🇵🇰 HEC USAT · subject

HEC USAT Physics Syllabus

The Physics syllabus for HEC USAT in full: 6 chapters and 20 topics, every one listed below, plus 54 Physics flashcards with answers.

6Chapters
20Topics
54Flashcards

Physics syllabus: all 6 chapters

Expand any chapter to see its topics and sub-topics.

  1. Mechanics

    4 topics
    • Kinematics
    • Newton's Laws of Motion
    • Work, Energy and Power
    • Momentum and Collisions
  2. Waves and Oscillations

    3 topics
    • Simple Harmonic Motion
    • Wave Properties
    • Sound and Acoustics
  3. Heat and Thermodynamics

    3 topics
    • Temperature and Thermal Expansion
    • Laws of Thermodynamics
    • Heat Transfer
  4. Electricity and Magnetism

    4 topics
    • Electrostatics
    • Current Electricity and Ohm's Law
    • Magnetic Fields and Forces
    • Electromagnetic Induction
  5. Optics

    3 topics
    • Reflection and Refraction
    • Lenses and Mirrors
    • Wave Optics
  6. Modern Physics

    3 topics
    • Atomic Structure
    • Photoelectric Effect
    • Nuclear Physics and Radioactivity

HEC USAT Physics flashcards — 54 questions with answers

  1. Define displacement and state how it differs from distance.

    Displacement is the change in position of an object in a given direction; it is a vector (has magnitude and direction). Distance is the total path length travelled and is a scalar.

  2. State the three equations of motion for uniform acceleration.

    v = u + at; s = ut + ½at²; v² = u² + 2as (where u = initial velocity, v = final velocity, a = acceleration, s = displacement, t = time).

  3. What is the difference between speed and velocity?

    Speed is the rate of change of distance (scalar). Velocity is the rate of change of displacement (vector), having both magnitude and direction.

  4. For a projectile launched at angle θ with speed u, give the formulas for time of flight, maximum height, and range.

    Time of flight = 2u sinθ / g; Maximum height = u²sin²θ / 2g; Range = u²sin2θ / g.

  5. What does the slope and the area of a velocity–time graph represent?

    The slope gives acceleration; the area under the graph gives displacement.

  6. What is the acceleration due to gravity near Earth's surface, and in which direction does it act?

    Approximately 9.8 m/s² (often taken as 9.81 or 10 m/s²), directed vertically downward toward Earth's centre.

  7. State Newton's First Law of Motion.

    A body remains at rest or in uniform motion in a straight line unless acted upon by a net external force. (Law of inertia.)

  8. State Newton's Second Law of Motion and its formula.

    The rate of change of momentum of a body is directly proportional to the applied force and occurs in the direction of the force. F = ma (or F = dp/dt).

  9. State Newton's Third Law of Motion.

    For every action there is an equal and opposite reaction; the forces act on two different bodies.

  10. Define inertia and state what it depends on.

    Inertia is the tendency of a body to resist any change in its state of rest or motion. It depends on (is directly proportional to) the body's mass.

  11. What is the SI unit of force and how is it defined?

    The newton (N). One newton is the force that gives a 1 kg mass an acceleration of 1 m/s² (1 N = 1 kg·m/s²).

  12. Distinguish between mass and weight.

    Mass is the amount of matter in a body (scalar, in kg, constant everywhere). Weight is the gravitational force on the body, W = mg (vector, in newtons, varies with g).

  13. What is the difference between static friction and kinetic friction?

    Static friction acts between surfaces at rest and adjusts up to a maximum to prevent motion. Kinetic (sliding) friction acts between surfaces in relative motion and is generally smaller than maximum static friction.

  14. Define work in physics and give its formula and SI unit.

    Work is the product of force and displacement in the direction of the force: W = Fs cosθ. SI unit is the joule (J).

  15. Give the formulas for kinetic energy and gravitational potential energy.

    Kinetic energy KE = ½mv²; Gravitational potential energy PE = mgh.

  16. State the work–energy theorem.

    The net work done on a body equals the change in its kinetic energy: W_net = ½mv² − ½mu² = ΔKE.

