Wave Functions and the Schrödinger Equation - Prof. David Peak, Study notes of Physics

The concept of wave functions in quantum mechanics, focusing on the schrödinger equation and its implications. It explains how the probabilities of finding a particle in a particular state can be calculated using wave functions and the concept of superposition before measurement.

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Pre 2010

Uploaded on 07/30/2009

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Wavefunctions, 2710 Fall 2008
More about wavefunctions
If
!
"1
and
!
"2
satisfy the Schrödinger Equation then so does
!
"=a1"1+a2"2
.
In order for
!
"
#$
+$
%
2
dx =1
, it must be that
!
a1
2+a2
2=1
.
When you make a series of N (>>1) measurements on
!
"
, you find a result corresponding
to
!
"1
about
!
Na1
2
times and one corresponding to
!
"2
about
!
Na2
2
times.
The average value of a measurement on state
!
"
corresponding to the operator Qop is
defined as
. This implies that for the wavefunction abo ve
!
Q=a1
2Q
1+a2
2Q2
.
Example: Suppose Q is energy and
!
"1
and
!
"2
are the two lowest energy eigenstates of the
infinite square well. Suppose that
!
a1=1 2
and
!
a2=1 2
. What is
!
E
in terms of E1, the
ground state energy? Answer:
!
E=1
2
E1+1
2
E2=1
2+1
2
22
"
#
$ %
&
'
E1=2.5E1
.
You interpret
!
a1
2
and
!
a2
2
as the probabilities of being in
!
"1
and
!
"2
, respectively.
After making the measurement, if the result corresponded to
!
"1
then an immediate
subsequent measurement will also correspond to
!
"1
; the wavefunction
!
"
is said to be
“collapsed” into
!
"1
by the measurement. It will stay in
!
"1
as long as there are no other
interactions (fro m the rest of the universe). Thus, QM says that before a measurement is
made the most that can be said about the state of a system is that it is some superposition
(i.e., sum) of eigenstates. The act of measurement “creates the reality” of the system
being in one of them.
More generally,
!
"=an
n
#"n
, where the sum can involve any number of terms, and
!
Q=an
2Qn
n
"
.

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Wavefunctions, 2710 Fall 2008

More about wavefunctions

  • If !

(^) " 1 and !

(^) " 2 satisfy the Schrödinger Equation then so does !

  • In order for^ "^ =^ a^1 "^1 +^ a^2 "^2. !

% #$^ +$ "^2 dx = 1 , it must be that

  • When you make a series of N (>>1) measurements on^^ a^12 +^ a^22 =^1. !

to^ ", you find a result corresponding !

" 1 about !

Na 12 times and one corresponding to !

" 2 about !

  • The average value of a measurement on state^^ Na^22 times. !

defined as^ "corresponding to the operator^ Q op^ is !

Q = % #$^ +$"* Q op" dx. This implies that for the wavefunction above

Q = a 12 Q 1 + a 22 Q 2. Example: Suppose Q is energy and !

" 1 and !

infinite square well. Suppose that^ "^2 are the two lowest energy eigenstates of the !

a 1 = 1 2 and !

a 2 = 1 2. What is !

E in terms of E 1 , the ground state energy? Answer: !

E = 12 E 1 + 12 E 2 = " # $ 12 + 12 22 % & ' E 1 = 2.5 E 1.

  • You interpret !

a 12 and !

a 22 as the probabilities of being in !

" 1 and !

  • After making the measurement, if the result corresponded to^ "^2 , respectively. !

subsequent measurement will also correspond to^ "^1 then an immediate !

" 1 ; the wavefunction !

“collapsed” into^ "is said to be !

" 1 by the measurement. It will stay in !

interactions (from the rest of the universe). Thus, QM says that before a measurement is^ "^1 as long^ as there are no other made the most that can be said about the state of a system is that it is some (i.e., sum) of eigenstates. The act of measurement “creates the reality” of the system superposition

  • being in one of them.More generally, !

" = # n an " n , where the sum can involve any number of terms, and

Q = " nan^2 Qn.