🇮🇳 AIIMS Nursing (BSc) Entrance · subject

AIIMS Nursing (BSc) Entrance Physics Syllabus

The Physics syllabus for AIIMS Nursing (BSc) Entrance in full: 5 chapters, 22 topics and 52 sub-topics, every one listed below, plus 60 Physics flashcards with answers.

5Chapters
22Topics
52Sub-topics
60Flashcards

Physics syllabus: all 5 chapters

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

  1. Mechanics

    5 topics
    • Units, Dimensions and Measurement
      • SI units and fundamental quantities
      • Dimensional analysis and applications
      • Significant figures and error analysis
    • Kinematics
      • Motion in a straight line and equations of motion
      • Projectile motion
      • Relative velocity
    • Laws of Motion
      • Newton's three laws and momentum
      • Friction and its laws
      • Circular motion and centripetal force
    • Work, Energy and Power
      • Work-energy theorem
      • Conservation of mechanical energy
      • Collisions (elastic and inelastic)
    • Gravitation
      • Newton's law of gravitation
      • Acceleration due to gravity and its variation
      • Escape velocity and satellite motion
  2. Properties of Matter and Heat

    5 topics
    • Elasticity
      • Stress, strain and Hooke's law
      • Young's, bulk and rigidity modulus
    • Fluid Mechanics
      • Pressure, Pascal's and Archimedes' principle
      • Bernoulli's theorem and viscosity
      • Surface tension and capillarity
    • Thermal Properties
      • Thermal expansion and calorimetry
      • Modes of heat transfer
    • Thermodynamics
      • Laws of thermodynamics
      • Thermodynamic processes and heat engines
    • Kinetic Theory of Gases
      • Gas laws and ideal gas equation
      • Degrees of freedom and specific heats
  3. Oscillations and Waves

    3 topics
    • Simple Harmonic Motion
      • Displacement, velocity and acceleration in SHM
      • Simple pendulum and spring-mass system
    • Wave Motion
      • Transverse and longitudinal waves
      • Speed of waves and superposition
    • Sound and Acoustics
      • Standing waves and resonance
      • Beats and Doppler effect
  4. Electricity and Magnetism

    4 topics
    • Electrostatics
      • Coulomb's law and electric field
      • Electric potential and capacitance
      • Gauss's law
    • Current Electricity
      • Ohm's law and resistance
      • Kirchhoff's laws and Wheatstone bridge
      • Heating effect of current
    • Magnetic Effects of Current
      • Biot-Savart and Ampere's law
      • Force on current-carrying conductor
    • Electromagnetic Induction and AC
      • Faraday's and Lenz's law
      • Alternating current and LCR circuits
  5. Optics and Modern Physics

    5 topics
    • Ray Optics
      • Reflection and refraction at surfaces
      • Lenses, mirrors and optical instruments
    • Wave Optics
      • Interference and Young's double slit
      • Diffraction and polarization
    • Dual Nature of Matter and Radiation
      • Photoelectric effect
      • de Broglie wavelength
    • Atoms and Nuclei
      • Bohr model of atom
      • Radioactivity and nuclear reactions
    • Semiconductor Electronics
      • p-n junction diode and rectifiers
      • Transistors and logic gates

AIIMS Nursing (BSc) Entrance Physics flashcards — 60 questions with answers

  1. State the principle of homogeneity of dimensions and one of its uses.

    Every term on both sides of a valid physical equation must have the same dimensions. It is used to check the correctness of equations and to derive relations between physical quantities.

  2. What are the dimensional formulae of force, work/energy, and power?

    Force = [MLT^-2]; Work/Energy = [ML^2T^-2]; Power = [ML^2T^-3].

  3. Define a light year and give its approximate value.

    A light year is the distance travelled by light in one year in vacuum; it equals about 9.46 x 10^15 metres.

  4. What is the difference between accuracy and precision in measurement?

    Accuracy is how close a measurement is to the true value; precision is how close repeated measurements are to one another (consistency), independent of the true value.

  5. Distinguish between distance and displacement.

    Distance is the total path length covered (a scalar, always positive); displacement is the shortest straight-line vector from initial to final position (can be zero or negative).

