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AKU MBBS Admission Test Physics Syllabus

The Physics syllabus for AKU MBBS Admission Test in full: 7 chapters and 24 topics, every one listed below, plus 61 Physics flashcards with answers.

7Chapters
24Topics
61Flashcards

Physics syllabus: all 7 chapters

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

  1. Mechanics

    5 topics
    • Kinematics
    • Newton's Laws of Motion
    • Work, Energy and Power
    • Momentum and Collisions
    • Circular and Rotational Motion
  2. Properties of Matter

    2 topics
    • Elasticity and Stress-Strain
    • Fluid Dynamics
  3. Waves and Oscillations

    3 topics
    • Simple Harmonic Motion
    • Wave Properties and Sound
    • Resonance and Doppler Effect
  4. Thermodynamics

    3 topics
    • Heat, Temperature and Thermal Expansion
    • Laws of Thermodynamics
    • Kinetic Theory of Gases
  5. Optics

    4 topics
    • Reflection and Refraction
    • Lenses and Mirrors
    • Interference and Diffraction
    • Optical Instruments
  6. Electricity and Magnetism

    4 topics
    • Electrostatics
    • Current Electricity and Circuits
    • Magnetic Fields and Forces
    • Electromagnetic Induction
  7. Modern Physics

    3 topics
    • Photoelectric Effect and Quantum Theory
    • Atomic and Nuclear Physics
    • Radioactivity

AKU MBBS Admission Test Physics flashcards — 61 questions with answers

  1. In kinematics, what is the difference between distance and displacement?

    Distance is the total path length travelled (a scalar, always positive). Displacement is the straight-line change in position from start to end, with direction (a vector); its magnitude can be less than or equal to distance.

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

    v = u + at; s = ut + (1/2)at^2; v^2 = u^2 + 2as, where u = initial velocity, v = final velocity, a = acceleration, t = time, s = displacement.

  3. For a body in free fall (ignoring air resistance), what is its acceleration and does it depend on mass?

    It accelerates downward at g (about 9.8 m/s^2 on Earth), independent of mass; all bodies fall at the same rate in a vacuum.

  4. For projectile motion, what are the horizontal and vertical acceleration components?

    Horizontal acceleration is zero (constant horizontal velocity); vertical acceleration equals g downward. The two motions are independent.

  5. What are the formulas for the time of flight, maximum height, and range of a projectile launched at angle theta with speed u?

    Time of flight T = 2u sin(theta)/g; Maximum height H = u^2 sin^2(theta)/(2g); Range R = u^2 sin(2theta)/g. Maximum range occurs at theta = 45 degrees.

  6. State Newton's First Law of Motion (law of inertia).

    A body remains at rest or in uniform motion in a straight line unless acted upon by a net external force. This property of resisting change in motion is called inertia.

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

    The rate of change of momentum of a body is proportional to the applied net force and occurs in the direction of the force: F = dp/dt = ma (for constant mass).

  8. State Newton's Third Law of Motion.

    For every action there is an equal and opposite reaction; the action and reaction forces act on two different bodies and are equal in magnitude, opposite in direction.

  9. What is the difference 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).

  10. Define the coefficient of friction and write the formula for limiting friction.

    The coefficient of friction (mu) is the ratio of the limiting frictional force to the normal reaction: mu = F/R, so limiting friction F = mu R. It is dimensionless.

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

    Work is done when a force moves its point of application along its direction: W = F s cos(theta), where theta is the angle between force and displacement. SI unit is the joule (J) = N·m.

  12. Write the formulas for kinetic energy and gravitational potential energy.

    Kinetic energy KE = (1/2)mv^2; gravitational potential energy PE = mgh (near Earth's surface).

  13. State the work-energy theorem.

    The net work done on a body equals the change in its kinetic energy: W_net = (1/2)mv^2 - (1/2)mu^2 = delta KE.

  14. Define power and give two formulas for it.

    Power is the rate of doing work: P = W/t. It also equals P = F·v (force times velocity). SI unit is the watt (W) = J/s.

  15. State the law of conservation of energy.

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

  16. Define linear momentum and state the law of conservation of momentum.

    Linear momentum p = mv (a vector). In the absence of an external force, the total momentum of an isolated system remains constant before and after interaction.

  17. Define impulse and state the impulse-momentum theorem.

    Impulse = force × time = F·t, equal to the change in momentum: F·t = delta p = m(v - u). SI unit is N·s (or kg·m/s).

  18. Compare 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 converts to heat/sound); in a perfectly inelastic collision the bodies stick together.

  19. In a one-dimensional elastic collision of two equal masses, one moving and one at rest, what happens?

    The moving body stops and transfers all its velocity to the stationary body; they exchange velocities.

  20. Define centripetal acceleration and force for circular motion, with formulas.

    Centripetal acceleration a = v^2/r = omega^2 r, directed toward the center. Centripetal force F = mv^2/r = m omega^2 r, the net inward force needed to keep a body in a circular path.

