WHY these two? Ingredient 1 pure classical physics hai (jo electron ko circling rakhta hai). Ingredient 2 woh naya quantum rule hai jo Bohr ne bolt on kiya — taaki electron nucleus mein spiral karke na gire aur sharp spectral lines explain ho sakein.
Step 1 — Simplify Coulomb = centripetal. Dono sides ko r se multiply karo:
\frac{1}{4\pi\varepsilon_0}\frac{Ze^2}{r} = m v^2 \tag{A}Why this step? Hume r aur v ke beech ek aisa relation chahiye jo quantization ke saath combine ho sake.
Step 2 — Get v from quantization.mvr=2πnh se:
v = \frac{nh}{2\pi m r} \tag{B}Why this step? Quantization rule woh ek maatra extra information hai jo r ki value pin down karega.
Step 3 — Substitute (B) into (A).4πε01rZe2=m(2πmrnh)2=4π2mr2n2h2Why this step?v ko khatam karo taaki sirf r bache.
Step 4 — Solve for r. Ek r cancel karo aur rearrange karo:
4πε0Ze2=4π2mrn2h2⇒r=πmZe2ε0n2h2
Read it off: radius ==n2== ke saath badhti hai aur Z badhne par ghatti hai (bada nuclear charge electron ko aur kareeb kheench leta hai).
Step 2 — Use (A) to relate KE and PE. (A) se, mv2=4πε01rZe2, toh
KE=21mv2=21⋅4πε01rZe2=−21PEWhy this step? Yeh 1/r force ke liye virial result hai — yeh humein sab kuch PE ke terms mein likhne deta hai.
Step 3 — Total energy.E=KE+PE=−21PE+PE=21PE=−21⋅4πε01rZe2E=−8πε0rZe2Why this step? Energy potential energy ki half hai — aur yeh negative hai, matlab electron bound hai.
Step 4 — Plug in rn.rn=πmZe2ε0n2h2 substitute karo:
En=−8πε0Ze2⋅ε0n2h2πmZe2=−8ε02n2h2mZ2e4
Read it off: energy negative hai (bound), ==Z2/n2== ke saath scale karti hai, aur n badhne par 0 ke kareeb aati jaati hai (kam bound hoti hai).
Socho ek ball ek string par hai jise tum apne sir ke upar ghuma rahe ho. String ki pull use circling rakhti hai — atom mein woh "string" hai tiny positive middle (nucleus) ka electron par electric attraction. Lekin nature ka ek ajeeb rule hai: electron sirf kuch special sizes par hi ghoom sakta hai, jaise staircase ke steps, beech mein kabhi nahi. Sirf in do facts se — "pull equals whirl-force" aur "only special step-sizes allowed hain" — tum exactly calculate kar sakte ho ki har orbit kitni badi hai aur usme kitni energy hai. Bas yahi Bohr ne kiya tha.