Edumath by Sereddy logo

Physics Formula Sheet: What to Memorise vs What to Derive

16 August 2026 · Yesunadhareddy SereddyClass 11 PhysicsClass 12 PhysicsJEE PrepNEET Prep

A standard Class 11–12 Physics syllabus contains well over 400 formulas across Mechanics, Electromagnetism, Optics, Thermodynamics, and Modern Physics. Attempting to brute-force memorise every variation leads to formula confusion during high-pressure exams like JEE Main, NEET, and Board assessments.

Conversely, attempting to derive everything from first principles drains your exam clock. The secret to scoring consistently lies in categorising formulas into three distinct tiers: absolute fundamentals to memorise, high-frequency results to internalise, and situational expressions to derive on the spot.

The 3-Tier Formula Framework

To build a streamlined formula sheet under the NCERT/NCF-SE curriculum, classify every relation you encounter into one of three buckets.

+-------------------------------------------------------------+
| Tier 1: Non-negotiable Core Laws (Memorise directly)        |
+-------------------------------------------------------------+
| Tier 2: High-Frequency Operational Results (Memorise limits)|
+-------------------------------------------------------------+
| Tier 3: Case-Specific Variants (Derive in 15-30 seconds)   |
+-------------------------------------------------------------+

Tier 1: Non-Negotiable Core Laws (Memorise)

These are fundamental definitions, empirical laws, and conservation principles. They cannot be derived from simpler high-school mechanics or electromagnetism equations.

  • Mechanics: Newton's Laws (F=dpdtF = \frac{dp}{dt}), Work-Energy Theorem (Wnet=ΔKW_{\text{net}} = \Delta K), Impulse definition (J=FdtJ = \int F \, dt).
  • Thermodynamics: First Law (ΔQ=ΔU+W\Delta Q = \Delta U + W), Ideal Gas Equation (PV=nRTPV = nRT), Relation CpCv=RC_p - C_v = R.
  • Electromagnetism: Coulomb's Law, Gauss's Law (EdA=qenclε0\oint \vec{E} \cdot d\vec{A} = \frac{q_{\text{encl}}}{\varepsilon_0}), Biot-Savart Law, Faraday's Law (E=dΦBdt\mathcal{E} = -\frac{d\Phi_B}{dt}).
  • Modern Physics: Einstein’s photoelectric equation (Kmax=hνΦK_{\text{max}} = h\nu - \Phi), de Broglie relation (λ=hp\lambda = \frac{h}{p}).

Tier 2: High-Yield Shortcuts (Memorise with Boundary Conditions)

These are standard derivations that appear repeatedly in numerical problems. You must memorise them, but always alongside their validity conditions.

  • Projectiles: Range R=u2sin2θgR = \frac{u^2 \sin 2\theta}{g} (Valid only for flat, horizontal ground).
  • SHM: Time period of a simple pendulum T=2πLgT = 2\pi\sqrt{\frac{L}{g}} (Valid only for small angular amplitudes, θ5\theta \le 5^\circ).
  • Electrostatics: Electric field on the axial line of a short dipole Eaxial=2kpr3E_{\text{axial}} = \frac{2kp}{r^3} and equatorial line Eeq=kpr3E_{\text{eq}} = \frac{kp}{r^3} (Valid only when rar \gg a).
  • Capacitance: Energy density uE=12ε0E2u_E = \frac{1}{2}\varepsilon_0 E^2.

Tier 3: Case-Specific Variants (Derive on the Fly)

These equations make formula sheets unnecessarily bulky. Memorising them increases your risk of sign-error traps. You should derive them during problem-solving using basic Tier 1 relations.