Show the other 41 Physics flashcards
  1. Define angular velocity and relate it to linear velocity.

    Angular velocity omega = theta/t (rad/s) is the rate of change of angular displacement. Linear (tangential) velocity v = r omega, where r is the radius.

  2. Define torque and write its formula.

    Torque (moment of force) is the turning effect of a force: tau = r F sin(theta) = r × F. SI unit is N·m. It causes angular acceleration.

  3. Define moment of inertia and state its role in rotational motion.

    Moment of inertia I = sum of m r^2 is the rotational analogue of mass; it measures resistance to angular acceleration. Rotational form of Newton's second law: tau = I alpha.

  4. State the law of conservation of angular momentum and define angular momentum.

    Angular momentum L = I omega (= mvr for a point mass). In the absence of external torque, total angular momentum is conserved; e.g., a spinning skater speeds up when pulling arms in (I decreases, omega increases).

  5. Define stress and strain and give the formula for Young's modulus.

    Stress = force per unit area (F/A, in pascals). Strain = change in dimension/original dimension (dimensionless). Young's modulus Y = tensile stress/tensile strain = (F/A)/(delta L/L).

  6. State Hooke's law for elastic materials.

    Within the elastic limit, stress is directly proportional to strain (stress = constant × strain); equivalently, for a spring, force F = -kx, where k is the spring constant.

  7. What do the elastic limit and yield point mean on a stress-strain curve?

    The elastic limit is the maximum stress a material can endure and still return to its original shape. Beyond the yield point the material deforms permanently (plastically) and will not fully recover.

  8. State the equation of continuity for fluid flow and what it expresses.

    A1 v1 = A2 v2 (volume flow rate is constant for an incompressible fluid). It shows that fluid speed increases where the cross-sectional area decreases.

  9. State Bernoulli's equation and the principle it expresses.

    P + (1/2)rho v^2 + rho g h = constant along a streamline. It expresses conservation of energy in fluid flow: where speed is higher, pressure is lower.

  10. Define viscosity and state Stokes' law for a sphere in a fluid.

    Viscosity is a fluid's internal resistance to flow. Stokes' law: the drag force on a small sphere is F = 6 pi eta r v, where eta is viscosity, r the radius, v the velocity.

  11. What is terminal velocity?

    Terminal velocity is the constant maximum velocity reached by an object falling through a fluid when the net force is zero (weight balanced by drag plus buoyancy), so acceleration becomes zero.

  12. Define simple harmonic motion (SHM) and give its defining equation.

    SHM is oscillatory motion in which acceleration is directly proportional to displacement from the mean position and directed toward it: a = -omega^2 x. The restoring force F = -kx.

  13. Give the formulas for the time period of a mass-spring system and a simple pendulum.

    Mass-spring: T = 2 pi sqrt(m/k). Simple pendulum: T = 2 pi sqrt(L/g). Both are independent of amplitude (for small oscillations).

  14. For SHM, where are velocity and acceleration maximum and minimum?

    Velocity is maximum at the mean (equilibrium) position and zero at the extremes. Acceleration is maximum at the extremes and zero at the mean position.

  15. Differentiate between transverse and longitudinal waves with examples.

    In transverse waves particles vibrate perpendicular to the direction of propagation (e.g., light, water surface, string waves). In longitudinal waves particles vibrate parallel to propagation, forming compressions and rarefactions (e.g., sound waves).

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

    v = f λ, where v is wave speed, f is frequency, and λ is wavelength. Period T = 1/f.

  17. How does the speed of sound vary with the medium and temperature?

    Sound travels fastest in solids, slower in liquids, slowest in gases. In a gas, speed increases with temperature (roughly proportional to the square root of absolute temperature); in air it is about 343 m/s at 20 degrees C.

  18. Define resonance.

    Resonance occurs when a system is driven at its natural frequency, causing the amplitude of oscillation to become maximum because energy transfer from the driver is most efficient.

  19. State the formula for the fundamental frequency of a stretched string.

    f = (1/2L) sqrt(T/mu), where L is the length, T is the tension, and mu is the mass per unit length. The fundamental has one antinode and nodes at both ends.

  20. State the Doppler effect and what happens to observed frequency as a source approaches or recedes.

    The Doppler effect is the apparent change in frequency due to relative motion between source and observer. Frequency increases (pitch rises) when they approach and decreases (pitch falls) when they recede.

  21. Distinguish between heat and temperature.

    Heat is the total thermal energy transferred between bodies due to a temperature difference (in joules). Temperature is the measure of the average kinetic energy of particles and determines the direction of heat flow (in kelvin/celsius).

  22. Convert between Celsius and Kelvin, and give absolute zero.

    K = degrees C + 273.15. Absolute zero is 0 K = -273.15 degrees C, the temperature at which molecular kinetic energy is minimum.

