1.2.7 · Chemistry › Atomic Structure (Classical)
Intuition The big picture
Electron ek chhoti si negative charge hai jo positive nucleus ke around ghoomti hai. Agar classical physics ko akele chhod do, toh yeh andar ki taraf spiral karke crash kar jaati. Bohr ka fix yeh tha: electron sirf kuch special circular tracks par hi rehne ki IJAZAT hai — jaise stairs hote hain, ramp nahi. Un tracks par yeh radiate nahi karta. Har track ka ek fixed radius aur fixed energy hoti hai. Sirf yeh ek "allowed tracks only" rule explain karta hai ki hydrogen sharp coloured lines mein kyun chamakta hai, na ki ek continuous smear mein.
Definition Bohr's postulates
Circular orbits: Electron nucleus ke around ek circle mein move karta hai, jo Coulomb (electrostatic) attraction se hold hota hai, jo centripetal force provide karta hai.
Quantised angular momentum: Sirf woh orbits allowed hain jahan angular momentum ℏ ka whole-number multiple ho:
m v r = n ℏ = 2 π nh , n = 1 , 2 , 3 , …
Stationary states / quantum jumps: Allowed orbit mein electron energy radiate nahi karta . Yeh photon tabhi emit ya absorb karta hai jab orbits ke beech jump karta hai: Δ E = h ν .
YEH KYUN? Postulate 3 atom ko classical collapse se bachata hai (ek accelerating charge ko radiate karna chahiye — Bohr sirf allowed orbits mein ise forbid kar deta hai). Postulate 2 woh quantisation seed hai jo energies ko discrete banata hai → discrete spectral lines.
Step 1 — Force balance. Coulomb attraction = centripetal force.
4 π ε 0 1 r 2 ( Z e ) ( e ) = r m v 2
Yeh step kyun? Electron fly off nahi karta, toh inward electric pull mass×centripetal-acceleration ke barabar honi chahiye jo ise circling mein rakhe. Nuclear charge + Z e hai, electron − e hai.
Simplify karo (ek r cancel karo):
\frac{kZe^2}{r} = mv^2, \qquad k=\frac{1}{4\pi\varepsilon_0} \tag{1}
Step 2 — Quantisation. Postulate 2 se, v = 2 π m r nh .
Yeh step kyun? Hamare paas do unknowns v aur r hain; quantisation condition woh doosri equation deti hai jo humein chahiye.
Step 3 — Substitute v ko (1) mein:
r k Z e 2 = m ( 2 π m r nh ) 2 = 4 π 2 m r 2 n 2 h 2
Dono sides ko r 2 se multiply karo aur k Z e 2 se divide karo:
r n = 4 π 2 mk Z e 2 n 2 h 2 = π m Z e 2 ε 0 n 2 h 2
Step 4 — Numbers plug karo (n = 1 , Z = 1 ke liye): n 2 / Z ko chhod kar baaki sab ek constants ka bundle hai jo 0.529 × 1 0 − 10 m evaluate karta hai.
Step 1 — Total energy = kinetic + potential.
E = K E 2 1 m v 2 + P E ( − r k Z e 2 )
Yeh step kyun? PE negative hai kyunki attraction energy ko lower karta hai (bound = ek well mein trapped).
Step 2 — (1) use karo: m v 2 = r k Z e 2 , toh K E = 2 r k Z e 2 .
E = \frac{kZe^2}{2r} - \frac{kZe^2}{r} = -\frac{kZe^2}{2r} \tag{2}
Yeh step kyun? Notice karo E = − K E = 2 1 P E — yeh inverse-square force ki ek pehchaan hai (virial theorem ). Total energy negative hai → electron bound hai.
Step 3 — r n insert karo:
E n = − 2 k Z e 2 ⋅ n 2 h 2 4 π 2 mk Z e 2 = − n 2 h 2 2 π 2 m k 2 Z 2 e 4
Constants ka bundle 13.6 eV evaluate karta hai.
n 2 → n 1 jump (n 2 > n 1 ke saath) ek photon emit karta hai:
Δ E = E n 2 − E n 1 = 13.6 Z 2 ( n 1 2 1 − n 2 2 1 ) eV
ν ˉ = λ 1 = R H Z 2 ( n 1 2 1 − n 2 2 1 ) , R H = 1.097 × 1 0 7 m − 1
Kyunki n discrete hai, sirf certain Δ E exist karte hain → sharp lines (Lyman n 1 = 1 , Balmer n 1 = 2 , etc.).
Worked example 1. Li²⁺ ke 3rd orbit ka radius
Z = 3 , n = 3 : r 3 = 0.529 ⋅ 3 3 2 = 0.529 × 3 = 1.587 Å.
Kyun? n 2 / Z = 9/3 = 3 use karo. Note karo yeh Bohr radius ka 3 guna hai, bhaari ion hone ke bawajood.
Worked example 2. He⁺ ke 2nd orbit ki energy
Z = 2 , n = 2 : E 2 = − 13.6 ⋅ 4 4 = − 13.6 eV.
Kyun? Z 2 / n 2 = 4/4 = 1 . Interesting: He⁺ (n = 2 ) ki energy H (n = 1 ) ke SAME hai kyunki Z 2 boost n 2 spreading ko cancel kar deta hai.