  17. Define power and give its formula and SI unit.

    Power is the rate of doing work (or rate of energy transfer): P = W/t = Fv. SI unit is the watt (W), where 1 W = 1 J/s.

  18. State the principle (law) of conservation of energy.

    Energy can neither be created nor destroyed; it can only be transformed from one form to another. The total energy of an isolated system remains constant.

  19. Define efficiency and give its formula.

    Efficiency is the ratio of useful output energy (or power) to total input energy (or power): Efficiency = (useful output / total input) × 100%.

  20. Define linear momentum and give its formula, unit, and type of quantity.

    Momentum is the product of mass and velocity: p = mv. SI unit is kg·m/s. It is a vector quantity.

Show the other 34 Physics flashcards
  1. State the law of conservation of momentum.

    If no external force acts on a system, its total momentum remains constant; the total momentum before a collision equals the total momentum after it.

  2. Define impulse and state its relationship to momentum.

    Impulse is the product of force and the time for which it acts: J = F·t. Impulse equals the change in momentum: F·t = Δp = mv − mu.

  3. Distinguish between elastic and inelastic collisions.

    In an elastic collision both momentum and kinetic energy are conserved. In an inelastic collision momentum is conserved but kinetic energy is not (some is converted to heat, sound, etc.).

  4. What is a perfectly inelastic collision?

    A collision in which the colliding bodies stick together and move with a common velocity afterward; momentum is conserved but the maximum possible kinetic energy is lost.

  5. Define Simple Harmonic Motion (SHM).

    SHM is oscillatory motion in which the restoring force (and acceleration) is directly proportional to the displacement from the mean position and always directed toward it: a = −ω²x.

  6. Give the formula for the time period of a simple pendulum.

    T = 2π√(L/g), where L is the length of the pendulum and g is the acceleration due to gravity.

  7. Give the formula for the time period of a mass–spring system in SHM.

    T = 2π√(m/k), where m is the mass and k is the spring constant.

  8. Define amplitude, time period, and frequency of an oscillation, and give the relation between period and frequency.

    Amplitude is the maximum displacement from the mean position; time period (T) is the time for one complete oscillation; frequency (f) is the number of oscillations per second. Relation: f = 1/T.

  9. In SHM, where are the velocity and acceleration of the oscillating body maximum and minimum?

    Velocity is maximum at the mean position and zero at the extreme positions. Acceleration is maximum at the extreme positions and zero at the mean position.

  10. State the wave equation relating speed, frequency, and wavelength.

    v = fλ, where v is wave speed, f is frequency, and λ is wavelength.

  11. Distinguish between transverse and longitudinal waves, giving one example of each.

    In transverse waves the particles vibrate perpendicular to the direction of wave travel (e.g., light, water surface waves). In longitudinal waves the particles vibrate parallel to the direction of travel (e.g., sound waves).

  12. Define wavelength and frequency of a wave.

    Wavelength is the distance between two consecutive points in phase (e.g., crest to crest). Frequency is the number of complete waves passing a point per second, measured in hertz (Hz).

  13. Name the four main wave phenomena.

    Reflection, refraction, diffraction, and interference.

  14. What is the difference between constructive and destructive interference?

    Constructive interference occurs when waves meet in phase, producing a larger amplitude. Destructive interference occurs when waves meet out of phase (antiphase), reducing or cancelling the amplitude.

  15. Approximately what is the speed of sound in air at room temperature, and how does it compare with its speed in solids?

    About 340 m/s in air at room temperature. Sound travels faster in liquids and fastest in solids; it cannot travel through a vacuum.

  16. What property of a sound wave determines its loudness and which determines its pitch?

    Loudness is determined by the amplitude of the wave; pitch is determined by its frequency.

  17. Define the Doppler effect.

    The Doppler effect is the apparent change in the observed frequency (or wavelength) of a wave due to relative motion between the source and the observer — frequency increases as they approach and decreases as they move apart.

  18. What is an echo and what causes it?

    An echo is a reflected sound heard distinctly after the original sound; it is caused by the reflection of sound waves from a hard, distant surface, with a delay long enough for the ear to distinguish the two.

