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AFMC / NEET-linked AFMC Admission Physics (NEET-UG Academic Component) Syllabus
The Physics (NEET-UG Academic Component) syllabus for AFMC / NEET-linked AFMC Admission in full: 5 chapters, 23 topics and 66 sub-topics, every one listed below, plus 66 Physics (NEET-UG Academic Component) flashcards with answers.
Physics (NEET-UG Academic Component) syllabus: all 5 chapters
Expand any chapter to see its topics and sub-topics.
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Mechanics
6 topics- Kinematics
- Motion in a straight line; displacement, velocity, acceleration
- Uniformly accelerated motion and equations of motion
- Projectile motion and motion in a plane
- Relative velocity in one and two dimensions
- Laws of Motion
- Newton's three laws and concept of inertia
- Friction: static, kinetic, rolling
- Dynamics of circular motion; banking of roads
- Impulse and conservation of linear momentum
- Work, Energy and Power
- Work-energy theorem
- Conservative and non-conservative forces
- Elastic and inelastic collisions
- Rotational Motion
- Centre of mass and moment of inertia
- Torque, angular momentum and its conservation
- Theorems of parallel and perpendicular axes
- Gravitation
- Universal law of gravitation; Kepler's laws
- Acceleration due to gravity and its variation
- Gravitational potential energy and escape velocity
- Orbital velocity and satellites
- Properties of Bulk Matter
- Elasticity: stress, strain, moduli
- Fluid pressure, Pascal's and Archimedes' principles
- Viscosity, Bernoulli's theorem, surface tension
- Kinematics
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Thermodynamics and Kinetic Theory
4 topics- Thermal Properties of Matter
- Thermal expansion and calorimetry
- Heat transfer: conduction, convection, radiation
- Newton's law of cooling and Stefan's law
- Laws of Thermodynamics
- Zeroth and first law; internal energy and work
- Second law, entropy and reversibility
- Carnot engine, refrigerator and efficiency
- Kinetic Theory of Gases
- Ideal gas equation and assumptions
- RMS speed and degrees of freedom
- Equipartition of energy and specific heats
- Thermodynamic Processes
- Isothermal, adiabatic, isobaric, isochoric processes
- PV diagrams and work calculations
- Thermal Properties of Matter
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Oscillations and Waves
3 topics- Simple Harmonic Motion
- Equations of SHM; phase, amplitude, period
- Energy in SHM
- Simple pendulum and spring systems
- Wave Motion
- Transverse and longitudinal waves
- Speed of waves; principle of superposition
- Standing waves in strings and pipes
- Sound and Doppler Effect
- Beats and resonance
- Doppler effect for sound
- Simple Harmonic Motion
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Electrodynamics
5 topics- Electrostatics
- Coulomb's law and electric field
- Gauss's law and applications
- Electric potential, capacitance and dielectrics
- Current Electricity
- Ohm's law, resistivity, drift velocity
- Kirchhoff's laws and Wheatstone bridge
- Potentiometer and metre bridge
- Magnetic Effects of Current
- Biot-Savart and Ampere's circuital law
- Force on current-carrying conductor; moving coil galvanometer
- Magnetism and matter; earth's magnetism
- Electromagnetic Induction and AC
- Faraday's and Lenz's laws
- Self and mutual inductance
- AC circuits, LCR resonance, transformers
- Electromagnetic Waves
- Displacement current and Maxwell's equations (qualitative)
- Electromagnetic spectrum and uses
- Electrostatics
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Optics and Modern Physics
5 topics- Ray Optics
- Reflection and refraction; mirrors and lenses
- Total internal reflection and optical instruments
- Prism and dispersion
- Wave Optics
- Huygens' principle; interference and Young's double slit
- Diffraction and polarisation
- Dual Nature of Matter and Radiation
- Photoelectric effect and Einstein's equation
- de Broglie wavelength
- Atoms and Nuclei
- Bohr model and hydrogen spectrum
- Radioactivity, mass-energy, binding energy
- Nuclear fission and fusion
- Semiconductor Electronics
- Diodes, rectifiers and Zener diode
- Transistors and logic gates
- Ray Optics
AFMC / NEET-linked AFMC Admission Physics (NEET-UG Academic Component) flashcards — 66 questions with answers
In kinematics, what does the area under a velocity-time graph represent, and what does its slope represent?
The area under a v-t graph gives displacement; the slope of a v-t graph gives acceleration.
State the three equations of motion for uniform acceleration (constant a).
v = u + at; s = ut + ½at²; v² = u² + 2as (where u = initial velocity, v = final velocity, s = displacement, t = time).
