8. Quantum Numbers
• According to Heisenberg’s Uncertainty
Principle, it is not possible to give the
exact position of an electron and its
energy at the same time.
• But the probability of finding an electron in
an orbital of given energy can be
determined.
9. • In atom : large of orbitals are possible.
• Orbitals : differ in size, shape & orientation
in space around the nucleus.
• State of e in atom: its location with respect
to the nucleus & its energy.
• Permissible state of an e : orbitals
• Quantum numbers.
10. The 4 Quantum Numbers
• Principal Quantum Number, n
• Azimuthal Quantum Number, l
• Magnetic Quantum Number, ml
• Spin Quantum Number, ms
11. Principal Quantum Number
• Determines Main energy level of an orbital
- shell
• An increase in n also means increase in
the energy of the electron in the orbital.
• n= 1, 2, 3….
• Maximum no.of electrons = 2n^2
12. Azimuthal Quantum Number
• Also called Angular Momentum Number
• Defines the shape of the orbital
• Values range from 0 to n-1
13. Azimuthal Quantum Number
l Sublevel Orbital Shape
0 s(harp) Spherical
1 p(rincipal) dumbbell-
shaped
2 d(iffused) Cloverleaf
3 f(undamental) Too complex
14. Azimuthal Quantum Number
• A sublevel in a particular main energy
level is defined by its n and its l values.
n l Kind of
Sublevel
1 0 1s
3 1 3p
15. Magnetic Quantum Number, ml
• Charged particle – in motion: produce magnetic field
• Magnetic field value represented by,ml
• Describes the orientation of the orbital in space
• Values are –l to +l
• Values per sublevel = 2l +1
16. • two orbitals in same shell-identical value, but they
must have different values of m.
• -nce of magnetic field – all orbitals having same
value of n & l, but different values of m: same
energies.
• Moving e- : small magnetic field
• When external magnetic field is applied, interaction
occur & e- : orient themselves.
• This changes energies slightly.
18. Spin Quantum Number, ms
• Spin of the electron
• e- two types of motion.
• 1. orbital & 2. axial motion
• Values are +1/2 and -1/2
• Clockwise and Counterclockwise
• Opposite spins because of Pauli Exclusion Principle
19. nn shellshell ll subshellsubshell mmll
#orbitals#orbitals
#e#e––
11 KK 00 ss 00 11 22
22 LL 00 ss 00 11 22
11 pp ––1,0,11,0,1 33 66
33 MM 00 ss 00 11 22
11 pp ––1,0,11,0,1 33 66
88
22 dd -2,-1,0,1,2-2,-1,0,1,2 55 1010
1818
44 NN 00 ss 00 11 22
11 pp ––1,0,11,0,1 33 66
22 dd -2,-1,0,1,2-2,-1,0,1,2 55 1010
33 ff -3,-2,-1,0,1,2,3-3,-2,-1,0,1,2,3 77 1414
3232
n2
1
4
9
16
Max
20. Shapes of atomic orbitals
• Atomic orbitals
• Probability(Ψ2) : distribution of e- cloud in
the space.
• Density of e- cloud = probability of finding
e-
• Probability of finding e- : not same
• Orbitals : not have a rigid boundary
• Atom : definite size.
22. Shapes of S-orbitals:sphere
• For s-orbitals, l=0 (ns)
• Distribution of e- density = symmetrical
• Probability of finding an e- : same at all angles.
• Sphere-no exact radius
• n increases : s orbital –larger
• Total no. of concentric sphere = n.
• For e.g., 1s = 1 sphere
2s = 2 sphere
Energy of s-orbital increses = n
23. P-orbitals(dumb-bell)
• l=1, m=-1, 0, +1
• Distribution of e- density: not spherical
• Same shape but directions are different.
• For 2p orbitals, e- density is maximum along the orbital
axis.
• e- density at nucleus = zero.
• Node & nodal plane.
• Size of p-orbital is increses with n.
• Lobes of 3p is bigger than 2p.
25. References
• Essentials of Physical chemistry by Bahl Arun, S Chand, 2012
• General chemistry by Ebbing Darrell D, 5th
, A I T B S Publishers,
2002