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RUHS / State Nursing Entrance Physics Syllabus

The Physics syllabus for RUHS / State Nursing Entrance in full: 4 chapters, 17 topics and 44 sub-topics, every one listed below, plus 59 Physics flashcards with answers.

4Chapters
17Topics
44Sub-topics
59Flashcards

Physics syllabus: all 4 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 and vector resolution
    • Laws of Motion
      • Newton's three laws
      • Friction and its applications
      • Circular motion and centripetal force
    • Work, Energy and Power
      • Work-energy theorem
      • Conservation of mechanical energy
      • Collisions: elastic and inelastic
    • Gravitation
      • Universal law of gravitation
      • Acceleration due to gravity and its variation
      • Satellites and escape velocity
  2. Properties of Matter and Heat

    4 topics
    • Elasticity and Fluid Mechanics
      • Stress, strain and modulus of elasticity
      • Pressure, Pascal's law and Archimedes principle
      • Surface tension and viscosity
    • Thermal Properties
      • Temperature scales and thermal expansion
      • Heat capacity, latent heat and calorimetry
      • Modes of heat transfer
    • Thermodynamics
      • Zeroth and first law of thermodynamics
      • Isothermal and adiabatic processes
      • Second law and heat engines
    • Kinetic Theory of Gases
      • Gas laws and ideal gas equation
      • Kinetic interpretation of temperature
  3. Electricity and Magnetism

    4 topics
    • Electrostatics
      • Coulomb's law and electric field
      • Electric potential and capacitance
    • Current Electricity
      • Ohm's law and resistance
      • Kirchhoff's laws and circuit networks
      • Heating effect of current
    • Magnetic Effects of Current
      • Biot-Savart law and Ampere's law
      • Force on a current-carrying conductor
    • Electromagnetic Induction
      • Faraday's and Lenz's laws
      • Self and mutual inductance
  4. Optics and Modern Physics

    4 topics
    • Ray Optics
      • Reflection and refraction
      • Lenses, mirrors and lens formula
      • Optical instruments: microscope and telescope
    • Wave Optics
      • Interference and Young's double slit
      • Diffraction and polarization
    • Atomic and Nuclear Physics
      • Bohr model of the atom
      • Radioactivity and nuclear reactions
    • Dual Nature and Electronics
      • Photoelectric effect
      • Semiconductors, diodes and logic gates

RUHS / State Nursing Entrance Physics flashcards — 59 questions with answers

  1. State the principle of homogeneity of dimensions.

    In any physically correct equation, the dimensions of all the terms on both sides must be the same. It is used to check the correctness of equations and to derive relations among physical quantities.

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

    Force = [MLT⁻²]; Work/Energy = [ML²T⁻²]; Power = [ML²T⁻³].

  3. Define the SI base unit and dimensional formula of pressure.

    Pressure = force/area. SI unit = pascal (Pa) = N/m². Dimensional formula = [ML⁻¹T⁻²].

  4. Distinguish between accuracy and precision in measurement.

    Accuracy is how close a measured value is to the true value; precision is how close repeated measurements are to one another (reproducibility). High precision does not guarantee high accuracy.

  5. Write 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.

  6. At what angle of projection is the horizontal range of a projectile maximum, and what is that range?

    Maximum range occurs at a projection angle of 45°. Maximum range R = u²/g, where u is the launch speed.

  7. Differentiate between distance and displacement.

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

  8. 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; net force equals rate of change of momentum. 3rd: For every action there is an equal and opposite reaction.

  9. What is impulse, and how is it related to momentum?

    Impulse = force × time of action (J = F·Δt). By the impulse–momentum theorem, impulse equals the change in momentum: J = Δp = mΔv. Units: N·s or kg·m/s.

  10. State the law of conservation of linear momentum.

    In the absence of a net external force, the total linear momentum of a system remains constant. For a collision: m₁u₁ + m₂u₂ = m₁v₁ + m₂v₂.

  11. Distinguish between static, limiting, and kinetic friction.

    Static friction adjusts to prevent motion (0 ≤ fs ≤ μsN); limiting friction is its maximum value just before sliding (μsN); kinetic friction acts during sliding (μkN) and is slightly less than limiting friction (μk < μs).

  12. State the work–energy theorem.

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

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

    Kinetic energy KE = ½mv²; gravitational potential energy (near Earth's surface) PE = mgh, where h is height above the reference level.

  14. Differentiate between conservative and non-conservative forces.

    For a conservative force (e.g., gravity, spring), work done is path-independent and around a closed loop is zero; potential energy can be defined. For a non-conservative force (e.g., friction), work is path-dependent and energy is dissipated.

  15. 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.

  16. State Newton's law of universal gravitation.

    Every two point masses attract each other with a force F = G·m₁m₂/r², directed along the line joining them, where G = 6.67 × 10⁻¹¹ N·m²/kg².

  17. What is acceleration due to gravity g, and how does it relate to G?

    g = GM/R², where M and R are Earth's mass and radius. Standard value ≈ 9.8 m/s². It is independent of the mass of the falling body.

