properties of wavefunctions

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http://www.colorado.edu/physics/phys2170/ Physics 2170 – Fall 2013 1 Properties of Wavefunctions •2 nd exam is next Thursday (Nov. 7) in G2B90 from 7:30 – 9:00 pm. New Homework posted and due next week – it is from material in chapter 7. So I think it is part of studying. A past exam from 2011 has posted on D2L – both exam and solution. Announcements:

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Page 1: Properties of Wavefunctions

http://www.colorado.edu/physics/phys2170/ Physics 2170 – Fall 2013 1

Properties of Wavefunctions

•  2nd exam is next Thursday (Nov. 7) in G2B90 from 7:30 – 9:00 pm.

•  New Homework posted and due next week – it is from material in chapter 7. So I think it is part of studying.

•  A past exam from 2011 has posted on D2L – both exam and solution.

Announcements:

Page 2: Properties of Wavefunctions

http://www.colorado.edu/physics/phys2170/

Friday Facts

Physics 2170 – Fall 2013 2

What is it?

Page 3: Properties of Wavefunctions

http://www.colorado.edu/physics/phys2170/

How will the detectors see gravitational waves? When gravitational waves pass through LIGO's L-

shaped detector they will decrease the distance between the test masses in one arm of the L, while increasing it in the other. These changes are minute: just 10-16 centimeters, or one-hundred-millionth the diameter of a hydrogen atom over the 4 kilometer length of the arm.

Measurement is performed by bouncing high-power laser light beams back and forth between the test masses in each arm, and then interfering the two arms' beams with each other. The slight changes in test-mass distances throw the two arms' laser beams out of phase with each other, thereby disturbing their interference and revealing the form of the passing gravitational wave. Physics 2170 – Fall 2013 3

Page 4: Properties of Wavefunctions

http://www.colorado.edu/physics/phys2170/

LIGO

Physics 2170 – Fall 2013 4

Page 5: Properties of Wavefunctions

http://www.colorado.edu/physics/phys2170/ Physics 2170 – Fall 2013 5

Superposition If Ψ1(x,t) and Ψ2(x,t) are both solutions to the wave equation then the sum Ψ1(x,t) + Ψ2(x,t) is also a solution.

Actually, any linear combination AΨ1(x,t) + BΨ2(x,t) is a solution.

This is the superposition principle.

This seems pretty straightforward but is actually an important result

Let’s look at the infinite square well solution.

Page 6: Properties of Wavefunctions

http://www.colorado.edu/physics/phys2170/

Infinite Square Well

Physics 2170 – Fall 2013 6

For each n, can have a , corresponding to an eigenfunction for each eigenvalue. For each eigenfunction we have a wave function.

ψn (x) + φn (t)

Can have a linear combination (superposition) of these states -

Ψ(x, t) = a Ψ1(x, t) + b Ψ2(x,t)where a and b are coefficients and are normalized so the overall probability is 100%.

Note E1, E2, …., En are called eigenvalues of the potential.

n is the quantum number

Page 7: Properties of Wavefunctions

http://www.colorado.edu/physics/phys2170/

Mathematical Properties of WF

Physics 2170 – Fall 2013 7

Ψ(x, t) = a Ψ1(x, t) + b Ψ2(x,t)

Substituting this function into the Schrodinger equation,

−2

2md2Ψdx 2 +VΨ - i∂Ψ

∂t= 0

Since both satisfy the Schrodinger equation, both brackets must vanish.

Ψ1 and Ψ2

a −2

2md2Ψ1

dx 2 +V Ψ1 - i∂Ψ1

∂t⎡

⎣ ⎢

⎦ ⎥

+ b −2

2md2Ψ2

dx 2 +V Ψ2 - i∂Ψ2

∂t⎡

⎣ ⎢

⎦ ⎥ ≡ 0

Page 8: Properties of Wavefunctions

http://www.colorado.edu/physics/phys2170/

Mathematical Properties cont.

Physics 2170 – Fall 2013 8

We can write the wave function

and the complex conjugate as

Ψ(x, t) = ane−iEnt / ψn (x)

n=1

Ψ*(x, t) = an*e+iEnt / ψn

* (x)l=1

Multiplying the two together we get:

Ψ*(x, t)Ψ(x,t) = an*

n=1∑ anψn

* (x)ψn (x)

+l=1∑ al

*

n=1∑ anψ l

*(x)ψn (x)e−i(En −El )t /

Note we see that in general the probability density depends on time. Means to locate the particle depends on the time at which the measurement is made.

