If an alpha particle with energy 7.7 MeV is bombarded on a thin gold foil, the closest distance from nucleus it can reach is ____ m. (Atomic number of gold = 79 and frac14pi in_0 = 9 times 10^9 in SI units)

Solution & Explanation

### Related Formula K_textinitial = U_textclosest approach K = frac14pi epsilon_0 frac(2e)(Ze)r_0 ### Core Logic By energy conservation, the entire kinetic energy of the alpha particle gets converted to electrostatic potential energy at the distance of closest approach (r_0). K_i + U_i = K_f + U_f K_i + 0 = 0 + frac14piepsilon_0 frac(2e)(79e)r_0 ### Step 1: Convert Energy and Solve Initial kinetic energy K_i = 7.7text MeV = 7.7 times 10^6 times 1.6 times 10^-19text J. 7.7 times 10^6 times 1.6 times 10^-19 = frac9 times 10^9 times (2 times 1.6 times 10^-19) times (79 times 1.6 times 10^-19)r_0 r_0 = frac9 times 10^9 times 2 times 79 times (1.6 times 10^-19)^27.7 times 10^6 times 1.6 times 10^-19 r_0 = frac9 times 10^9 times 158 times 1.6 times 10^-197.7 times 10^6 r_0 = frac2275.2 times 10^-107.7 times 10^6 = 295.48 times 10^-16text m approx 2.95 times 10^-14text m ### Pattern Recognition Distance of closest approach problem: Simply equate initial Kinetic Energy (in Joules) to Potential Energy k(Z_1e)(Z_2e)/r_0. Alpha particle has charge 2e. ### Evaluation Rubric / Model Answer null ### Chapter Mix Class 12 Physics: Atoms

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Q16 jee_main_2025_07_april_morning Hydrogen Spectrum
For a hydrogen atom, the ratio of the largest wavelength of Lyman series to that of the Balmer series is.
  • A. 5:36
  • B. 5:27
  • C. 3 : 4
  • D. 27:5

Solution

### Related Formula The wavelength lambda for a transition in a hydrogen atom is given by the Rydberg formula: frac1lambda = R left( frac1n_1^2 - frac1n_2^2 right) To find the largest wavelength (minimum energy transition), select the adjacent higher shell n_2 = n_1 + 1. ### Core Logic - **Lyman Series largest wavelength (lambda_L)**: Transition from n = 2 to 1 frac1lambda_L = R left( frac11^2 - frac12^2 right) = frac3R4 implies lambda_L = frac43R - **Balmer Series largest wavelength (lambda_B)**: Transition from n = 3 to 2 frac1lambda_B = R left( frac12^2 - frac13^2 right) = R left( frac14 - frac19 right) = frac5R36 implies lambda_B = frac365R ### Step 1: Ratio Calculation Now, compute the ratio of the wavelengths: fraclambda_Llambda_B = fracfrac43Rfrac365R = frac43 times frac536 = frac527 ### Pattern Recognition Sees: Ratio of largest wavelengths of series. Shortcut: The largest wavelength in a series starting at ground level n_1 is \lambda \propto \frac{n_1^2 (n_1+1)^2}{2n_1 + 1}. For Lyman (n_1=1): \lambda_L \propto \frac{4}{3}. For Balmer (n_1=2): \lambda_B \propto \frac{36}{5}. Ratio: \frac{4/3}{36/5} = \frac{5}{27}$. ### Evaluation Rubric / Model Answer null ### Chapter Mix Class 12 Physics: Atoms
Q20 jee_main_2025_29_jan_evening Hydrogen Spectrum
The number of spectral lines emitted by atomic hydrogen that is in the 4^textth energy level, is:
  • A. 6
  • B. 0
  • C. 3
  • D. 1