Worked example 3. H Balmer-α line (
n 2 = 3 → n 1 = 2 ) ki wavelength
ν ˉ = 1.097 × 1 0 7 ( 1/4 − 1/9 ) = 1.097 × 1 0 7 × 0.1389 = 1.524 × 1 0 6 m − 1 .
λ = 1/ ν ˉ = 6.56 × 1 0 − 7 m = 656 nm (red).
Kyun? 1/4 − 1/9 = ( 9 − 4 ) /36 = 5/36 . Yeh famous red hydrogen line se match karta hai — evidence ki Bohr sahi tha.
n badhne ke saath increase hoti hai, toh yeh zyada positive aur badi ho jaati hai."
Kyun sahi lagta hai: higher orbit = zyada energy, toh "bada number." Fix: energies negative hoti hain; n badhane se E n less negative hoti hai (0 ke closer). E 3 = − 1.51 eV higher (greater) hai E 1 = − 13.6 eV se bhaale hi ∣ E 3 ∣ chhota hai.
∝ Z , toh bhaari atoms ke bade orbits hote hain."
Kyun sahi lagta hai: bada nucleus = bada atom, intuitively. Fix: r n ∝ 1/ Z . Bada Z electron ko andar kheenchta hai — orbits shrink ho jaate hain. Size par n 2 dependence dominate karti hai, na ki Z .
m v r = nh use karna nh /2 π ki jagah.
Kyun sahi lagta hai: quantum n times Planck's h natural lagta hai. Fix: angular momentum ℏ = h /2 π units mein quantised hai. 2 π drop karne se har derived constant galat ho jaata hai.
Common mistake Yeh sochna ki Bohr multi-electron atoms ke liye kaam karta hai.
Kyun sahi lagta hai: yeh H ko itne khoobsoorti se nail karta hai. Fix: yeh sirf one-electron species ke liye kaam karta hai (H, He⁺, Li²⁺, Be³⁺…). Electron–electron repulsion ise otherwise tod deti hai.
Bohr model mein centripetal force kaun si force provide karti hai? Nucleus (+Ze) aur electron (−e) ke beech Electrostatic (Coulomb) attraction.
Bohr ki quantisation condition batao. m v r = nh /2 π = n ℏ (angular momentum quantised hai).
Bohr orbit radius ka formula? r n = 0.529 ( n 2 / Z ) Å.
Bohr energy levels ka formula? E n = − 13.6 ( Z 2 / n 2 ) eV.
Total energy negative kyun hoti hai? Electron bound hai; PE (negative) KE se zyada hai, deta hai E = − K E = 2 1 P E .
Radius n aur Z ke saath kaise scale karta hai? r n ∝ n 2 aur ∝ 1/ Z .
Ground-state hydrogen ki ionisation energy? 13.6 eV (electron ko n = 1 se n = ∞ tak le jaane ki energy).
Bohr model kin species ke liye kaam karta hai? One-electron (hydrogen-like) species: H, He⁺, Li²⁺, Be³⁺.
Line spectra ke liye Rydberg formula? ν ˉ = R H Z 2 ( 1/ n 1 2 − 1/ n 2 2 ) , R H = 1.097 × 1 0 7 m⁻¹.
H ke n = 1 orbit mein kya special hai? Iska radius Bohr radius a 0 = 0.529 Å hai; ground state, E = − 13.6 eV.
Recall Feynman: explain to a 12-year-old
Ek ball ko string par imagine karo jo circle mein ghoom rahi hai — string nucleus ki electric pull jaisi hai jo electron ko ghoomte rehne deti hai. Ab imagine karo ki electron sirf certain "magic circles" par hi ride kar sakta hai, jaise sirf staircase ke specific steps par khade hone ki ijazat ho, beech mein kabhi nahi. Ek step par woh calm rehta hai aur koi light nahi deta. Jab woh ek step NEECHE jump karta hai, toh ek exact colour ki light ki flash fenk deta hai; UPAR jaane ke liye use woh exact colour nighalni padti hai. Isliye hydrogen kuch sharp colours mein chamakta hai — har colour do steps ke beech ek particular jump hai.
Mnemonic Do headline formulas yaad rakho
"Radius Up, Energy Down."
Radius: 0.529 ("0-five-two-nine" bolo) × n 2 / Z — n upar hai (orbits badhte hain).
Energy: −13.6 × Z 2 / n 2 — Z upar hai (stronger charge, deeper well). Sign minus hai = "bound = zero se neeche."
Rutherford model — Bohr iske stability problem ko fix karta hai.
Hydrogen spectrum & Rydberg formula — direct application.
Photoelectric effect & Planck's quantisation — same E = h ν quantum idea.
de Broglie wavelength — standing-wave picture Bohr ka m v r = n ℏ derive karta hai.
Quantum mechanical model of atom — orbits ki jagah orbitals aate hain; explain karta hai kahan Bohr fail karta hai.
Ionisation energy — hydrogen-like ions ke liye ∣ E 1 ∣ ke barabar hai.
Postulate 1 circular orbits
Postulate 2 quantised mvr = nh - 2pi
Postulate 3 stationary states no radiation
Force balance Coulomb = centripetal
Radius rn = 0.529 n2 - Z Angstrom
Energy En = -13.6 Z2 - n2 eV
Avoids classical collapse