Unit 15 | AP Physics 2
Physics 2 Test Booklet Notes
Section 1: Atomic Structure and Properties
Graph of Electron-Nucleus Attraction:
- The graph demonstrates how the attractive force between an electron and a bare nucleus varies with distance.
- Possible representations for the nucleus include labels (A), (B), (C), and (D).Lithium Ion Formation:
- A lithium atom with a net charge can be transformed by:
- (A) Removing two electrons from a neutral lithium atom.
- (B) Adding two electrons to a neutral lithium atom.
- (C) Adding two protons to a neutral lithium atom.
- (D) Removing one electron and adding one proton to a neutral lithium atom.
- Correct Answer: Remove one electron and add one proton (D).Atom Mass Calculation:
- A neutral atom has a mass represented by a notation (A), (B), (C), (D). Determine the most accurate mass approximation for given isotopes.Ranking Neutron Count:
- Given notation for three atomic nuclei, rank the number of neutrons in the three:
- Possible answers include choices (A), (B), (C), and (D).Identifying Isotope Properties:
- To distinguish different isotopes of the same element, consider:
- (A) Mass of the nucleus
- (B) Net charge of the nucleus
- (C) Net charge of the atom or ion
- (D) Number of electrons in the atom or ion.
Section 2: Blackbody Radiation
Modeling Objects:
- Objects 1 and 2 modeled as blackbodies with respective temperatures and surface areas.
- Comparison of total radiated power and peak wavelength:
- Analyze possibilities (A), (B), (C), (D).Blackbody Temperature Graph:
- Evaluate the graph representing intensity of blackbody radiation per unit wavelength as a function of absolute temperature.Star Evolution Dynamics:
- A star, modeled as a spherical blackbody, decreases its radius to one-third while doubling surface temperature:
- Evaluate power changes based on radius and temperature effects. Options:
- (A) Power increases due to radius decrease being stronger than temperature increase.
- (B) Power increases more due to temperature increase.
- (C) Power decrease due to radius effect.
- (D) Power decrease favored by temperature.Thermal Equilibrium of Blackbody:
- Statement about a blackbody at equilibrium:
- (A) Transmits all radiation, emits none.
- (B) Reflects all, emits none.
- (C) Absorbs all radiation, emitting at the same rate.
- (D) Reflects all, emits at the rate reflected.Spherical Blackbodies Comparison:
- Two blackbodies at the same temperature:
- (A) One with a greater mass; analyze claims about peak wavelength.
Section 3: Photon Behavior and Particle Interactions
Photon Collisions:
- Scattering event of photon with stationary electron; resulting velocity components analyzed: (A), (B), (C), (D).Conservation during Scattering:
- Effects of scattering on photon and particle momentum discussed through alternative particle interactions.Photoelectric Effect:
- Emission of electrons from surface due to incident photons, detailing kinetic energy range comparisons under varying power.Energy Transfer Analysis:
- Photon wavelength impact on scattered photons; reactions at various angles and energy considerations listed.Radiative Decay Types:
- Cobalt nucleus remains stable in decay; options detail beta-minus or gamma decay effects.
Section 4: Radioactive Decay Quantifications
Radioactive Decay Rate/Time Calculations:
- Decay constants and remaining atoms calculations between samples across various isotopes.
- Application of half-life considerations over distinct periods.Comparison of Kinetic Energies in Decay:
- Kinetic energy relationships in alpha versus beta decay considered.
Section 5: Quantum Mechanics and Energy Levels
Photon Emission and Absorption Events:
- Examination of energy state transitions and allowed photon interactions.Kinetic Energy of Emitted Electrons:
- Analysis of the relationship between emitted electron speeds post photon interaction.Wavelength and Frequency Relations:
- Corresponding energy calculations to establish photon transition limits.Graphical Representations:
- Interpret the slope relationships in kinetic energy versus frequency graphs showing photoelectric incidences.
Conclusion: These notes encompass a detailed understanding of atomic properties, blackbody radiation, photon interactions, radioactive decay processes, and quantum mechanical principles vital for AP Physics 2 mastery.