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.
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
Formula
Condition or trap
Z = AᵖBᵠ/Cʳ gives ΔZ/Z = pΔA/A + qΔB/B + rΔC/C
Relative errors always add, even when quantities divide
Z = A ± B gives ΔZ = ΔA + ΔB
Absolute errors add, even for a difference
v = u + at, s = ut + ½at², v² = u² + 2as
Constant acceleration only
Distance in the nth second: sₙ = u + a(2n − 1)/2
Constant acceleration
Projectile: T = 2u sin θ/g, H = u² sin²θ/2g, R = u² sin 2θ/g
Level ground, no air resistance; R is greatest at 45°
Uniform circular motion: a = v²/r = ω²r
Directed towards the centre
Laws of motion, work, energy and power
Formula
Condition or trap
F = dp/dt; impulse = FΔt = Δp
Use Δp for collisions and catches
Static friction f ≤ μₛN; kinetic f = μₖN
Static friction adjusts up to its maximum
Apparent weight in a lift: m(g + a) when accelerating up, m(g − a) when accelerating down
Free 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/rg
The speed at which no friction is needed
W = Fs cos θ; W_net = ΔK
Work–energy theorem holds for all forces together
Spring energy ½kx²; P = Fv
x 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 rest
Velocities are exchanged
Rotational motion
Formula
Condition or trap
τ = r × F; τ = Iα; L = Iω
I depends on the axis
Ring MR²; disc ½MR²; solid sphere ⅖MR²; hollow sphere ⅔MR²; rod (centre) ML²/12
About the symmetry axis or diameter as usual
Parallel axes: I = I_cm + Md²
One axis must pass through the centre of mass
Perpendicular axes: I_z = I_x + I_y
Plane (flat) bodies only
I₁ω₁ = I₂ω₂
No external torque
Rotational KE = ½Iω²
Add ½Mv² of the centre of mass if it also translates
Gravitation
Formula
Condition or trap
g = GM/R²
At 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/r
Zero at infinity
Orbital speed v = √(GM/r) ≈ √(gR) near the surface
About 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/2r
KE = +GMm/2r
Solids, fluids and heat
Formula
Condition or trap
Y = (F/A)/(ΔL/L)
Within the elastic limit
P = P₀ + ρgh
Fluid at rest
A₁v₁ = A₂v₂; P + ½ρv² + ρgh = constant
Incompressible, 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/9η
Single slit minima a sin θ = nλ; central maximum 2λD/a wide
Here the condition gives dark bands, not bright
Malus I = I₀ cos²θ; Brewster tan θ_B = n
Unpolarised light through one polaroid: I₀/2
Modern physics and semiconductors
Formula
Condition or trap
K_max = hν − φ₀ = eV₀
Intensity changes current, not K_max
E (eV) ≈ 1240/λ (nm)
Photon energy
λ = h/p = h/√(2mK); electron λ ≈ 1.227/√V nm
V in volts
Eₙ = −13.6 Z²/n² eV; rₙ ∝ n²/Z
Hydrogen-like atoms
Lines from level n: n(n − 1)/2
Many atoms, all transitions
R = R₀A¹ᐟ³ (cube root of A), R₀ ≈ 1.2 fm
Nuclear density is the same for all nuclei
BE = Δm × 931.5 MeV (Δm in u)
BE per nucleon peaks near A = 56
ne × nh = nᵢ²
Thermal equilibrium
Full-wave output frequency = 2 × input
Half-wave: same as input
Quick self-test
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%
A satellite's orbital radius is doubled. Its orbital speed becomes: (a) 2 times (b) √2 times (c) 1/√2 times (d) ½
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
At resonance in a series LCR circuit, the impedance equals: (a) X_L (b) X_C (c) R (d) zero
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
A Carnot engine works between 500 K and 300 K. Its efficiency is: (a) 20% (b) 40% (c) 60% (d) 67%
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
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
(c) V ∝ r³, so 3 × 2% = 6%.
(c) v ∝ 1/√r.
(a) f = v/4L = 340/(4 × 0.5) = 170 Hz.
(c) X_L = X_C, so Z = R.
(a) P = +2 D, f = 1/2 m = 50 cm.
(b) 1 − 300/500 = 0.4.
(b) λ becomes λ/n, so β becomes 3β/4.
(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.
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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