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NEET physics formula sheet, with the conditions that matter

Every key physics formula for NEET, unit by unit, with the condition each one needs and the traps attached to it. Use it for the final revision pass, then test yourself with the quick quiz at the end.

11 Oct 2026 11 min read

In this guide
  1. How to use this sheet
  2. Units, measurement and kinematics
  3. Laws of motion, work, energy and power
  4. Rotational motion
  5. Gravitation
  6. Solids, fluids and heat
  7. Thermodynamics and kinetic theory
  8. Oscillations and waves
  9. Electrostatics and current electricity
  10. Magnetism, EMI and AC
  11. Optics
  12. Modern physics and semiconductors
  13. Quick self-test
  14. What to do next

A formula sheet is only useful if it tells you when each formula works. Most wrong answers in NEET physics come from a correct formula used in the wrong situation: an equation of motion with changing acceleration, the small-height gravity approximation at a large height, or a series rule applied to capacitors in parallel.

So this sheet lists each formula with its condition or its trap. Read it once a week in the last three months, and daily in the last fortnight. It is a revision tool, not a first reading: if a line here makes no sense, go back to that chapter's guide.

How to use this sheet

  • Cover the right-hand column and say the condition aloud before you check it.
  • Mark the lines you hesitate on, and copy only those to a short personal sheet.
  • Pair each line with one question. A formula you have used in a numerical this week is a formula you will remember in the hall.

Units, measurement and kinematics

FormulaCondition or trap
Z = AᵖBᵠ/Cʳ gives ΔZ/Z = pΔA/A + qΔB/B + rΔC/CRelative errors always add, even when quantities divide
Z = A ± B gives ΔZ = ΔA + ΔBAbsolute errors add, even for a difference
v = u + at, s = ut + ½at², v² = u² + 2asConstant acceleration only
Distance in the nth second: sₙ = u + a(2n − 1)/2Constant acceleration
Projectile: T = 2u sin θ/g, H = u² sin²θ/2g, R = u² sin 2θ/gLevel ground, no air resistance; R is greatest at 45°
Uniform circular motion: a = v²/r = ω²rDirected towards the centre

Laws of motion, work, energy and power

FormulaCondition or trap
F = dp/dt; impulse = FΔt = ΔpUse Δp for collisions and catches
Static friction f ≤ μₛN; kinetic f = μₖNStatic friction adjusts up to its maximum
Apparent weight in a lift: m(g + a) when accelerating up, m(g − a) when accelerating downFree fall: apparent weight is zero
Safe speed on a flat curve: v = √(μrg)Friction supplies the centripetal force
Banked road without friction: tan θ = v²/rgThe speed at which no friction is needed
W = Fs cos θ; W_net = ΔKWork–energy theorem holds for all forces together
Spring energy ½kx²; P = Fvx is measured from the natural length
Vertical circle: v at top ≥ √(gr); v at bottom ≥ √(5gr)For a string, to complete the circle
Perfectly inelastic: v = (m₁u₁ + m₂u₂)/(m₁ + m₂)KE is lost; momentum is conserved
Elastic, equal masses, one at restVelocities are exchanged

Rotational motion

FormulaCondition or trap
τ = r × F; τ = Iα; L = IωI depends on the axis
Ring MR²; disc ½MR²; solid sphere ⅖MR²; hollow sphere ⅔MR²; rod (centre) ML²/12About the symmetry axis or diameter as usual
Parallel axes: I = I_cm + Md²One axis must pass through the centre of mass
Perpendicular axes: I_z = I_x + I_yPlane (flat) bodies only
I₁ω₁ = I₂ω₂No external torque
Rotational KE = ½Iω²Add ½Mv² of the centre of mass if it also translates

Gravitation

FormulaCondition or trap
g = GM/R²At the surface
g(h) = gR²/(R + h)² ≈ g(1 − 2h/R)The approximation needs h ≪ R
g(d) = g(1 − d/R)Uniform Earth; g = 0 at the centre
U = −GMm/rZero at infinity
Orbital speed v = √(GM/r) ≈ √(gR) near the surfaceAbout 7.9 km/s close to Earth
Escape speed v_e = √(2GM/R) = √(2gR)About 11.2 km/s; independent of the mass launched
T² ∝ r³ (T = 2π√(r³/GM))Kepler's third law
Total energy of a satellite = −GMm/2rKE = +GMm/2r

