BOHR ATOMIC MODEL
Bohr Atomic Model
In Bohr model, Niles Bohr atom with a positively charged
nucleus surrounded by electrons that travel in circular orbits around the
nucleus-similar in structure to the solar system, but with attraction provided
by electrostatic forces.
He suggested that electrons could only have certain
classical motions:
1. Electrons in atoms
orbit the nucleus.
2. The electrons can
only orbit stably, without radiating, in certain orbits (called by Bohr the
"stationary orbits"): at a certain discrete set of distances from the
nucleus. These orbits are associated with definite energies and are also called
energy shells or energy levels. In these orbits, the electron's acceleration
does not result in radiation and energy loss as required by classical
electromagnetic.
3. Electrons can only
gain and lose energy by jumping from one allowed orbit to another, absorbing or
emitting electromagnetic radiation with a frequency ν determined by the energy
difference of the levels according to the Planck relation:
DE= E2 -E1
=hn where h is Planck’s constant .
The frequency of the radiation emitted at an orbit of period
T is as it would be in classical mechanics; it is the reciprocal of the
classical orbit period: n = 1/T
Bohr Quantization Rule
The significance of the Bohr model is that the laws of
classical mechanics apply to the motion of the electron about the nucleus only
when restricted by a quantum rule. The angular momentum L is restricted to be
an integer multiple of a fixed unit:
L = nℏ where n =
1, 2,3...
ℏ
=h/2p
n is called the
principle quantum number, . The lowest
value of n is 1
this gives a smallest possible orbital radius of 0 0.592 A0 known as the Bohr radius.
Hydrogen
Atom
A hydrogen atom
is an atom of the chemical element hydrogen. The electrically neutral atom
contains a single positively charged proton and a single negatively charged
electron bound to the nucleus by the Coulomb force. According to Bohr electron
revolve about the nucleus in different quantized circular orbits whose angular
momentum is given by L n =
h where n = 1, 2,3... .The electron is held in a circular orbit
by electrostatic attraction. The centripetal force is equal to the Coulomb
force.
mev2/r =(1/4pe0
) e2/r2
where me
is the electron's mass e is the charge of the electron, (1/4pe0 ) is Coulomb's constant and v is velocity of
electrons in orbit.
This equation
determines the electron's speed at any radius:
v = √(ke2/ mer)
K=1/4pe0
It also determines the electron's total
energy at any radius:
E= mev2/2 - ke2/r
Putting the value of v one will get ; E=-
ke2/2r
The total energy is
negative and inversely proportional to r. This means that it takes energy to
pull the orbiting electron away from the proton. For infinite values of r, the
energy is zero, corresponding to a motionless
electron infinitely far from the proton. The total energy is half the potential
energy,
From the quantization the angular momentum
L=
n ℏ
=mevr =nℏ
Substituting the expression for the velocity gives an
equation for r in terms of n
√(ke2/
mer) =ℏn
So that
the allowed orbit radius at any n is
rn=n2ℏ2/ ke2me
r1=0.53*10-10m
(For n =1)
The smallest
possible value of r in the hydrogen atom is called the Bohr radius r1.
The energy of the
n th level for any atom is determined by the radius and quantum number:
En = ke2/ rn =-( ke2 )2me
/2n2ℏ2 =(-13.6/n2)ev
The combination of natural constants in the
energy formula is called the Rydberg energy R which is given by R= (ke2 )2me
/2ℏ2
This expression is clarified by
interpreting it in combinations which form more natural units: mec2 is the rest mass energy of the electron
(511 ) keV .
(ke2) /ℏc =α= 1/137 is
the fine structure constant .
R=1/2(mec2 )
α2 = ( 1.097 ´107 m-1)
For nuclei with Z protons, the energy levels
are (to a rough approximation):
En= -Z2R/n2
Atomic Spectra
The spectrum of
atomic hydrogen arises from transitions between its permitted states.
· Each
element has a characteristic line spectrum
· When an atomic gas is
excited by passing electric current, it emits radiation. The radiation has a
spectrum which contains certain specific wavelength, called Emission line
spectrum.
· When while light is
passed through a gas, gas absorb light of certain wavelength present in its
emission spectrum. Resulting spectrum is called Absorption line spectrum.
· The
number, intensity and exact wavelength of the lines in the spectrum depend on
Temperature, Pressure, Presence of Electric field, Magnetic field, and the
motion of the source.
Spectral
series
When an electric discharge is passed through gaseous
hydrogen, the H2 molecules dissociate and the energetically excited H atoms
that are produced emit light of discrete frequencies, producing a spectrum of a
series of lines
(i) Lyman Series: 1/λ=R(1/12 -1/n2) ; n =
2,3,4,5,…(In U.V. region)
Where, R is Rydberg constant = ( 1.097 ´107
m-1)
(ii) Balmer Series: 1/λ=R(1/22 -1/n2) ; n =
3,4,5,6,…(In Visible region)
n= 3 for Ha
line n=4 for Hb Line, n =5
for Hg
(iii) Paschen series: 1/λ=R(1/32 -1/n2) ; n=4,
5, 6 …(Near Infra Red)
(iv) Bracket Series: 1/λ =R(1/42 -1/n2) ; n=5, 6,7,8,….(Infra
Red)
(v) Pfund Series: 1/λ=R(1/52 -1/n2) ; n=6,7,8,9….(Far
Infra Red)
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