  6. Write the three equations of motion for uniform acceleration.

    v = u + at; s = ut + (1/2)at^2; v^2 = u^2 + 2as.

  7. For a projectile launched at angle θ with speed u, give time of flight, maximum height, and horizontal range.

    Time of flight T = 2u sinθ/g; Max height H = u^2 sin^2θ/(2g); Range R = u^2 sin2θ/g (maximum at θ = 45°).

  8. What is the relation between linear velocity v, angular velocity ω, and radius r in circular motion?

    v = ωr; and centripetal acceleration a = v^2/r = ω^2 r.

  9. State Newton's three laws of motion.

    1st: A body remains at rest or in uniform motion unless acted on by a net external force (inertia). 2nd: F = ma (rate of change of momentum equals applied force). 3rd: Every action has an equal and opposite reaction.

  10. State the law of conservation of linear momentum.

    If no external force acts on a system, its total linear momentum remains constant. For two bodies: m1u1 + m2u2 = m1v1 + m2v2.

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

    Impulse = force x time = F·t (a vector). Impulse-momentum theorem: impulse equals the change in momentum, F·t = Δp = m(v - u).

  12. Differentiate between static, limiting, and kinetic friction.

    Static friction acts on a stationary body and self-adjusts up to a maximum; limiting friction is that maximum value just before motion; kinetic friction acts during sliding and is slightly less than limiting friction (f = μN).

  13. State the work-energy theorem.

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

  14. Write the formulae for kinetic energy and gravitational potential energy.

    Kinetic energy KE = (1/2)mv^2; Gravitational PE near Earth = mgh.

  15. 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 lost as heat/sound/deformation).

  16. State Newton's law of universal gravitation.

    Every two masses attract each other with a force F = G m1 m2 / r^2, directed along the line joining them; G = 6.67 x 10^-11 N m^2 kg^-2.

  17. Write the formulae for acceleration due to gravity g, orbital velocity, and escape velocity.

    g = GM/R^2; orbital velocity v_o = √(GM/R); escape velocity v_e = √(2GM/R) = √2 · v_o (≈11.2 km/s for Earth).

  18. State Kepler's three laws of planetary motion.

    1st (Law of orbits): planets move in ellipses with the Sun at one focus. 2nd (Law of areas): the line joining planet and Sun sweeps equal areas in equal times. 3rd (Law of periods): T^2 ∝ a^3.

  19. Define stress, strain, and Young's modulus.

    Stress = force/area (N/m^2); strain = change in dimension/original dimension (dimensionless); Young's modulus Y = longitudinal stress/longitudinal strain.

  20. State Hooke's law of elasticity.

    Within the elastic limit, stress is directly proportional to strain; stress = (modulus of elasticity) x strain.

Show the other 40 Physics flashcards
  1. State Pascal's law.

    Pressure applied to an enclosed fluid is transmitted undiminished equally in all directions and to the walls of the container. It is the basis of the hydraulic press.

  2. State Archimedes' principle.

    A body fully or partially immersed in a fluid experiences an upward buoyant force equal to the weight of the fluid displaced.

  3. State Bernoulli's theorem for streamline flow.

    For an ideal incompressible fluid in streamline flow, P + (1/2)ρv^2 + ρgh = constant along a streamline (conservation of energy per unit volume).

  4. Define coefficient of viscosity and state Stokes' law.

    Viscosity measures a fluid's resistance to flow. Stokes' law: viscous drag on a small sphere of radius r moving with velocity v in a fluid of viscosity η is F = 6πηrv.

  5. Distinguish between heat and temperature.

    Heat is the total thermal energy transferred between bodies due to a temperature difference (measured in joules); temperature is the degree of hotness/average kinetic energy of molecules (measured in kelvin/°C).

  6. Give the formulae for linear, areal, and cubical (volume) thermal expansion coefficients' relation.

    If α is linear, β is areal, γ is cubical expansion coefficient, then β = 2α and γ = 3α (so α:β:γ = 1:2:3).