Solids, fluids and heat

FormulaCondition or trap
Y = (F/A)/(ΔL/L)Within the elastic limit
P = P₀ + ρghFluid at rest
A₁v₁ = A₂v₂; P + ½ρv² + ρgh = constantIncompressible, non-viscous, steady flow along a streamline
Torricelli: v = √(2gh)Speed of efflux from depth h
Stokes: F = 6πηrv; terminal speed v = 2r²(ρ − σ)g/9ηSmall sphere, slow flow
Excess pressure: drop 2T/r, soap bubble 4T/rA bubble has two surfaces
Capillary rise h = 2T cos θ/rρgFalls (h < 0) when θ > 90°, as with mercury
ΔL = LαΔT; β = 2α; γ = 3αIsotropic solids
Q = mcΔT; Q = mLNo temperature change during a change of state
Conduction H = kAΔT/L; radiation H = eσAT⁴T in kelvin for radiation
Wien: λ_m T = constant; Newton's cooling: rate ∝ (T − Tₛ)Newton's law for small temperature differences

Thermodynamics and kinetic theory

FormulaCondition or trap
ΔQ = ΔU + ΔWΔW is work done by the gas (physics convention)
Isobaric W = PΔV; isochoric W = 0Work is the area under the P–V curve
Isothermal W = nRT ln(V₂/V₁); ΔU = 0Ideal gas
Adiabatic PVᵞ = constant; W = nR(T₁ − T₂)/(γ − 1)Q = 0
Cp − Cv = R; γ = 5/3 (monatomic), 7/5 (diatomic)Per mole, ideal gas
Carnot efficiency η = 1 − T₂/T₁T in kelvin; the upper limit for any engine between T₁ and T₂
v_rms = √(3RT/M)M in kg mol⁻¹
Mean KE per molecule = (3/2)kTTranslational only
Equipartition: ½kT per degree of freedomDiatomic gas at room temperature: 5 degrees

Oscillations and waves

FormulaCondition or trap
x = A sin(ωt + φ); v = ω√(A² − x²); a = −ω²xSHM only
Total energy ½kA² = ½mω²A²Constant; KE and PE trade places
Spring T = 2π√(m/k); pendulum T = 2π√(l/g)Pendulum: small angles
v = fλ; string v = √(T/μ)μ is mass per unit length
Speed of sound v = √(γP/ρ)Laplace's correction
String fixed at both ends or open pipe: fₙ = nv/2LAll harmonics
Closed pipe: f = (2n − 1)v/4LOdd harmonics only
Beats = f₁ − f₂Small frequency difference

Electrostatics and current electricity

FormulaCondition or trap
F = kq₁q₂/r², k = 9 × 10⁹ N m² C⁻²Point charges
Dipole field: axial 2kp/r³, equatorial kp/r³r much larger than the dipole length
Torque on a dipole τ = pE sin θNet force is zero in a uniform field
Gauss: flux = q_enclosed/ε₀Only enclosed charge counts
Line charge λ/2πε₀r; sheet σ/2ε₀Infinite line or sheet
C = ε₀A/d; with dielectric KCParallel plates
U = ½CV² = Q²/2CSeries: 1/C = ∑1/Cᵢ; parallel: C = ∑Cᵢ
I = neAv_d; R = ρl/AStretching a wire keeps its volume fixed
V = E − Ir (discharging); V = E + Ir (charging)Internal resistance r
Wheatstone balance: P/Q = R/SNo current through the galvanometer
P = VI = I²R = V²/RUse I²R for series, V²/R for parallel comparisons

Magnetism, EMI and AC

FormulaCondition or trap
Long straight wire B = μ₀I/2πr; loop centre μ₀I/2R; solenoid μ₀nISolenoid: long, field inside
F = qvB sin θ; r = mv/qB; T = 2πm/qBT does not depend on speed
Force on a wire F = BIl sin θ; between wires μ₀I₁I₂/2πd per metreLike currents attract
Torque on a coil τ = NIAB sin θθ is between the field and the coil's normal
Ammeter shunt S = I_g G/(I − I_g); voltmeter series R = V/I_g − GShunt is small and in parallel; the voltmeter resistor is large and in series
e = −dΦ/dt; motional e = BlvLenz's law gives the minus sign
Inductor energy ½LI²Stored in the magnetic field
V_rms = V₀/√2; X_L = ωL; X_C = 1/ωCSinusoidal AC; X_C falls as frequency rises
Z = √[R² + (X_L − X_C)²]; resonance ω₀ = 1/√(LC)At resonance Z = R, current is greatest
P = V_rms I_rms cos φ; cos φ = R/ZPure L or C: power is zero
Transformer V_s/V_p = N_s/N_p = I_p/I_sIdeal transformer
EM waves: c = 1/√(μ₀ε₀); E₀ = cB₀E and B are in phase and perpendicular