For projectile motion launched at angle θ with speed u, give the formulas for time of flight, maximum height, and horizontal range.
Time of flight T = 2u sinθ/g; Maximum height H = u²sin²θ/2g; Range R = u²sin2θ/g. Range is maximum at θ = 45°.
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 = dp/dt = ma. 3rd: To every action there is an equal and opposite reaction.
Define impulse and state the impulse-momentum theorem.
Impulse J = F·Δt (force × time); it equals the change in momentum: J = Δp = mv − mu. Impulse is a vector measured in N·s.
Distinguish between static, limiting, and kinetic friction. Which coefficient is larger?
Static friction is self-adjusting up to a maximum (limiting friction = μₛN); kinetic friction (μₖN) acts during relative motion. μₛ > μₖ, so it takes more force to start motion than to keep it moving.
What is the work-energy theorem?
The net work done by all forces on a body equals its change in kinetic energy: W_net = ΔKE = ½mv² − ½mu².
State the law of conservation of mechanical energy and give the condition for it to hold.
In a system where only conservative forces act, total mechanical energy (KE + PE) remains constant. It does not hold when non-conservative forces (e.g., friction) are present.
Define power and give its formula in terms of force and velocity. What is its SI unit?
Power is the rate of doing work: P = W/t = F·v (dot product). SI unit is the watt (W = J/s). 1 horsepower = 746 W.
Compare elastic and inelastic collisions in terms of what is conserved.
In both, momentum is conserved. In an elastic collision, kinetic energy is also conserved; in an inelastic collision, kinetic energy is NOT conserved (some converts to heat/deformation). In a perfectly inelastic collision the bodies stick together.
Define moment of inertia and give its formula for a system of particles.
Moment of inertia is the rotational analogue of mass, measuring resistance to angular acceleration: I = Σmᵢrᵢ², where rᵢ is the perpendicular distance from the axis. SI unit: kg·m².
State the moment of inertia of a solid sphere, a hollow sphere, a solid cylinder/disc, and a thin ring about their central axes.
Solid sphere: (2/5)MR²; Hollow (thin) sphere: (2/3)MR²; Solid cylinder/disc: (1/2)MR²; Thin ring/hoop: MR².
State the parallel axis theorem.
I = I_cm + Md², where I_cm is the moment of inertia about an axis through the center of mass and d is the perpendicular distance to the parallel axis.
What is torque, and how is it related to angular momentum and to angular acceleration?
Torque τ = r × F. It equals the rate of change of angular momentum: τ = dL/dt, and for rigid bodies τ = Iα. When net external torque is zero, angular momentum L is conserved.
State Newton's law of universal gravitation.
Every mass attracts every other mass with a force F = G·m₁m₂/r², directed along the line joining them, where G = 6.67 × 10⁻¹¹ N·m²/kg².
Give the formulas for orbital velocity and escape velocity from a planet's surface.
Orbital velocity (close orbit) v₀ = √(gR) = √(GM/R); Escape velocity vₑ = √(2gR) = √(2GM/R). Thus vₑ = √2 · v₀. For Earth, vₑ ≈ 11.2 km/s.
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 to Sun sweeps equal areas in equal times (constant areal velocity). 3rd (Law of Periods): T² ∝ a³ (square of period proportional to cube of semi-major axis).
How does acceleration due to gravity g vary with height h and depth d (for h, d << R)?
At height: g_h = g(1 − 2h/R). At depth: g_d = g(1 − d/R). g is maximum at the surface and zero at the center of the Earth.
Define stress, strain, and Young's modulus.
Stress = restoring force per unit area (F/A); Strain = fractional change in dimension (ΔL/L), dimensionless; Young's modulus Y = longitudinal stress/longitudinal strain = (F·L)/(A·ΔL). SI unit of Y: pascal (Pa).
State Hooke's law and define the elastic limit.
Hooke's law: within the elastic limit, stress is directly proportional to strain (stress = modulus × strain). The elastic limit is the maximum stress up to which a body returns to its original shape after the load is removed.
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State Pascal's law and the principle behind a hydraulic lift.
Pascal's law: pressure applied to an enclosed fluid is transmitted undiminished to every part of the fluid and the walls. A hydraulic lift uses this to multiply force: F₂/F₁ = A₂/A₁.
State Bernoulli's theorem for ideal fluid flow.
For steady, incompressible, non-viscous flow: P + ½ρv² + ρgh = constant along a streamline (pressure energy + kinetic energy + potential energy per unit volume is conserved).
Define surface tension and state the excess pressure inside a liquid drop and a soap bubble.