  7. Name the three modes of heat transfer with one feature each.

    Conduction (heat through a solid without bulk movement of particles); Convection (heat by actual movement of fluid particles); Radiation (heat as electromagnetic waves, needs no medium).

  8. State Newton's law of cooling.

    The rate of loss of heat of a body is directly proportional to the difference in temperature between the body and its surroundings (for small temperature differences).

  9. State the first law of thermodynamics.

    Heat supplied to a system equals the increase in internal energy plus the work done by the system: ΔQ = ΔU + ΔW. It is the law of conservation of energy.

  10. State the second law of thermodynamics (Kelvin-Planck and Clausius statements).

    Kelvin-Planck: no engine can convert all absorbed heat completely into work. Clausius: heat cannot spontaneously flow from a colder to a hotter body without external work.

  11. Define an isothermal and an adiabatic process.

    Isothermal: process at constant temperature (ΔT = 0, PV = constant). Adiabatic: process with no heat exchange with surroundings (ΔQ = 0, PV^γ = constant).

  12. Give the efficiency formula of a Carnot engine.

    Efficiency η = 1 - T2/T1, where T1 is the source (hot) temperature and T2 the sink (cold) temperature in kelvin.

  13. State the postulates relating pressure to molecular motion in kinetic theory.

    Gas pressure P = (1/3)ρ c_rms^2 = (1/3)(mN/V)c_rms^2, where c_rms is the root-mean-square molecular speed; pressure arises from molecular collisions with walls.

  14. State the law of equipartition of energy and average KE of a gas molecule.

    Each degree of freedom carries average energy (1/2)kT. Average translational KE of a molecule = (3/2)kT, where k = Boltzmann constant (1.38 x 10^-23 J/K).

  15. Define simple harmonic motion (SHM).

    SHM is motion in which the restoring force (or acceleration) is directly proportional to displacement from the mean position and always directed toward it: a = -ω^2 x.

  16. Give the time period formulae for a simple pendulum and a spring-mass system.

    Simple pendulum: T = 2π√(L/g). Spring-mass: T = 2π√(m/k).

  17. In SHM, where are velocity and acceleration maximum and minimum?

    Velocity is maximum at the mean position and zero at the extremes; acceleration is zero at the mean position and maximum at the extremes.

  18. Differentiate between transverse and longitudinal waves with examples.

    Transverse: particles vibrate perpendicular to wave direction (e.g., light, waves on a string). Longitudinal: particles vibrate parallel to wave direction, forming compressions and rarefactions (e.g., sound in air).

  19. Write the wave relation connecting speed, frequency, and wavelength.

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

  20. What are beats and the formula for beat frequency?

    Beats are periodic variations in sound intensity due to superposition of two waves of slightly different frequencies; beat frequency = |f1 - f2|.

  21. State the Doppler effect for sound.

    The apparent change in frequency of sound due to relative motion between source and observer; apparent frequency f' = f (v ± v_o)/(v ∓ v_s), where v is sound speed, v_o observer speed, v_s source speed.

  22. State Coulomb's law of electrostatics.

    The force between two point charges is F = k q1 q2 / r^2 (k = 1/4πε₀ = 9 x 10^9 N m^2 C^-2 in vacuum), directed along the line joining the charges.

  23. Define electric field intensity and electric potential.

    Electric field E = force per unit positive charge = F/q (N/C or V/m, a vector). Electric potential V = work done per unit charge to bring it from infinity to a point (volt, a scalar).

  24. Give the formula for the capacitance of a parallel-plate capacitor and energy stored.

    C = ε₀A/d (with a dielectric, multiply by k). Energy stored U = (1/2)CV^2 = (1/2)QV = Q^2/(2C).

  25. State Ohm's law and define resistance and resistivity.

    Ohm's law: V = IR at constant temperature. Resistance R = V/I (ohm). Resistivity ρ relates by R = ρL/A; it is a material property independent of dimensions.

  26. Write the formulae for resistors in series and in parallel.

    Series: R = R1 + R2 + R3 + ... Parallel: 1/R = 1/R1 + 1/R2 + 1/R3 + ...

