Fundamentals

1,200 must-knows for NEET & JEE

The core facts every aspirant should own — each a titled nugget with a real-world story, the concept in plain words, and a memory trick. Works even when the internet doesn't.

1,200 fundamentals

PhysicsMagnetism & Electromagnetic Induction· Class 12

Myth: Magnetic force does work

Every power plant on Earth spins a magnet to make your electricity — Faraday's idea, scaled up.

It is always perpendicular to velocity, so it can never change a charge's speed or energy.

PhysicsModern Physics· Class 12

Photoelectric effect — common mistake

The solar panel and the smoke detector both run on Einstein-era quantum physics.

A frequent error is thinking very bright low-frequency light can eject electrons. In reality, light ejects electrons from a metal only if its frequency exceeds a threshold, regardless of intensity.

Memory trick: frequency decides IF electrons come out; intensity only decides HOW MANY.

PhysicsModern Physics· Class 12

Photon energy — common mistake

The solar panel and the smoke detector both run on Einstein-era quantum physics.

A frequent error is treating light purely as a wave when explaining the photoelectric effect. In reality, light comes in packets of energy E = hf = hc/λ.

Memory trick: higher frequency (bluer light) means more energetic photons.

PhysicsModern Physics· Class 12

Bohr model — common mistake

The solar panel and the smoke detector both run on Einstein-era quantum physics.

A frequent error is using a positive energy for a bound electron — bound states are negative. In reality, electrons occupy quantised orbits; for hydrogen E_n = −13.6/n² eV.

Memory trick: the electron is most tightly bound (most negative) in n=1.

PhysicsModern Physics· Class 12

Mass–energy and binding energy

The solar panel and the smoke detector both run on Einstein-era quantum physics.

A nucleus weighs less than its parts; the missing mass becomes binding energy via E = Δmc².

Memory trick: fusion and fission both release the difference in binding energy.

PhysicsModern Physics· Class 12

Mass–energy and binding energy — common mistake

The solar panel and the smoke detector both run on Einstein-era quantum physics.

A frequent error is ignoring the mass defect when computing nuclear energy. In reality, a nucleus weighs less than its parts; the missing mass becomes binding energy via E = Δmc².

Memory trick: fusion and fission both release the difference in binding energy.

PhysicsModern Physics· Class 12

de Broglie wavelength — common mistake

The solar panel and the smoke detector both run on Einstein-era quantum physics.

A frequent error is expecting everyday objects to show wave behaviour (their λ is unimaginably small). In reality, every particle has a wavelength λ = h/p, significant only for tiny masses.

Memory trick: matter waves matter only at the electron/atom scale.

PhysicsModern Physics· Class 12

E = hf = hc/λ

The solar panel and the smoke detector both run on Einstein-era quantum physics.

Energy of a photon. Use it when electromagnetic radiation of frequency f.

E = hf = hc/λ

PhysicsModern Physics· Class 12

E_n = −13.6/n² eV

The solar panel and the smoke detector both run on Einstein-era quantum physics.

Energy of the nth hydrogen level. Use it when hydrogen atom (Bohr model).

E_n = −13.6/n² eV

PhysicsModern Physics· Class 12

E = Δmc²

The solar panel and the smoke detector both run on Einstein-era quantum physics.

Energy equivalent of a mass defect. Use it when nuclear reactions.

E = Δmc²

PhysicsModern Physics· Class 12

λ = h/p

The solar panel and the smoke detector both run on Einstein-era quantum physics.

De Broglie wavelength of a particle. Use it when particle with momentum p.

λ = h/p

PhysicsModern Physics· Class 12

nuclear fission vs nuclear fusion

The solar panel and the smoke detector both run on Einstein-era quantum physics.

Fission splits a heavy nucleus into lighter ones (reactors); fusion joins light nuclei into a heavier one (the Sun) — both release energy.

ChemistrySome Basic Concepts (Mole Concept)· Class 11

Avogadro's number

It's such a huge number that a mole of rice grains would cover Earth metres deep.

One mole of any substance contains 6.022×10²³ particles.

N_A = 6.022×10²³

Memory trick: Mole = chemistry's 'dozen'.

ChemistrySome Basic Concepts (Mole Concept)· Class 11

Molar mass

18 g of water is exactly one mole — about a mouthful.

The mass of one mole of a substance in grams, equal to its atomic/molecular mass.

n = m/M

Memory trick: moles = mass ÷ molar mass.

ChemistrySome Basic Concepts (Mole Concept)· Class 11

Empirical vs molecular formula

Glucose and formaldehyde share the empirical formula CH₂O but are wildly different molecules.

Empirical is the simplest whole-number atom ratio (CH₂O); molecular is the actual count (C₆H₁₂O₆).

Memory trick: Molecular = whole-number multiple of empirical.

ChemistrySome Basic Concepts (Mole Concept)· Class 11

Molarity

A doctor's saline drip is dosed precisely in molarity.

Concentration as moles of solute per litre of solution.

M = n/V

Memory trick: Molarity = moles ÷ litres.

ChemistrySome Basic Concepts (Mole Concept)· Class 11

Limiting reagent

In a sandwich with 10 slices of bread but 4 fillings, the filling is the limiting reagent.

The reactant that runs out first and caps how much product forms.

Memory trick: Convert to moles, then compare.

ChemistryStructure of Atom· Class 11

Subatomic particles

The nucleus is a fly in a stadium — atoms are almost entirely empty space.

Atoms contain protons (+), neutrons (0) in the nucleus and electrons (−) around it.

Memory trick: Protons define the element.

ChemistryStructure of Atom· Class 11

Atomic number vs mass number

Change the neutrons and you get an isotope; change the protons and you get a new element.

Atomic number = protons; mass number = protons + neutrons.

A = Z + N

Memory trick: Z = protons; A = protons + neutrons.

ChemistryStructure of Atom· Class 11

Isotopes

Carbon-12 and carbon-14 are chemically identical twins with different weights.

Atoms of the same element with different numbers of neutrons.

Memory trick: Same protons, different neutrons.

ChemistryStructure of Atom· Class 11

Quantum numbers

They're the unique 'postal address' of every electron in an atom.

Four numbers (n, l, m, s) fix an electron's shell, subshell, orbital and spin.

Memory trick: n=floor, l=room type, m=room, s=spin.

ChemistryStructure of Atom· Class 11

Aufbau principle

Like people filling a cinema from the front rows, electrons take the cheapest seats first.

Electrons fill the lowest-energy orbitals first.

Memory trick: Fill low energy before high.

ChemistryStructure of Atom· Class 11

Pauli exclusion principle

Two electrons can share a room only if they spin opposite ways.

No two electrons in an atom can have all four quantum numbers identical; an orbital holds at most two, with opposite spins.

Memory trick: Max 2 per orbital, opposite spins.

ChemistryStructure of Atom· Class 11

Hund's rule

Passengers take empty double-seats alone before doubling up.

Electrons singly occupy each orbital of a subshell before pairing, with parallel spins.

Memory trick: Fill singly first, same spin.

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