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IB PHYSICS
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1. Measurement
A. Units and Magnitude
B. Uncertainties
C. Vectors and Scalars
2. Mechanics
A. Motion
B. Equations of motion and Projectile motion
C. Forces and Newton's laws
D. Momentum and Impulse
E. Work, Energy and Power
03. Thermal Physics
A. Modelling a gas
B. Thermal Concepts
04. SHM and Waves
A. Oscillations
B. Travelling waves
C. Reflection and Refraction
D. Polarisation
E. Standing waves
F. Interference and Diffraction
05. Electricity and Magnetism
A. Electric fields
B. The heating effects of electric current
C. Electric cells
D. The magnetic effects of electric currents
06. Circular motion and Gravity
A. Circular motion
B. Newton's law of gravitation
07. Atomic, Nuclear and Particle Physics
A. Discrete energy and Radioactivity
B. Nuclear reactions
C. The structure of matter
08. Energy Production
A. Energy sources
B. Thermal energy transfer
09. Wave Phenomena (HL)
A. Simple Harmonic motion
B. Single-slit diffraction
C. Interference
D. Resolution
E. Doppler effect
10. Fields (HL)
A. Describing fields
B. Fields at work
11. Electromagnetic Induction (HL)
A. Electromagnetic Induction
B. Power generation and transmission
C. Capacitance
12. Quantum and Nuclear Physics (HL)
A. The interaction of matter with radiation
B. Nuclear Physics
OPTION Astrophysics (SL and HL)
A. Stellar quantities
B. Stellar characteristics and evolution
C. Cosmology
D. Stellar processes (HL)
E. Further Cosmology (HL)
Revision
Internal Assessment
The Nature of Science
Extended Essay in Physics
Theory of Knowledge
Answers to Textbook questions (Oxford Physics)
LoggerPro
Pre-IB Physics course
IB PHYSICS
Stellar processes (HL)
Understandings:
The Jeans criterion
Nuclear fusion
Nucleosynthesis off the main sequence
Type Ia and II supernovae
Applications and skills:
Applying the Jeans criterion to star formation
Describing the different types of nuclear fusion reactions taking place off the main sequence
Applying the mass–luminosity relation to compare lifetimes on the main sequence relative to that of our Sun
Describing the formation of elements in stars that are heavier than iron including the required increases in temperature
Qualitatively describe the s and r processes for neutron capture
Distinguishing between type Ia and II supernovae
Guidance:
Only an elementary application of the Jeans criterion is required, ie collapse of an interstellar cloud may begin if M > Mj
Students should be aware of the use of type Ia supernovae as standard candles
Stellar evolution.pptx
stellar evolution questions and MS.docx
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