  27. State Kirchhoff's two laws for electric circuits.

    Junction (current) law: the sum of currents entering a junction equals the sum leaving (charge conservation). Loop (voltage) law: the algebraic sum of EMFs and potential drops around any closed loop is zero (energy conservation).

  28. State the right-hand rule and the formula for force on a current-carrying conductor in a magnetic field.

    Force F = BIL sinθ, where B is magnetic field, I current, L length, θ angle between I and B. The right-hand rule gives the force direction perpendicular to both I and B.

  29. State Faraday's laws of electromagnetic induction and Lenz's law.

    Faraday: an induced EMF is produced when magnetic flux through a circuit changes, with magnitude EMF = -dΦ/dt. Lenz's law: the induced current opposes the change in flux causing it (gives the minus sign, conserving energy).

  30. For a transformer, write the turns ratio relation and state which type steps voltage up.

    Vs/Vp = Ns/Np = Ip/Is (for an ideal transformer). A step-up transformer has more turns in the secondary (Ns > Np), increasing voltage.

  31. State the laws of reflection and the mirror formula.

    Laws of reflection: angle of incidence = angle of reflection, and incident ray, reflected ray, and normal lie in one plane. Mirror formula: 1/f = 1/v + 1/u.

  32. State Snell's law and the lens maker's/thin-lens formula.

    Snell's law: n1 sin i = n2 sin r (refractive index n = sin i/sin r). Thin-lens formula: 1/f = 1/v - 1/u; power P = 1/f (in dioptres).

  33. What is total internal reflection and the condition for it?

    When light travels from a denser to a rarer medium and the angle of incidence exceeds the critical angle, it is fully reflected back into the denser medium. Condition: i > critical angle C, where sin C = 1/n.

  34. State Young's double-slit fringe width formula and the condition for interference.

    Fringe width β = λD/d, where D is slit-to-screen distance and d slit separation. Sustained interference requires two coherent sources (constant phase difference, same frequency).

  35. State the photoelectric equation and define work function.

    Einstein's photoelectric equation: hf = φ + (1/2)mv²max, where hf is photon energy, φ the work function (minimum energy to eject an electron), and the rest is the electron's max KE.

  36. State de Broglie's hypothesis and the wavelength formula.

    Moving particles have an associated wave; de Broglie wavelength λ = h/p = h/mv, where h is Planck's constant and p the momentum.

  37. State Bohr's postulates for the hydrogen atom and the energy of the nth level.

    Electrons revolve in stationary orbits where angular momentum mvr = nh/2π, radiating energy only when jumping between orbits (E = hf). Energy of nth level: En = -13.6/n² eV.

  38. Differentiate between nuclear fission and nuclear fusion.

    Fission: a heavy nucleus splits into lighter nuclei releasing energy (e.g., uranium in reactors). Fusion: light nuclei combine to form a heavier nucleus releasing energy (e.g., in the Sun). Both release energy due to mass defect (E = mc²).

  39. Distinguish between intrinsic and extrinsic semiconductors, and between p-type and n-type.

    Intrinsic: pure semiconductor (Si, Ge). Extrinsic: doped semiconductor. n-type: doped with pentavalent impurity, electrons are majority carriers; p-type: doped with trivalent impurity, holes are majority carriers.

  40. What is a p-n junction diode and what is meant by forward and reverse bias?

    A p-n junction diode allows current mainly in one direction. Forward bias (p to +, n to -) lowers the barrier and conducts; reverse bias raises the barrier and blocks current. Its main use is rectification (AC to DC).

AIIMS Nursing (BSc) Entrance Physics FAQ

What is in the AIIMS Nursing (BSc) Entrance Physics syllabus?

AIIMS Nursing (BSc) Entrance Physics is split into 5 chapters: Mechanics, Properties of Matter and Heat, Oscillations and Waves, Electricity and Magnetism and Optics and Modern Physics. Together they contain 22 topics and 52 sub-topics.

How many chapters are in AIIMS Nursing (BSc) Entrance Physics?

5 chapters, containing 22 topics and 52 sub-topics. The largest chapter is Mechanics, with 5 topics.

Are there flashcards for AIIMS Nursing (BSc) Entrance Physics?

Yes — a 60-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.