  19. Define the audible frequency range for humans and the terms ultrasound and infrasound.

    The human audible range is about 20 Hz to 20,000 Hz. Ultrasound is sound above 20,000 Hz; infrasound is sound below 20 Hz.

  20. What is temperature, and name three common temperature scales.

    Temperature is a measure of the average kinetic energy of the particles of a substance (its degree of hotness or coldness). Three scales: Celsius (°C), Fahrenheit (°F), and Kelvin (K).

  21. Convert between Celsius and Kelvin, and give the value of absolute zero.

    K = °C + 273.15. Absolute zero is 0 K = −273.15 °C, the lowest possible temperature.

  22. Give the formula for linear thermal expansion of a solid.

    ΔL = αL₀ΔT, where ΔL is change in length, α is the coefficient of linear expansion, L₀ is original length, and ΔT is change in temperature.

  23. State the First Law of Thermodynamics and its formula.

    Energy is conserved: the heat added to a system equals the increase in its internal energy plus the work done by the system. ΔU = Q − W (or Q = ΔU + W).

  24. State the Second Law of Thermodynamics.

    Heat flows spontaneously from a hotter body to a colder body, never the reverse without external work; the entropy of an isolated system tends to increase. No engine can convert all heat into work.

  25. What is internal energy of a system?

    Internal energy is the total energy contained within a system — the sum of the kinetic and potential energies of all its molecules.

  26. Name and describe the three modes of heat transfer.

    Conduction: heat transfer through direct contact of particles (mainly in solids). Convection: heat transfer by the bulk movement of a heated fluid (liquids and gases). Radiation: heat transfer by electromagnetic waves, requiring no medium.

  27. What is thermal conduction and in which state of matter is it most effective?

    Conduction is the transfer of heat through a material by particle vibrations/collisions without bulk movement of the material. It is most effective in solids, especially metals (good conductors).

  28. Why is heat transfer by radiation different from conduction and convection?

    Radiation transfers heat as electromagnetic waves and does not require a material medium, so it can occur through a vacuum (e.g., heat from the Sun). Conduction and convection both require matter.

  29. State Coulomb's law and give its formula.

    The electrostatic force between two point charges is directly proportional to the product of the charges and inversely proportional to the square of the distance between them: F = kq₁q₂/r² (k ≈ 9×10⁹ N·m²/C²).

  30. What is the SI unit of electric charge, and what is the charge on a single electron?

    The SI unit of charge is the coulomb (C). The charge on an electron is −1.6×10⁻¹⁹ C (the proton carries +1.6×10⁻¹⁹ C).

  31. State Ohm's law and give its formula.

    At constant temperature, the current through a conductor is directly proportional to the potential difference across it: V = IR, where R is the resistance.

  32. Define electric current and give its SI unit.

    Electric current is the rate of flow of electric charge: I = Q/t. Its SI unit is the ampere (A), where 1 A = 1 C/s.

  33. How do total resistances combine for resistors in series and in parallel?

    In series: R_total = R₁ + R₂ + R₃ + … In parallel: 1/R_total = 1/R₁ + 1/R₂ + 1/R₃ + … (parallel total is less than the smallest resistor).

  34. Give two formulas for electrical power dissipated in a resistor.

    P = VI; and using Ohm's law, P = I²R or P = V²/R.

HEC USAT Physics FAQ

What is in the HEC USAT Physics syllabus?

HEC USAT Physics is split into 6 chapters: Mechanics, Waves and Oscillations, Heat and Thermodynamics, Electricity and Magnetism, Optics and Modern Physics. Together they contain 20 topics.

How many chapters are in HEC USAT Physics?

6 chapters, containing 20 topics. The largest chapter is Mechanics, with 4 topics.

Are there flashcards for HEC USAT Physics?

Yes — a 54-card Physics deck, printed in full in the flashcards section of this page and available in the Examius app with spaced repetition. The free plan covers one exam of your choice, including its flashcards; Examius Pro, a one-time purchase, unlocks every other exam and deck.