  18. Write the formulae for escape velocity and orbital velocity of a satellite near Earth's surface.

    Escape velocity v_e = √(2GM/R) = √(2gR) ≈ 11.2 km/s. Orbital velocity (near surface) v_o = √(GM/R) = √(gR) ≈ 7.9 km/s. Note v_e = √2 · v_o.

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

    1st (Orbits): Planets move in ellipses with the Sun at one focus. 2nd (Areas): The line joining planet and Sun sweeps equal areas in equal times. 3rd (Periods): T² ∝ a³, where a is the semi-major axis.

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

    Stress = force/area (N/m²); strain = change in dimension/original dimension (dimensionless); Young's modulus Y = longitudinal stress/longitudinal strain. Higher Y means a stiffer (less elastic) material.

Show the other 39 Physics flashcards
  1. State Hooke's law and define the elastic limit.

    Hooke's law: within the elastic limit, stress is directly proportional to strain (stress = E × strain). The elastic limit is the maximum stress up to which a body fully regains its shape after the load is removed.

  2. State Pascal's law and give an application.

    Pascal's law: pressure applied to an enclosed fluid is transmitted undiminished to every part of the fluid and the container walls. Application: hydraulic lift/brakes/jack.

  3. State Archimedes' principle.

    A body wholly or partially immersed in a fluid experiences an upward buoyant force equal to the weight of the fluid displaced. It determines flotation and apparent weight loss.

  4. State Bernoulli's theorem (equation) for fluid flow.

    For steady, non-viscous, incompressible flow: P + ½ρv² + ρgh = constant along a streamline (sum of pressure, kinetic, and potential energy per unit volume is constant).

  5. Define coefficient of viscosity and state the SI unit.

    Viscosity measures a fluid's internal resistance to flow (η = shearing stress / velocity gradient). SI unit = pascal-second (Pa·s) or N·s/m²; CGS unit = poise.

  6. Convert between Celsius, Fahrenheit, and Kelvin temperature scales.

    K = °C + 273.15; °F = (9/5)°C + 32; °C = (5/9)(°F − 32). Ice point = 0°C = 32°F = 273.15 K.

  7. Distinguish between specific heat capacity and latent heat.

    Specific heat (c) is heat per unit mass to change temperature by 1°C (Q = mcΔT); latent heat (L) is heat per unit mass to change phase at constant temperature (Q = mL), with no temperature change.

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

    Conduction: heat flows through a medium by molecular collisions without bulk motion (solids). Convection: heat transfer by actual movement of fluid (liquids/gases). Radiation: transfer by electromagnetic waves, needing no medium.

  9. State Newton's law of cooling.

    The rate of loss of heat of a body is directly proportional to the difference between its temperature and that of the surroundings, provided this difference is small: dQ/dt ∝ (T − T_surr).

  10. 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 applied to heat.

  11. Define isothermal, adiabatic, isobaric, and isochoric processes.

    Isothermal: constant temperature (ΔU = 0). Adiabatic: no heat exchange (ΔQ = 0). Isobaric: constant pressure. Isochoric (isovolumetric): constant volume (ΔW = 0).

  12. State the second law of thermodynamics (Kelvin–Planck statement) and efficiency of a heat engine.

    No process can convert heat completely into work with no other effect (no 100%-efficient engine). Efficiency η = W/Q₁ = 1 − Q₂/Q₁, where Q₁ is heat absorbed and Q₂ is heat rejected.

  13. What is the Carnot engine efficiency formula?

    η = 1 − T₂/T₁, where T₁ and T₂ are the source and sink absolute (Kelvin) temperatures. It is the maximum possible efficiency of any heat engine operating between these temperatures.

  14. State the postulates of the kinetic theory of gases.

    Gas consists of many tiny molecules in random motion; molecular volume is negligible; collisions are perfectly elastic; no intermolecular forces except during collisions; time between collisions ≫ collision time; pressure is due to molecular impacts on walls.

  15. Write the kinetic theory expression for the pressure of an ideal gas.

    P = (1/3)·(mN/V)·v̄² = (1/3)ρv_rms², where v_rms is the root-mean-square speed, ρ the density, and N the number of molecules. Hence PV = (1/3)Nmv_rms².

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

    Each degree of freedom contributes ½kT of energy per molecule. Average translational KE of a molecule = (3/2)kT, where k is Boltzmann's constant (1.38 × 10⁻²³ J/K).

  17. State Coulomb's law of electrostatics.

    The force between two point charges is F = k·q₁q₂/r², directed along the line joining them; like charges repel, unlike attract. k = 1/4πε₀ ≈ 9 × 10⁹ N·m²/C².

  18. Define electric field intensity and electric potential.

    Electric field E = force per unit positive test charge (E = F/q₀; units N/C or V/m, a vector). Electric potential V = work done per unit charge to bring it from infinity to that point (units volt = J/C, a scalar).

  19. State Gauss's law.

    The total electric flux through a closed surface equals 1/ε₀ times the net charge enclosed: Φ = ∮E·dA = q_enclosed/ε₀.