Surface tension is force per unit length acting along a liquid surface (N/m). Excess pressure inside a drop: ΔP = 2T/r; inside a soap bubble (two surfaces): ΔP = 4T/r.
State Stokes' law and define terminal velocity.
Viscous drag on a sphere of radius r moving with velocity v in a fluid of viscosity η: F = 6πηrv. Terminal velocity is the constant maximum velocity attained when net force is zero: v_t = 2r²(ρ−σ)g/9η.
Define coefficient of linear, area, and volume thermal expansion and give their relationship.
α (linear), β (area), γ (volume) are fractional changes in length/area/volume per unit temperature rise. Relationship: β = 2α and γ = 3α.
State the principle of calorimetry and define specific heat capacity and latent heat.
Principle of calorimetry: heat lost by hot body = heat gained by cold body (no losses). Specific heat c: heat to raise unit mass by 1°C (Q = mcΔT). Latent heat L: heat to change phase of unit mass without temperature change (Q = mL).
State the three modes of heat transfer and the law governing radiation (Stefan-Boltzmann).
Conduction, convection, and radiation. Stefan-Boltzmann law: energy radiated per unit area per unit time E = σeT⁴, where σ = 5.67×10⁻⁸ W/m²K⁴ and e is emissivity.
State Wien's displacement law and Newton's law of cooling.
Wien's law: λ_max·T = b (b = 2.9×10⁻³ m·K); the wavelength of peak radiation is inversely proportional to temperature. Newton's law of cooling: rate of cooling ∝ temperature difference with surroundings (for small differences).
State the first law of thermodynamics and give the sign convention.
ΔU = Q − W (or Q = ΔU + W). Q is positive when heat is added to the system; W is positive when work is done BY the system; ΔU is the change in internal energy.
State the second law of thermodynamics (Kelvin-Planck and Clausius statements).
Kelvin-Planck: no process can convert heat completely into work with no other effect. Clausius: heat cannot flow spontaneously from a colder to a hotter body. Both imply entropy of an isolated system never decreases.
Define the efficiency of a heat engine and a Carnot engine.
Engine efficiency η = W/Q₁ = 1 − Q₂/Q₁. Carnot (maximum) efficiency η = 1 − T₂/T₁, where T₁ is the source and T₂ the sink temperature (in kelvin). No engine can exceed Carnot efficiency.
State the postulates/assumptions of the kinetic theory of gases.
Gas molecules are point masses in random motion; collisions are perfectly elastic; no intermolecular forces except during collisions; time of collision is negligible; molecules obey Newton's laws; average KE depends only on absolute temperature.
Give the expression for pressure of a gas from kinetic theory and the relation between average KE and temperature.
P = (1/3)(mN/V)v̄² = (1/3)ρv_rms². Average translational KE per molecule = (3/2)kT, where k is Boltzmann's constant. v_rms = √(3RT/M).
State the law of equipartition of energy and degrees of freedom for monatomic and diatomic gases.
Each degree of freedom contributes ½kT of energy per molecule. Monatomic gas: 3 degrees of freedom (translational). Diatomic gas: 5 (3 translational + 2 rotational) at ordinary temperatures.
For an ideal gas, define Cp, Cv and give the ratio γ for monatomic and diatomic gases. State Mayer's relation.
Cp = molar heat at constant pressure, Cv = at constant volume. Mayer's relation: Cp − Cv = R. γ = Cp/Cv: monatomic γ = 5/3 ≈ 1.67; diatomic γ = 7/5 = 1.4.
Compare isothermal and adiabatic processes (condition, equation, work, internal energy).
Isothermal: T constant, PV = constant, ΔU = 0, Q = W. Adiabatic: Q = 0, PVγ = constant, W = −ΔU. Adiabatic curve is steeper than isothermal on a P-V diagram.
Define isochoric (isovolumetric) and isobaric processes and the work done in each.
Isochoric: volume constant, W = 0, so Q = ΔU. Isobaric: pressure constant, W = PΔV, so Q = ΔU + PΔV = nCpΔT.
Define simple harmonic motion and give its displacement, velocity, and acceleration equations.
SHM is motion where restoring force ∝ −displacement (a = −ω²x). x = A sin(ωt + φ); v = Aω cos(ωt + φ), v = ω√(A²−x²); a = −ω²x. Acceleration is maximum at extremes, velocity maximum at mean position.
Give the time period of a simple pendulum and a spring-mass system.
Simple pendulum: T = 2π√(L/g). Spring-mass system: T = 2π√(m/k), where k is the spring constant. Energy in SHM: E = ½kA² = ½mω²A² (constant).
Distinguish between transverse and longitudinal waves with examples.