  • Banking of roads with friction: Start from free-body force resolution rather than mugging up tan(θ±ϕ)\tan(\theta \pm \phi) permutations.
  • Terminal velocity: Derive by balancing forces (Fg=Fb+FvF_g = F_b + F_v) using Stokes' Law (6πηrvt6\pi\eta r v_t).
  • Magnetic field at the centre of an arc: Start from Biot-Savart's B=μ0I4πrθB = \frac{\mu_0 I}{4\pi r} \theta, where θ\theta is in radians.
  • Equivalent focal length of separated lenses: Derive using step-by-step refraction instead of memorising multiple sign-heavy equations.

Decision Matrix: Memorise vs Derive

| Unit | Memorise Directly | Derive on the Fly | Why? | | :--- | :--- | :--- | :--- | | Mechanics | v2=u2+2asv^2 = u^2 + 2as, Iring=MR2I_{\text{ring}} = MR^2, Idisc=12MR2I_{\text{disc}} = \frac{1}{2}MR^2 | Moment of inertia of cutouts, composite bodies | Standard axes are base units; composite shapes use parallel/perpendicular axis theorems. | | Gravitation | g(h)=g(12hR)g(h) = g\left(1 - \frac{2h}{R}\right) for hRh \ll R | Escape velocity from a given height or planetary depth | Energy conservation (Ui+Ki=Uf+KfU_i + K_i = U_f + K_f) is faster and less prone to power-of-radius errors. | | Current Electricity | I=neAvdI = n e A v_d, V=IRV = IR, ΔVloop=0\Delta V_{\text{loop}} = 0 | Meter bridge / Potentiometer balancing lengths | Memorising specific wire resistance proportions creates confusion if the circuit adds shunts. | | Ray Optics | Lens Maker's Formula: 1f=(μ1)(1R11R2)\frac{1}{f} = (\mu - 1)\left(\frac{1}{R_1} - \frac{1}{R_2}\right) | Silvered lens combinations (Peq=2PL+PMP_{\text{eq}} = 2P_L + P_M) | Silvering questions frequently change medium; power summation (ΣP\Sigma P) prevents sign errors. | | Wave Optics | Fringe width β=λDd\beta = \frac{\lambda D}{d} | Path difference with thin glass slab Δx=(μ1)tDd\Delta x = \frac{(\mu - 1)t D}{d} | Slab insertion questions vary (single vs double slit); build from Δx=(μ1)t\Delta x = (\mu - 1)t. |


How to Test if a Formula Belongs on Your Sheet

When making your revision notes for Board exams or competitive tests:

  1. Dimensional Consistency Check: Can you extract the formula's units instantly? If an expression looks complex (like the velocity of a transverse wave on a string, v=T/μv = \sqrt{T/\mu}), check whether you can quickly verify it via dimensional analysis.
  2. The 30-Second Rule: If a formula takes longer than 30 seconds to derive from a primary law, memorise it as a Tier-2 standard result. If it takes under 15 seconds (e.g., maximum height of a projectile H=uy22gH = \frac{u_y^2}{2g} from vy2=uy22gHv_y^2 = u_y^2 - 2gH), derive it.
  3. Limiting Cases: Whenever you write down a memorised formula, write its boundary condition next to it in red ink. For example, alongside the Doppler effect formula for sound, note down that it applies only when medium velocity is zero and speeds are sub-sonic.

Quick Checklist for Your Revision Sheet

  • [ ] Every Tier-1 fundamental law is present with standard SI units and vector notation where applicable.
  • [ ] Boundary limits (e.g., rar \gg a, small θ\theta, non-relativistic speeds) are written next to Tier-2 shortcuts.
  • [ ] Long derivations from Boards (e.g., electric field due to a uniformly charged spherical shell) are condensed into a 2-line step: Gauss's Law \to Symmetry Argument \to Result.
  • [ ] You have eliminated duplicate algebraic rearrangements (e.g., write only v=fλv = f\lambda, not three separate lines for ff, λ\lambda, and TT).
  • [ ] Constants like ε0\varepsilon_0, μ0\mu_0, hh, kBk_B, and RR have their values and derived units double-checked.