Solution

### Related Formula N = fracn(n - 1)2 where n is the principal quantum number of the starting energy level. ### Core Logic For a hydrogen sample initially in the n = 4 level, the possible downward transition pathways to reach the ground state (n=1) are:
Hydrogen Spectrum Transitions diagram for Q20 - JEE Main 2025 Evening
Hydrogen Spectrum Transitions diagram for Q20 - JEE Main 2025 Evening
Using the combination formula for all transitions: N = frac4(4 - 1)2 = frac4 times 32 = 6 Thus, 6 distinct spectral lines are generated. ### Pattern Recognition Think of it as counting combinations of transitions between levels: _nC_2. For n=4, _4C_2 = 6 lines. ### Evaluation Rubric / Model Answer null ### Chapter Mix Class 12 Physics: Atoms
Q5 jee_main_2025_24_jan_morning Bohr Model of the Hydrogen Atom
During the transition of electron from state A to state C of a Bohr atom, the wavelength of emitted radiation is 2000 Å and it becomes 6000 Å when the electron jumps from state B to state C. Then the wavelength of the radiation emitted during the transition of electrons from state A to state B is :-
  • A. 3000 Å
  • B. 6000 Å
  • C. 4000 Å
  • D. 2000 Å

Solution

### Related Formula The energy of the emitted photon during an atomic transition between energy states is given by: Delta E = frachclambda where h is Planck's constant, c is speed of light, and lambda is the photon wavelength. ### Core Logic Write equations for the energy transitions from the layout of levels
Bohr Model of the Hydrogen Atom diagram for Q5 - JEE Main 2025 Morning
Bohr Model of the Hydrogen Atom diagram for Q5 - JEE Main 2025 Morning
: E_A - E_C = frachclambda_AC = frachc2000text AA quad dots (i) E_B - E_C = frachclambda_BC = frachc6000text AA quad dots (ii) ### Step 1: Finding Transition A to B Subtracting equation (ii) from equation (i) gives the net transition energy from A to B : E_A - E_B = (E_A - E_C) - (E_B - E_C) frachclambda_AB = frachc2000 - frachc6000 frac1lambda_AB = frac3 - 16000 = frac26000 = frac13000 lambda_AB = 3000text AA ### Pattern Recognition Energy differences add linearly, which means their corresponding inverse wavelengths satisfy a parallel reciprocal subtraction rule: frac1lambda_AB = frac1lambda_AC - frac1lambda_BC. ### Evaluation Rubric / Model Answer null ### Chapter Mix Class 12 Physics: Atoms
Q7 jee_main_2025_28_jan_evening Bohr Model
The frequency of revolution of the electron in Bohr's orbit varies with n , the principal quantum number as
  • A. frac1n
  • B. frac1mathrmn^3
  • C. frac1mathrmn^4
  • D. frac1n^2

Solution

### Related Formula The orbital frequency of revolution f of an electron is inversely proportional to its time period T: f = frac1T = fracv2pi r In Bohr's Atomic Model: * Velocity v propto fracZn * Radius r propto fracn^2Z ### Core Logic Substitute the proportional relationships of v and r into the frequency expression: f propto fracleft(frac1nright)n^2 implies f propto frac1n^3 ### Step 1: Verification Thus, the frequency varies inversely with the cube of the principal quantum number: f propto frac1n^3. ### Pattern Recognition Remember the sequence of powers of n in Bohr's model: radius expands as n^2, velocity drops as n^-1, angular momentum grows as n^1, and orbital time period or frequency changes as n^3 or n^-3 respectively. ### Evaluation Rubric / Model Answer null ### Chapter Mix Class 12 Physics: Atoms
Q49 jee_main_2024_01_february_morning Hydrogen Spectrum
The minimum energy required by a hydrogen atom in ground state to emit radiation in Balmer series is nearly:
  • A. 1.5 eV
  • B. 13.6 eV
  • C. 1.9 eV
  • D. 12.1 eV

Solution

### Related Formula Bohr state energy level values: E_n = -frac13.6n^2mathrm~eV Transition excitation requirement: Delta E = E_textfinal - E_textinitial ### Core Logic To emit radiation in the Balmer series, the hydrogen electron must first be excited to at least the n=3 shell. This allows it to jump down to n=2 and produce the first spectral line of the Balmer series. Energy required to transition from ground state (n=1) to n=3: E_1 = -13.6mathrm~eV E_3 = -frac13.63^2 = -1.51mathrm~eV ### Step 1: Calculate Energy Gap Delta E = E_3 - E_1 = -1.51 - (-13.6) = 12.09mathrm~eV approx 12.1mathrm~eV ### Pattern Recognition Balmer emissions always return down to n=2. Thus, the initial excitation starting from ground state n=1 must reach at least n=3 to create a valid Balmer transition. ### Evaluation Rubric / Model Answer null ### Chapter Mix Class 12 Physics: Atoms

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