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Atoms appeared 22 times across 3 years — 2.5% of Physics. This question is from Bohr Model.

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Questions 5 8 9 22

The frequency of revolution of the electron in Bohr's orbit varies with n , the principal quantum number as

Solution & Explanation

Related Formula

The orbital frequency of revolution f of an electron is inversely proportional to its time period T:

f = (1)/(T) = (v)/(2π r)

In Bohr's Atomic Model:

  • Velocity v ∝ (Z)/(n)
  • Radius r ∝ (n²)/(Z)
Core Logic

Substitute the proportional relationships of v and r into the frequency expression:

f ∝ (((1)/(n)))/(n²) f ∝ (1)/(n³)
Step 1: Verification

Thus, the frequency varies inversely with the cube of the principal quantum number: f ∝ (1)/(n³).

Pattern Recognition

Remember the sequence of powers of n in Bohr's model: radius expands as n², velocity drops as n⁻¹, angular momentum grows as n¹, and orbital time period or frequency changes as n³ or n⁻³ respectively.

Chapter Mix

Class 12 Physics: Atoms

Reference Study Guides

More Atoms Previous-Year Questions — Page 4

Q53 jee_main_2024_29_january_evening Bohr's Model of Hydrogen Atom and Hydrogen Spectrum
Hydrogen atom is bombarded with electrons accelerated through a potential difference of V, which causes excitation of hydrogen atoms. If the experiment is being performed at T = 0 K, the minimum potential difference needed to observe any Balmer series lines in the emission spectra will be (α)/(10) V, where α = ________.
Numerical Answer. Answer: 121 to 121

Solution

Related Formula

The energy of an electron in the n-th state of a hydrogen atom is:

Eₙ = -(13.6)/(n²) eV
Core Logic

At T = 0 K, all hydrogen atoms are in their ground state (n = 1). To observe any lines in the Balmer series emission spectrum:

  • The emission lines must result from a transition terminating in the state n = 2.
  • This requires the hydrogen electron to first be excited to at least the state n = 3.
  • Thus, the bombarding electrons must have enough kinetic energy to excite the ground-state electron (n = 1) to the n = 3 state.

Step 1: Calculate the Required Energy and Potential

The required energy difference is:

Δ E = E₃ - E₁ = -(13.6)/(3²) - (-(13.6)/(1²)) eV Δ E = 13.6 (1 - (1)/(9)) eV = 13.6 × (8)/(9) eV ≈ 12.09 eV

Since the excitation energy is provided by electrons accelerated through potential V, the minimum potential difference required is:

V ≈ 12.09 V ≈ 12.1 V
Step 2: Solve for Alpha

Comparing to the given form (α)/(10) V:

12.1 = (α)/(10) α = 121
Pattern Recognition

Balmer series emission requires excitation of the electron to at least n=3. Ground state n=1 to n=3 excitation energy is 12.09 eV ≈ 12.1 eV, matching α = 121 when multiplied by 10.

Chapter Mix

Class 12 Physics: Atoms

Q41 jee_main_2024_27_jan_morning Bohr Model of Hydrogen Atom
The radius of the third stationary orbit of an electron for a Bohr's atom is R. The radius of the fourth stationary orbit will be:
  • A. (4)/(3)R
  • B. (16)/(9)R
  • C. (3)/(4)R
  • D. (9)/(16)R

Solution

Related Formula
rₙ ∝ (n²)/(Z)

Where n is the principal quantum number and Z is the atomic number.

Core Logic

For a given atom, Z is constant, hence:

(r₄)/(r₃) = ((4)/(3))² = (16)/(9)

Given r₃ = R:

Step 1: Calculate the final radius
r₄ = (16)/(9)R
Pattern Recognition

Bohr orbital dimensions scale quadratically with quantum index (n²), rendering quick ratios straightforward via simple squaring operations.

