IB Physics Standard Level

This subject is broken down into 36 topics in 12 modules:

  1. Measurements and uncertainties 3 topics
  2. Mechanics 4 topics
  3. Thermal physics 2 topics
  4. Waves 5 topics
  5. Electricity and magnetism 4 topics
  6. Circular motion and gravitation 2 topics
  7. Atomic, nuclear and particle physics 3 topics
  8. Energy production 2 topics
  9. Option A: Relativity 3 topics
  10. Option B: Engineering physics 2 topics
  11. Option C: Imaging 3 topics
  12. Option D: Astrophysics 3 topics
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  • 12
    modules
  • 36
    topics
  • 14,561
    words of revision content
  • 1+
    hours of audio lessons

This page was last modified on 28 September 2024.

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Physics

Measurements and uncertainties

Measurements in physics

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Measurements in physics

Fundamental quantities and units

  • Understand and recall the seven fundamental quantities used in the International System of Units (SI) – second, metre, kilogram, ampere, kelvin, mole, and candela.
  • Be aware that each fundamental quantity has a associated SI unit: second for time, metre for length, kilogram for mass, ampere for electric current, kelvin for temperature, mole for number of particles, and candela for luminous intensity.
  • Recognise that derived units are generated by combining the fundamental units, e.g. newtons for force (kg m/s²) or joules for energy (kg m²/s²).

Precision, Accuracy and Uncertainty

  • Distinguish between precision (how closely individual measurements agree with each other) and accuracy (how close a measurement is to the true value).
  • Understand that uncertainty represents a range within which the true value is likely to lie, and is sometimes described as the precision of the equipment.
  • Reconstruct percentage uncertainty by dividing the absolute uncertainty by the measured value and multiplying by 100.

Measurement Techniques and Tools

  • Differentiate between the types of measurements taken in an experiment, including discrete, continuous, and categorical measurements.
  • Highlight the range of measuring tools, such as metre rules, vernier calipers, and micrometers, and their corresponding precisions.
  • Grasp how random vs systematic errors can have different impacts on results and recognise ways to reduce these.

Significant Figures and Scientific Notation

  • Implement the rules for counting significant figures in a given number.
  • Round numbers according to the principles of significant figures, appreciating that uncertainties should have a maximum of two significant figures.
  • Use scientific notation to conveniently express very large or small numbers.

Graphical Representation of Uncertainties

  • Identify error bars on a graph as a basic visual indicator of the uncertainty of each datapoint.
  • Understand how to calculate the gradient and its uncertainty of a line of best fit, incorporating uncertainties of individual measurements.
  • Interpret the y-intercept of the best fitting line and its uncertainty.

Data Analysis

  • Understand how to evaluate mean, median, and mode as statistical descriptors of a dataset.
  • Recognise standard deviation as a measure of dispersion of a dataset.
  • Perform propagation of uncertainties when doing calculations involving multiple measurements.

The aim is to understand and apply these principles and techniques to represent, analyse, and interpret scientific measurement data effectively in Physics.

Course material for Physics, module Measurements and uncertainties, topic Measurements in physics

Physics

Circular motion and gravitation

Circular motion

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Circular motion

Circular Motion Basics

  • Traditionally, motion is described along a straight line (rectilinear motion), but some objects like the moon, earth, and artificial satellites move in a circular path.
  • This unique behaviour is known as circular motion which happens when an object moves in a circle at a constant speed.
  • The velocity is always tangent to the circle at that point of motion.
  • Despite a constant speed, the object moving in a circle does change its velocity as there is a change in direction at every point in the orbit.

Key Terms in Circular Motion

Centripetal Force:

  • Centripetal force is the net force causing circular motion, acting towards the centre of the circle.
  • This force causes an object to move in a circular path and its absence causes the object to move off in a straight line.
  • The word 'centripetal' comes from Latin centr-, meaning centre, and petere, meaning to seek, hence it's a force that seeks the centre.
  • The net force is always equal to the centripetal force at any point in a circular path.

Centripetal Acceleration:

  • As there is a change in velocity in circular motion, the object experiences an acceleration.
  • This acceleration, known as centripetal acceleration, also always points towards the centre of the circle.
  • The centripetal force needed to maintain an object's circular motion is directly proportional to the object's mass and the square of its speed, and inversely proportional to the radius of the circle.
  • The formula to calculate centripetal acceleration is

    a = v^2 / r

    , where v is the velocity and r is the radius of the circular path.

Tangential Speed (Linear Speed):

  • Tangential speed or linear speed is the speed of an object moving along a circular path.
  • It is often described in terms of the rotation angle per unit of time.

Period and Frequency:

  • The period (T) of an object in circular motion refers to the time it takes for one complete rotation or revolution.
  • The frequency (f) is the number of rotations or revolutions per unit of time, usually per second.
  • The relationship between period and frequency is

    f = 1 / T

    .

Circular Motion Equations

  • Here are the main equations related to circular motion:
    • Centripetal Force:

      F = mv^2 / r

    • Centripetal Acceleration:

      a = v^2 / r

    • Tangential Speed:

      v = 2πr / T

  • Take note of the units used in these equations. Remember to convert them to SI units.

Understanding the Concepts

  • Circular motion concepts become clearer through real-world examples, such as spinning a stone tied to a string, the movement of celestial bodies, or the motion of an electron in a magnetic field.
  • Understanding the forces at work and how the acceleration and velocity of an object in circular motion changes is essential in solving problems.
  • Ask yourself: What would happen if the centripetal force suddenly disappeared? This helps understand its role in maintaining circular motion.

Solving Problems

  • When solving circular motion problems, identify the known and unknown variables.
  • Remember F=ma or Newton's second law of motion is applicable.
  • Make sure you understand whether the problem is asking for angular or tangential speed.
  • Be careful with unit conversions, especially when dealing with revolutions per minute (rpm) and radians per second.

Remember, practice makes perfect. Understanding circular motion requires continuous learning and solving various problems. Take your time and soon it will all make sense. Happy revising!

Course material for Physics, module Circular motion and gravitation, topic Circular motion

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