Transverse: particle vibration perpendicular to wave propagation (e.g., light, waves on a string), has crests and troughs. Longitudinal: particle vibration parallel to propagation (e.g., sound in air), has compressions and rarefactions.
State the relation between wave speed, frequency, and wavelength, and give the speed of a wave on a stretched string.
v = fλ (or v = λ/T). On a stretched string: v = √(T/μ), where T is tension and μ is linear mass density (mass per unit length).
Explain standing waves: what are nodes and antinodes, and the fundamental frequency of a string fixed at both ends?
Standing waves form from superposition of two identical oppositely-moving waves. Nodes are points of zero amplitude; antinodes are points of maximum amplitude. Fundamental frequency f₁ = v/2L; harmonics are integer multiples f_n = nv/2L.
State the Doppler effect formula for sound when the source and observer move.
f' = f·(v ± v₀)/(v ∓ v_s), where v = speed of sound, v₀ = observer speed, v_s = source speed. Use top signs for relative approach (frequency increases) and bottom signs for recession (frequency decreases).
State Coulomb's law and define electric field intensity.
Coulomb's law: F = (1/4πε₀)·q₁q₂/r², with 1/4πε₀ = 9×10⁹ N·m²/C². Electric field E = F/q₀ (force per unit positive test charge); SI unit N/C or V/m; it is a vector pointing away from positive charge.
State Gauss's law and the field due to an infinite line charge and an infinite sheet of charge.
Gauss's law: net flux Φ = q_enc/ε₀. Infinite line charge: E = λ/(2πε₀r). Infinite charged sheet: E = σ/(2ε₀) (independent of distance).
Define electric potential and capacitance, and give the capacitance of a parallel plate capacitor.
Electric potential V = work per unit charge to bring a charge from infinity (V = W/q). Capacitance C = Q/V (unit: farad). Parallel plate capacitor: C = ε₀A/d (vacuum); with dielectric C = Kε₀A/d. Energy stored = ½CV².
State Ohm's law and give formulas for resistors in series and in parallel.
Ohm's law: V = IR (at constant temperature). Series: R_eq = R₁ + R₂ + ... Parallel: 1/R_eq = 1/R₁ + 1/R₂ + ... Resistance R = ρL/A, where ρ is resistivity.
State Kirchhoff's two laws for circuits.
Junction (current) rule: sum of currents entering a junction = sum leaving (conservation of charge, ΣI = 0). Loop (voltage) rule: sum of EMFs and potential drops around any closed loop = 0 (conservation of energy).
State the right-hand rule and Biot-Savart law for the magnetic field of a current. Give B at the center of a circular loop and inside a solenoid.
Biot-Savart: dB = (μ₀/4π)·(I dl × r̂)/r². At the center of a circular loop of radius R: B = μ₀I/2R. Inside a long solenoid: B = μ₀nI, where n is turns per unit length.
State Faraday's law and Lenz's law of electromagnetic induction.
Faraday's law: induced EMF = −dΦ/dt (rate of change of magnetic flux). For N turns, EMF = −N dΦ/dt. Lenz's law: the induced current opposes the change in flux that produces it (the negative sign), consistent with conservation of energy.
Define inductive and capacitive reactance, and impedance in a series LCR AC circuit. When does resonance occur?
X_L = ωL = 2πfL; X_C = 1/ωC = 1/2πfC. Impedance Z = √(R² + (X_L − X_C)²). Resonance occurs when X_L = X_C, giving f = 1/(2π√(LC)), minimum impedance Z = R and maximum current.
List the electromagnetic spectrum in order of increasing frequency and give the speed of EM waves.
Radio waves < microwaves < infrared < visible light < ultraviolet < X-rays < gamma rays (increasing frequency, decreasing wavelength). All travel at c = 3×10⁸ m/s in vacuum; c = 1/√(μ₀ε₀); E and B are perpendicular to each other and to propagation.
State the laws of reflection and the mirror formula with sign convention.
Laws of reflection: angle of incidence = angle of reflection; incident ray, reflected ray, and normal lie in one plane. Mirror formula: 1/v + 1/u = 1/f, where f = R/2. Magnification m = −v/u.
State Snell's law of refraction and the condition for total internal reflection.
Snell's law: n₁ sinθ₁ = n₂ sinθ₂ (n = refractive index). Total internal reflection occurs when light travels from a denser to a rarer medium at an angle greater than the critical angle θc, where sinθc = 1/n (= n_rarer/n_denser).
Give the lens formula, lensmaker's formula, and definition of power of a lens.