Page 9: Properties of Wavefunctions

http://www.colorado.edu/physics/phys2170/

Mathematical properties cont.

Physics 2170 – Fall 2013 9

Ψ*(x, t)Ψ(x,t) = an*

n=1∑ anψn

* (x)ψn (x)

For the special case of a particle whose associated wavefunction is one of the functions corresponding to a single eigenvalue En, then

Probability is independent of time. These are called stationary states or eigenstates of potential V(x). Also, The probability interpretation demands that any wave function must be normalized.

It is clear that the normalization can be achieved at any instant of time, by proper choice of an, but it has to satisfied at all times.

Page 10: Properties of Wavefunctions

http://www.colorado.edu/physics/phys2170/

Math Properties cont.

Physics 2170 – Fall 2013 10

ψn* (x)

−∞

∫ ψn (x)dx =1

ψ l (x)−∞

∫ ψn (x)dx = 0 l ≠ n

Because of this property – product of on eigenfunction of the set times the complex conjugate of a different eigenfunction of the set vanishes, the eigenfunctions are said to be orthogonal.

Let’s try the product of eigenfunctions for the infinite square well.

Page 11: Properties of Wavefunctions

http://www.colorado.edu/physics/phys2170/

Infinite Square Well

Physics 2170 – Fall 2013 11

sinmx sin nx∫ dx =sin(m − n)x

2(m − n)−

sin(m + n)x2(m + n)

m2 ≠ n2[ ]

sin2 nx ∫ dx = −cosnx sinnx

2+nx2

When evaluated at 0 and at a for the infinite square well only the squared eigenfunctions are retained.

0 0 a

∞ ∞

V(x

)

Page 12: Properties of Wavefunctions

http://www.colorado.edu/physics/phys2170/ Physics 2170 – Fall 2013 12

Clicker question 1 Set frequency to DA Q. What atomic element comes last alphabetically?

A.  Beryllium B.  Copper C.  Arsenic D.  Barium E.  Zirconium

Page 13: Properties of Wavefunctions

http://www.colorado.edu/physics/phys2170/ Physics 2170 – Fall 2013 13

Clicker question 2 Set frequency to DA Q. What acronyms do physicists use to explain “Weakly interacting Massive Particles” and “Massive Compact Halo Objects” ?

A.  Whales and Marlins B.  Wimps and Machos C.  Willies and Massives D.  None of the above

Page 14: Properties of Wavefunctions

http://www.colorado.edu/physics/phys2170/

Probability Flux

Physics 2170 – Fall 2013 14

probability density =

=

Ψ*Ψ = A*e−i(kx−Et / )A e+ i(kx−Et / )

A*A

Probability flux =

=

kmA*A

v probability density

Page 15: Properties of Wavefunctions

http://www.colorado.edu/physics/phys2170/

Step Potential

Physics 2170 – Fall 2013 15

Think of a charged particle moving along x-axis of a system of two electrodes held at different voltages

Page 16: Properties of Wavefunctions

http://www.colorado.edu/physics/phys2170/

Step or Barrier Potential

Physics 2170 – Fall 2013 16

Take a particle of mass m and energy E < V0

Page 17: Properties of Wavefunctions

http://www.colorado.edu/physics/phys2170/

Solving the Step Potential- Use TISE

Physics 2170 – Fall 2013 17

Arbitrary constants A, B, C, D must satisfy boundary conditions ie C=0

Page 18: Properties of Wavefunctions

http://www.colorado.edu/physics/phys2170/

Step cont.

Physics 2170 – Fall 2013 18

Continuity of wave function at x=0 yields:

or D = A + B (1)

Continuity of derivative of wave function at x=0 yields

or (2)

Adding (1) and (2) gives

Subtracting (1) and (2) gives

Page 19: Properties of Wavefunctions

http://www.colorado.edu/physics/phys2170/

Step cont.

Physics 2170 – Fall 2013 19

S(x, t) = −i2m

Ψ*(x, t)∂Ψ(x, t)∂x

−Ψ(x, t)∂Ψ*(x,t)∂x

⎣ ⎢

⎦ ⎥ Remember