S. L. Arora Solutions for Chapter: Atoms, Exercise 1: Problems For Practice

Author:S. L. Arora

S. L. Arora Physics Solutions for Exercise - S. L. Arora Solutions for Chapter: Atoms, Exercise 1: Problems For Practice

Attempt the free practice questions on Chapter 4: Atoms, Exercise 1: Problems For Practice with hints and solutions to strengthen your understanding. PHYSICS A Reference Book for Class 12 Volume 2 solutions are prepared by Experienced Embibe Experts.

Questions from S. L. Arora Solutions for Chapter: Atoms, Exercise 1: Problems For Practice with Hints & Solutions

MEDIUM
12th CBSE
IMPORTANT

The second member of Lyman's series in hydrogen spectrum has a wavelength of 5400 A0. Calculate the wavelength of the first member.

EASY
12th CBSE
IMPORTANT

A photon of energy 12.09 eV is absorbed by an electron in ground state of a hydrogen atoms. What will be the energy level of electron? The energy of electron in the ground state of hydrogen atom is -13.6 eV.

MEDIUM
12th CBSE
IMPORTANT

The period of revolution of the electron in the third orbit in a hydrogen atom is 4.132×10-15 s. Hence find the period in the 5 th Bohr orbit.

EASY
12th CBSE
IMPORTANT

The electron, in a hydrogen atom, is in its second excited state. Calculate the wavelength of the lines in the Lyman series, that can be emitted through the permissible transitions of this electron.(Given the value of Rydberg constant, R=1.1×107 m-1.

MEDIUM
12th CBSE
IMPORTANT

Show that the shortest wavelength lines in Lyman, Balmer and Paschen series have their wavelengths in the ratio 1:4:9.

EASY
12th CBSE
IMPORTANT

The short wavelength limit for the Lyman series of the hydrogen spectrum is 913.4 A0. Calculate the short wavelength limit for Balmer series of hydrogen spectrum.

MEDIUM
12th CBSE
IMPORTANT

Find the ratio between the wavelengths of the 'most energetic' spectral lines in the Balmer and Paschen series of the hydrogen spectrum.

MEDIUM
12th CBSE
IMPORTANT

Find out the wavelength of the electron orbiting in the ground state of hydrogen atom.