Lens formula: 1/v − 1/u = 1/f. Lensmaker's formula: 1/f = (n−1)(1/R₁ − 1/R₂). Power P = 1/f (in meters), unit dioptre (D). For lenses in contact: P = P₁ + P₂.
State the conditions for sustained interference and the fringe width formula in Young's double-slit experiment.
Conditions: the two sources must be coherent (constant phase difference) and monochromatic, with comparable amplitudes. Fringe width β = λD/d, where D = slit-to-screen distance and d = slit separation. Constructive: path difference = nλ; destructive = (n+½)λ.
Explain diffraction and the condition for the first minimum in single-slit diffraction.
Diffraction is the bending of waves around obstacles/edges and spreading after passing through a slit. For single-slit, the first minimum occurs when a·sinθ = λ (a = slit width). The central maximum is the brightest and twice as wide as the others.
What is Brewster's law / polarization by reflection?
When unpolarized light strikes a surface at Brewster's angle θ_p, the reflected light is completely plane-polarized. Brewster's law: tanθ_p = n (refractive index). At this angle, reflected and refracted rays are perpendicular.
State the photoelectric effect and Einstein's photoelectric equation.
Photoelectric effect: emission of electrons when light of sufficient frequency hits a metal. Einstein's equation: KE_max = hf − φ₀, where φ₀ = hf₀ is the work function and f₀ the threshold frequency. Below f₀ no emission occurs regardless of intensity; KE depends on frequency, not intensity.
State the de Broglie hypothesis and give the de Broglie wavelength formula.
Matter has wave nature: every moving particle has an associated wavelength λ = h/p = h/mv. For an electron accelerated through potential V: λ = 12.27/√V Å. This explains wave-particle duality.
State the postulates of Bohr's model and give the energy of the nth orbit in hydrogen.
Postulates: electrons orbit in stationary states without radiating; angular momentum is quantized (mvr = nh/2π); energy is emitted/absorbed only on jumping between orbits (hf = E₂ − E₁). Energy of nth level: Eₙ = −13.6/n² eV. Ground state = −13.6 eV.
Define mass defect, binding energy, and explain nuclear fission vs fusion.
Mass defect Δm = (mass of nucleons) − (mass of nucleus); binding energy = Δm·c² (energy holding the nucleus together). Fission: a heavy nucleus splits into lighter ones releasing energy. Fusion: light nuclei combine into a heavier one releasing energy. Both release energy because products have higher binding energy per nucleon.
State the law of radioactive decay and define half-life and the three types of radiation.
N = N₀e^(−λt), where λ is the decay constant. Half-life T½ = 0.693/λ (time for half the nuclei to decay). Alpha (²He⁴, positive, low penetration), beta (electron, moderate penetration), gamma (high-energy EM wave, high penetration, no charge).
Distinguish between intrinsic and extrinsic semiconductors, and between p-type and n-type.
Intrinsic: pure semiconductor (Si/Ge), equal electrons and holes. Extrinsic: doped semiconductor. n-type: doped with pentavalent impurity (e.g., As/P), majority carriers = electrons. p-type: doped with trivalent impurity (e.g., B/Al), majority carriers = holes.
Explain the behavior of a p-n junction diode in forward and reverse bias.
Forward bias (p to +, n to −): depletion layer narrows, diode conducts, low resistance. Reverse bias (p to −, n to +): depletion layer widens, only tiny leakage current flows (high resistance). A diode acts as a one-way valve / rectifier.
Compare half-wave and full-wave rectifiers and name the basic logic gates.
Half-wave rectifier uses one diode, converts only one half of the AC cycle (low efficiency). Full-wave rectifier (two diodes or a bridge of four) uses both halves (higher efficiency, ripple frequency = 2× input). Basic logic gates: OR, AND, NOT; universal gates: NAND and NOR.
AFMC / NEET-linked AFMC Admission Physics (NEET-UG Academic Component) FAQ
What is in the AFMC / NEET-linked AFMC Admission Physics (NEET-UG Academic Component) syllabus?
AFMC / NEET-linked AFMC Admission Physics (NEET-UG Academic Component) is split into 5 chapters: Mechanics, Thermodynamics and Kinetic Theory, Oscillations and Waves, Electrodynamics and Optics and Modern Physics. Together they contain 23 topics and 66 sub-topics.
How many chapters are in AFMC / NEET-linked AFMC Admission Physics (NEET-UG Academic Component)?
5 chapters, containing 23 topics and 66 sub-topics. The largest chapter is Mechanics, with 6 topics.
Are there flashcards for AFMC / NEET-linked AFMC Admission Physics (NEET-UG Academic Component)?
Yes — a 66-card Physics (NEET-UG Academic Component) 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.