Chapter Mix

Class 12 Physics: Atoms

Q jee_main_2024_29_jan_morning Bohr Model of Hydrogen Atom
When a hydrogen atom going from n = 2 to n = 1 emits a photon, its recoil speed is (x)/(5) ~m / s. Where x = _______. (Use: mass of hydrogen atom = 1.6 × 10⁻²⁷ ~kg)
Numerical Answer. Answer: 17 to 17

Solution

Related Formula

By conservation of linear momentum, the momentum of the recoiling hydrogen atom matches the momentum of the emitted photon:

patom = pphoton m v = (Δ E)/(c)

Hence, the recoil speed v is:

v = (Δ E)/(m c)

where Δ E is the energy difference between the electronic energy levels.

Core Logic

For a hydrogen transition from n = 2 to n = 1:

Δ E = E₂ - E₁ = -3.4 ~eV - (-13.6 ~eV) = 10.2 ~eV

Converting energy to Joules:

Δ E = 10.2 × 1.6 × 10⁻¹⁹ ~J

Electronic transition energy level diagram from n=2 to n=1 for Q51
Electronic transition energy level diagram from n=2 to n=1 for Q51

Step 1: Compute Recoil Speed

Substituting given constant values:

v = 10.2 × 1.6 × 10⁻¹⁹ ~J(1.6 × 10⁻²⁷ ~kg) × (3 × 10⁸ ~m/s)
Step 2: Simplify Arithmetic Fractions

Cancelling out the factor 1.6 from numerator and denominator:

v = 10.2 × 10⁻¹⁹3 × 10⁻¹⁹ = (10.2)/(3) = 3.4 ~m/s
Step 3: Solve for Variable x

Equating the computed speed to the given parameter form:

3.4 = (x)/(5) x = 3.4 × 5 = 17

Therefore, the value of x is 17.

Pattern Recognition

Always look for clean component cancellation matches prior to raw exponential expansion. In this problem, the value 1.6 in the electron charge value cancels with the structural atomic mass constant value perfectly.

Chapter Mix

Class 12 Physics: Atoms

Q37 jee_main_2024_30_january_evening Bohr Model Magnetic Moment
An electron revolving in nth Bohr orbit has magnetic moment μₙ. If μₙ ∝ nx, the value of x is:
  • A. 2
  • B. 1
  • C. 3
  • D. 0

Solution

Related Formula
μₙ = i A = (e)/(T) π r²

Alternative relation using angular momentum:

μₙ = (e)/(2m) L
Core Logic

From Bohr's quantization condition, angular momentum L is given by:

L = (nh)/(2π)

Therefore, the magnetic moment can be written directly as:

μₙ = (e)/(2m) ((nh)/(2π)) μₙ ∝ n
Step 1: Direct Proportionality Analysis

We can also derive this via velocity and radius: v ∝ (1)/(n) and r ∝ n².

μₙ = (e v r)/(2) ∝ ((1)/(n)) (n²) = n

Comparing with μₙ ∝ n^x, we find x = 1.

Pattern Recognition

Magnetic moment of an electron in a Bohr orbit is always directly proportional to the principal quantum number n. It is an integer multiple of the Bohr magneton (μB = (eh)/(4π m)).

Chapter Mix

Class 12 Physics: Atoms

Q36 jee_main_2024_30_jan_morning Bohr Model and Electron Energy
The ratio of the magnitude of the kinetic energy to the potential energy of an electron in the 5th excited state of a hydrogen atom is :
  • A. 4
  • B. (1)/(4)
  • C. (1)/(2)
  • D. 1

Solution

Related Formula

KE = -E PE = 2E

KE = (1)/(2) |PE|
Core Logic

In any allowed Bohr orbit (for any value of principal quantum number n), the relationship between kinetic energy (KE), potential energy (PE), and total energy (E) strictly obeys the virial theorem for a Coulombic force field.

|PE| = 2 × KE
Step 1: Formulate the Ratio

The question asks for the ratio of the magnitude of KE to the magnitude of PE.

KE|PE| = (1)/(2)

This ratio is independent of the orbit state. Even though it is the 5th excited state, the ratio remains (1)/(2).

Pattern Recognition

Energy relationships in Bohr orbits (and planetary motion): K = -E = -U/2. The state number (n) is given solely as a distractor.

Chapter Mix

Class 12 Physics: Atoms

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