weak interactions are responsible for processes like beta decay and can change strangeness. Electromagnetic interactions involve charged particles and photons. Recognizing the type of interaction involved in a reaction is essential for understanding whether certain quantum numbers, like strangeness, are conserved.
Recommended video:
Guided course
Overview of Collision Types
Watch next
Master Conservation Of Mechanical Energy with a bite sized video explanation from Patrick
Start learningRelated Videos
Related Practice
Textbook Question
300
views