  20. Write the formula for capacitance of a parallel-plate capacitor and energy stored.

    C = ε₀A/d (with dielectric, C = Kε₀A/d). Energy stored U = ½CV² = ½QV = Q²/2C.

  21. State Ohm's law and define resistance.

    Ohm's law: at constant temperature, current through a conductor is directly proportional to the voltage across it (V = IR). Resistance R = V/I; SI unit = ohm (Ω).

  22. Write the formula for resistance in terms of resistivity, and how resistivity varies with temperature for metals.

    R = ρL/A, where ρ is resistivity, L length, A cross-sectional area. For metals, resistivity increases with temperature: ρ_T = ρ₀(1 + αΔT).

  23. Give the formulae for resistors in series and in parallel.

    Series: R_eq = R₁ + R₂ + R₃ + … (same current). Parallel: 1/R_eq = 1/R₁ + 1/R₂ + … (same voltage); R_eq is less than the smallest resistor.

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

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

  25. State the Biot–Savart law and the right-hand rule for a current-carrying wire.

    Biot–Savart: dB = (μ₀/4π)·(I·dl × r̂)/r², giving the magnetic field due to a current element. Right-hand rule: thumb points along current, curled fingers give the direction of the magnetic field lines.

  26. Write the expression for the magnetic force on a current-carrying conductor and on a moving charge.

    On a conductor: F = BIL sinθ. On a moving charge: F = qvB sinθ (Lorentz force F = q(v × B)). The force is maximum when motion/current is perpendicular to B.

  27. State Faraday's laws of electromagnetic induction.

    1st: A changing magnetic flux through a circuit induces an EMF. 2nd: The induced EMF equals the negative rate of change of magnetic flux: ε = −dΦ/dt (for N turns, ε = −N·dΦ/dt).

  28. State Lenz's law and the principle it conserves.

    The direction of an induced current always opposes the change in magnetic flux producing it. The negative sign in ε = −dΦ/dt expresses it; Lenz's law is a consequence of conservation of energy.

  29. 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/v + 1/u = 1/f; magnification m = −v/u = h'/h.

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

    Snell's law: n₁ sinθ₁ = n₂ sinθ₂ (sinθ₁/sinθ₂ = n₂/n₁ = constant). Refractive index n = speed of light in vacuum / speed in medium = c/v; it measures how much light bends.

  31. State the conditions for total internal reflection.

    (1) Light must travel from a denser to a rarer medium; (2) the angle of incidence must exceed the critical angle θ_c, where sinθ_c = 1/n. Used in optical fibres and prisms.

  32. Write the lens-maker's formula and define lens power.

    Lens-maker's formula: 1/f = (n − 1)(1/R₁ − 1/R₂). Power P = 1/f (in metres); unit = dioptre (D). Converging (convex) lenses have positive power; diverging (concave) lenses negative.

  33. State the conditions for constructive and destructive interference of light.

    Constructive (bright): path difference = nλ (phase difference 2nπ). Destructive (dark): path difference = (n + ½)λ (phase difference odd multiple of π), where n = 0, 1, 2, …

  34. In Young's double-slit experiment, what is the formula for fringe width?

    Fringe width β = λD/d, where λ is wavelength, D is slit-to-screen distance, and d is the slit separation. All bright/dark fringes are equally spaced.

  35. What is the photoelectric effect, and write Einstein's photoelectric equation.

    Emission of electrons from a metal when light of sufficient frequency falls on it. Einstein's equation: hν = φ + KE_max, i.e., KE_max = hν − hν₀, where φ = work function and ν₀ = threshold frequency.

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

    Every moving particle has an associated matter wave of wavelength λ = h/p = h/mv, where h is Planck's constant and p is momentum. It expresses the wave–particle dual nature of matter.

  37. Distinguish between nuclear fission and nuclear fusion.

    Fission: a heavy nucleus splits into lighter nuclei releasing energy (e.g., U-235). Fusion: light nuclei combine into a heavier nucleus releasing energy (e.g., H → He in the Sun). Both release energy via mass defect (E = mc²).

  38. Define half-life and write the radioactive decay law.

    Half-life (T½) is the time for half the nuclei in a sample to decay; T½ = 0.693/λ. Decay law: N = N₀e^(−λt), where λ is the decay constant and N₀ the initial number of nuclei.

  39. In a P–N junction diode, distinguish forward and reverse bias.

    Forward bias: p-side to positive terminal; depletion layer narrows, resistance is low, and the diode conducts. Reverse bias: p-side to negative terminal; depletion layer widens, resistance is high, and almost no current flows (only small leakage).

RUHS / State Nursing Entrance Physics FAQ

What is in the RUHS / State Nursing Entrance Physics syllabus?

RUHS / State Nursing Entrance Physics is split into 4 chapters: Mechanics, Properties of Matter and Heat, Electricity and Magnetism and Optics and Modern Physics. Together they contain 17 topics and 44 sub-topics.

How many chapters are in RUHS / State Nursing Entrance Physics?

4 chapters, containing 17 topics and 44 sub-topics. The largest chapter is Mechanics, with 5 topics.

Are there flashcards for RUHS / State Nursing Entrance Physics?

Yes — a 59-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.