  23. Give the formulas for linear, areal, and volumetric thermal expansion.

    Linear: delta L = L0 alpha delta T. Areal: delta A = A0 (2 alpha) delta T. Volumetric: delta V = V0 (3 alpha) delta T, where alpha is the coefficient of linear expansion.

  24. State the first law of thermodynamics.

    The heat supplied to a system equals the increase in its internal energy plus the work done by the system: Q = delta U + W. It is a statement of conservation of energy.

  25. State the second law of thermodynamics.

    Heat cannot spontaneously flow from a colder body to a hotter body; equivalently, no engine can convert all absorbed heat into work (entropy of an isolated system tends to increase).

  26. Give the formula for the efficiency of a Carnot engine.

    Efficiency = 1 - T_cold/T_hot, where temperatures are in kelvin. Carnot efficiency is the maximum possible for an engine between two given temperatures.

  27. State the postulates of the kinetic theory of gases (key assumptions).

    Gas consists of many tiny molecules in constant random motion; molecular volume is negligible vs container; collisions are perfectly elastic; no intermolecular forces except during collisions; average kinetic energy is proportional to absolute temperature.

  28. Relate the average translational kinetic energy of a gas molecule to temperature.

    Average translational KE = (3/2)kT per molecule, where k is the Boltzmann constant and T is absolute temperature. This shows temperature is a measure of molecular kinetic energy.

  29. State the laws of reflection of light.

    1) The incident ray, reflected ray, and the normal at the point of incidence all lie in the same plane. 2) The angle of incidence equals the angle of reflection.

  30. State Snell's law of refraction and define refractive index.

    n1 sin(theta1) = n2 sin(theta2). The refractive index n = speed of light in vacuum/speed in medium = c/v; it measures how much a medium bends light.

  31. Define total internal reflection and the critical angle.

    Total internal reflection occurs when light travels from a denser to a rarer medium and the angle of incidence exceeds the critical angle, so all light reflects back. Critical angle: sin(theta_c) = 1/n (for medium to air).

  32. Write the mirror/lens formula and the magnification formula.

    1/f = 1/v + 1/u (lens and mirror, using sign convention). Magnification m = h_image/h_object = -v/u (lens) or m = -v/u for mirrors. For mirrors f = R/2.

  33. Compare the images formed by convex and concave lenses.

    A convex (converging) lens can form real, inverted images or, when the object is within the focal length, a virtual, magnified, upright image. A concave (diverging) lens always forms a virtual, upright, diminished image.

  34. State the condition for constructive and destructive interference of light in terms of path difference.

    Constructive interference (bright fringe): path difference = n λ. Destructive interference (dark fringe): path difference = (n + 1/2) λ, where n is an integer.

  35. Give the fringe spacing formula for Young's double-slit experiment.

    Fringe spacing (separation between adjacent bright fringes) = λ D/d, where λ is wavelength, D is the slit-to-screen distance, and d is the slit separation.

  36. Define diffraction and give the diffraction grating equation.

    Diffraction is the bending and spreading of waves around obstacles or through narrow slits. Grating equation: d sin(theta) = n λ, where d is the grating spacing and n the order of the maximum.

  37. State the magnifying power of a simple microscope (magnifying glass) at near point.

    Magnifying power M = 1 + D/f, where D is the least distance of distinct vision (about 25 cm) and f is the focal length of the lens.

  38. Describe a compound microscope and a telescope in terms of their lenses.

    A compound microscope uses two convex lenses (objective of short focal length, eyepiece) to magnify small nearby objects. A refracting telescope uses a long-focal-length objective and a short-focal-length eyepiece to view distant objects; its magnification M = f_objective/f_eyepiece.

  39. State Coulomb's law of electrostatics.

    The 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 = k q1 q2 / r^2, where k = 1/(4 pi epsilon0) ≈ 9 × 10^9 N·m^2/C^2.

  40. Define electric field intensity and electric potential.

    Electric field intensity E = F/q (force per unit positive charge, in N/C or V/m), a vector. Electric potential V = W/q (work done per unit charge to bring it from infinity, in volts), a scalar; E = -dV/dr.

  41. Define capacitance and give the capacitance of a parallel-plate capacitor.

    Capacitance C = Q/V (charge stored per unit potential difference, in farads). For a parallel-plate capacitor C = epsilon0 epsilon_r A/d, where A is plate area, d the separation, and epsilon_r the relative permittivity of the dielectric.

AKU MBBS Admission Test Physics FAQ

What is in the AKU MBBS Admission Test Physics syllabus?

AKU MBBS Admission Test Physics is split into 7 chapters: Mechanics, Properties of Matter, Waves and Oscillations, Thermodynamics, Optics, Electricity and Magnetism and Modern Physics. Together they contain 24 topics.

How many chapters are in AKU MBBS Admission Test Physics?

7 chapters, containing 24 topics. The largest chapter is Mechanics, with 5 topics.

Are there flashcards for AKU MBBS Admission Test Physics?

Yes — a 61-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.