Title: Rutherford discovered the nucleus
1- Rutherford discovered the nucleus
- Natural to think of atoms as little planetary
systems
2Continuous Spectrum
White light
Emission Spectrum
Hot GAS
Absorption Spectrum
Cold Gas
White light
3The Balmer spectrum of hydrogen
- The Balmer series is in the visible
- the Lyman Series is in the UV
4(No Transcript)
5(No Transcript)
6(No Transcript)
7The Bohr model
- Energy was quantized
- Angular Momentum was quantized
8Bohrs argument
Assume nucleus infinitely heavy Assume electron
is moving in circular orbit of radius,r,with
speed v then
9Bohr assumed that the orbital angular momentum
was quantized i.e. Consequently we obtain
fixed values of
10(No Transcript)
11(No Transcript)
12(No Transcript)
13(No Transcript)
14For Hydrogen Z1
15(No Transcript)
16(No Transcript)
17De Broglie Hypothesis
18(No Transcript)
19?-wavelength
L ?/2 ? 2L f v/(2L) L ? ? L f
v/(L) L 3?/2 ? 2L/3 f 3v/(2L)
20The Schrödinger Wave Equation
21(No Transcript)
22Eigenvalue equation
Observable quantity
eigenvalue
operator
eigenfunction
23Three basic assumptions
- States of a system are described by wave
functions, Y - Observable quantities are associated with
operators - When the value of an observable, Q, is known to
be q, the system is in a state, whose function is
an eigenfunction of the associated operator
24The Hamiltonian
25Energy Eigenvalue Problem
The time independent Schrödinger equation
26Energy Eigenvalue Problem
The time dependent Schrödinger equation
27- We have not and indeed can not derive the
Schrödinger equation - We have motivated it as reasonable
- And shall now assume it is true for all non
relativistic microscopic situations
28Schrödingers original derivation
- Schrödinger began from the assumption of matter
waves, and by analogy with geometrical optics he
introduced a variational principle which lead him
to postulate that the matter waves satisfied the
equation. -
29Look for a stationary solution, i.e look for a
solution by separation of variables
30Easy to see solution is of the form
E is a constant that comes from the separation of
variables which we identify with the energy And
satisfies the eigenvalue equation
31Example
32(No Transcript)
33Comments
- This is of the same form as the Bohr atom
energies, i.e. discrete - Our solutions are only determined up to a
constant, i.e. - ?nBnsinknx
34- Notice we have implicitly assume that the
operator corresponding to postion acts as by
simply multiplying the wave function - All other operators which have a classical analog
can be deduced from this identification, as we
have seen for the energy
35(No Transcript)
36Particle in a box
37(No Transcript)
38(No Transcript)
39Spherical Symmetry
40Time dependent wave function We will assume that
potential V is independent of time and purely
radial
41Look for a stationary solution, i.e look for a
solution by separation of variables
42Easy to see solution is of the form
E is a constant that comes from the separation of
variables which we identify with the energy And
satisfies the eigenvalue equation
43Schrödinger Equation in Spherical polar
coordinates H-atom
44Schrödinger Equation in Spherical polar
coordinatesfor any radial potential V(r)
V(r)?E?
45Look for a solution by separation of variables
46(No Transcript)
47(No Transcript)
48(No Transcript)
49(No Transcript)
50Rhs independent of F
Lhs depends only on F
51Rhs independent of F
Lhs depends only on F
Common value must be a constant
52(No Transcript)
53Depends only on r
Depends only on ?
54Chose constant of separation to be l(l1)
55(No Transcript)
56T equation
To be determined
ml is a ve integer
57T equation
Make substitution zcos?
58T equation
This equation is well known its solutions are
the associated legendre polynomials
59(No Transcript)
60 61(No Transcript)
62(No Transcript)
63 64(No Transcript)
65(No Transcript)
66- Note angular momentum is now quantized
- automatically