Optics

FormulaCondition or trap
Mirror 1/v + 1/u = 1/f; f = R/2; m = −v/uCartesian signs
Lens 1/v − 1/u = 1/f; m = v/uConcave lens f is negative
Lens maker: 1/f = (n − 1)(1/R₁ − 1/R₂)Thin lens; n relative to the surroundings
P = 1/f (f in metres); P = P₁ + P₂Thin lenses in contact
Critical angle sin C = 1/nLight going from denser to rarer
Prism n = sin[(A + D_m)/2]/sin(A/2); thin prism δ = (n − 1)AMinimum deviation: the ray passes symmetrically
Apparent depth = real depth/nViewed from above, near normal
YDSE fringe width β = λD/dIn a medium, λ becomes λ/n
Single slit minima a sin θ = nλ; central maximum 2λD/a wideHere the condition gives dark bands, not bright
Malus I = I₀ cos²θ; Brewster tan θ_B = nUnpolarised light through one polaroid: I₀/2

Modern physics and semiconductors

FormulaCondition or trap
K_max = hν − φ₀ = eV₀Intensity changes current, not K_max
E (eV) ≈ 1240/λ (nm)Photon energy
λ = h/p = h/√(2mK); electron λ ≈ 1.227/√V nmV in volts
Eₙ = −13.6 Z²/n² eV; rₙ ∝ n²/ZHydrogen-like atoms
Lines from level n: n(n − 1)/2Many atoms, all transitions
R = R₀A¹ᐟ³ (cube root of A), R₀ ≈ 1.2 fmNuclear density is the same for all nuclei
BE = Δm × 931.5 MeV (Δm in u)BE per nucleon peaks near A = 56
ne × nh = nᵢ²Thermal equilibrium
Full-wave output frequency = 2 × inputHalf-wave: same as input

Quick self-test

  1. The percentage error in the radius of a sphere is 2%. The percentage error in its volume is: (a) 2% (b) 4% (c) 6% (d) 8%
  2. A satellite's orbital radius is doubled. Its orbital speed becomes: (a) 2 times (b) √2 times (c) 1/√2 times (d) ½
  3. A closed pipe 50 cm long, with sound at 340 m/s, has a fundamental frequency of: (a) 170 Hz (b) 340 Hz (c) 680 Hz (d) 85 Hz
  4. At resonance in a series LCR circuit, the impedance equals: (a) X_L (b) X_C (c) R (d) zero
  5. Two thin lenses of power +5 D and −3 D are in contact. The combined focal length is: (a) 50 cm (b) 20 cm (c) 12.5 cm (d) 2 m
  6. A Carnot engine works between 500 K and 300 K. Its efficiency is: (a) 20% (b) 40% (c) 60% (d) 67%
  7. In YDSE, the whole set-up is dipped in water (n = 4/3). The fringe width: (a) becomes 4/3 times (b) becomes 3/4 times (c) is unchanged (d) becomes zero
  8. The rms voltage of a 311 V peak AC supply is about: (a) 155 V (b) 220 V (c) 311 V (d) 440 V

Answers

  1. (c) V ∝ r³, so 3 × 2% = 6%.
  2. (c) v ∝ 1/√r.
  3. (a) f = v/4L = 340/(4 × 0.5) = 170 Hz.
  4. (c) X_L = X_C, so Z = R.
  5. (a) P = +2 D, f = 1/2 m = 50 cm.
  6. (b) 1 − 300/500 = 0.4.
  7. (b) λ becomes λ/n, so β becomes 3β/4.
  8. (b) 311/√2 ≈ 220 V.

What to do next

  • Cover the right-hand column of one table a day and recite the conditions.
  • Copy every line you missed onto one personal page. That page is your last-week sheet.
  • Pair this sheet with solving physics numericals faster and common physics mistakes, then move to chemistry with the NEET chemistry plan.

A note on dates and numbers. Exam patterns, vacancies and schedules change from year to year. Always confirm the current details in the latest notification on the National Testing Agency website .

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