Advertisements
Advertisements
Question
Using Bohr’s postulates, obtain the expression for the total energy of the electron in the stationary states of the hydrogen atom. Hence draw the energy level diagram showing how the line spectra corresponding to Balmer series occur due to transition between energy levels.
Advertisements
Solution
According to Bohr’s postulates, in a hydrogen atom, a single alectron revolves around a nucleus of charge +e. For an electron moving with a uniform speed in a circular orbit os a given radius, the centripetal force is provided by Columb force of attraction between the electron and the nucleus. The gravitational attraction may be neglected as the mass of electron and proton is very small.
So,
`(mv^2)/r = (ke^2)/r^2`
or `mv^2 = (ke^2)/r .............. (1)`
where m = mass of electron
r = radius of electronic orbit
v = velocity of electron.
Again,
`mvr = (nh)/(2π)`
or `v = (nh)/(2πmr)`
From eq.(1), we get,
`m((nh)/(2πmr)^2) = (ke^2)/r`
`=> r = (n^2h^2)/(4π^2kme^2).....................(2)`
(i) Kinetic energy of electron,
`E_k = 1/2 mv^2 = (ke^2)/(2r)`
Using eq (2), we get
`Ek =ke^2/2 (4π^2kme^2)/(n^2h^2)`
=`(4π^2kme^2)/(n^2h^2)`
`(2π^2k^2me^4)/(n^2h^2)`
(ii) Potential energy
`E_p = -(k(e) xx (e))/r = - (ke^2) / r `
Using eq (2), we get
`E^p =-ke^2 xx (4π^2kme^2)/(n^2h^2)`
= `-(4π^2k^2me^4)/(n^2h^2)`
Hence, total energy of the electron in the nth orbit
`E =E_p+E_k =(4π^2k^2me^4)/(n^2h^2)+(2π^2k^2me^4)/(n^2h^2) =- (2π^2k^2me^4)/(n^2h^2) =- (13.6)/n^2 eV `
When the electron in a hydrogen atom jumps from higher energy level to the lower energy level, the difference of energies of the two energy levels is emitted as a radiation of particular wavelength. It is called a spectral line.
In H-atom, when an electron jumps from the orbit ni to orbit nf, the wavelength of the emitted radiation is given by,
`1/λ = R (1/n_f^2 -1/n_i^2)`
Where,
R → Rydberg’s constant = 1.09678 ×107 m−1
For Balmer series, nf = 2 and ni = 3, 4, 5, …
`1/λ = R (1/2^2 -1/n_i^2)`
Where, ni = 3, 4, 5, …
These spectral lines lie in the visible region.

APPEARS IN
RELATED QUESTIONS
An electron is orbiting in 5th Bohr orbit. Calculate ionisation energy for this atom, if the ground state energy is -13.6 eV.
In accordance with the Bohr’s model, find the quantum number that characterises the earth’s revolution around the sun in an orbit of radius 1.5 × 1011 m with orbital speed 3 × 104 m/s. (Mass of earth = 6.0 × 1024 kg)
Using Bohr’s postulates, obtain the expression for total energy of the electron in the nth orbit of hydrogen atom.
Radiation coming from transition n = 2 to n = 1 of hydrogen atoms falls on helium ions in n = 1 and n = 2 states. What are the possible transitions of helium ions as they absorbs energy from the radiation?
A beam of monochromatic light of wavelength λ ejects photoelectrons from a cesium surface (Φ = 1.9 eV). These photoelectrons are made to collide with hydrogen atoms in ground state. Find the maximum value of λ for which (a) hydrogen atoms may be ionized, (b) hydrogen atoms may get excited from the ground state to the first excited state and (c) the excited hydrogen atoms may emit visible light.
Suppose in an imaginary world the angular momentum is quantized to be even integral multiples of h/2π. What is the longest possible wavelength emitted by hydrogen atoms in visible range in such a world according to Bohr's model?
Consider aiming a beam of free electrons towards free protons. When they scatter, an electron and a proton cannot combine to produce a H-atom ______.
- because of energy conservation.
- without simultaneously releasing energy in the from of radiation.
- because of momentum conservation.
- because of angular momentum conservation.
If a proton had a radius R and the charge was uniformly distributed, calculate using Bohr theory, the ground state energy of a H-atom when (i) R = 0.1 Å, and (ii) R = 10 Å.
The radius of the nth orbit in the Bohr model of hydrogen is proportional to ______.
The de Broglie wavelength of an electron in the first Bohr’s orbit of hydrogen atom is equal to ______.
