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Wednesday, Oct. 30, 2013 PHYS 3313-001, Fall 2013 Dr. Jaehoon Yu 1 PHYS 3313 – Section 001 Lecture #14 Wednesday, Oct. 30, 2013 Dr. Jaehoon Yu Infinite Square Well Potential Finite Potential Well Penetration Depth Degeneracy Simple Harmonic Oscillator
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Page 1: PHYS 3313 – Section 001 Lecture #14yu/teaching/fall13-3313-001/...Wednesday, Oct. 30, 2013 PHYS 3313-001, Fall 2013 Dr. Jaehoon Yu 2 Announcements • Homework #5 – CH6 end of

Wednesday, Oct. 30, 2013 PHYS 3313-001, Fall 2013 Dr. Jaehoon Yu

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PHYS 3313 – Section 001 Lecture #14

Wednesday, Oct. 30, 2013 Dr. Jaehoon Yu

•  Infinite Square Well Potential •  Finite Potential Well •  Penetration Depth •  Degeneracy •  Simple Harmonic Oscillator

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Wednesday, Oct. 30, 2013 PHYS 3313-001, Fall 2013 Dr. Jaehoon Yu

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Announcements •  Homework #5

–  CH6 end of chapter problems: 3, 5, 11, 14, 22, and 26 –  Due on Wednesday, Nov. 6 in class

•  Quiz #3 –  At the beginning of the class Wed., Nov. 6 –  Covers CH5.6 to what we cover Monday, Nov. 4 –  Prepare your own formula sheet

•  Research paper template is posted onto the research link –  Deadline for research paper submission is Monday, Nov. 25!!

•  Colloquium today –  4pm today, SH101, Dr. O. Auciello, UTD

•  Colloquium coming week –  4pm Monday, Nov. 4, SH101, Dr. Yujie Ding of Lehigh Univ.: Double extra credit –  4pm Wednesday, Nov. 6, SH101, Dr. David Nygren of Lorentz Berkeley National

Laboratory, Triple extra credit

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Wednesday, Oct. 30, 2013 PHYS 3313-001, Fall 2013 Dr. Jaehoon Yu

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Page 4: PHYS 3313 – Section 001 Lecture #14yu/teaching/fall13-3313-001/...Wednesday, Oct. 30, 2013 PHYS 3313-001, Fall 2013 Dr. Jaehoon Yu 2 Announcements • Homework #5 – CH6 end of

Wednesday, Oct. 30, 2013 PHYS 3313-001, Fall 2013 Dr. Jaehoon Yu

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Page 5: PHYS 3313 – Section 001 Lecture #14yu/teaching/fall13-3313-001/...Wednesday, Oct. 30, 2013 PHYS 3313-001, Fall 2013 Dr. Jaehoon Yu 2 Announcements • Homework #5 – CH6 end of

Special project #5 n Show that the Schrodinger equation

becomes Newton’s second law. (15 points) n Deadline Monday, Nov. 11, 2013 n You MUST have your own answers!

Wednesday, Oct. 30, 2013 5 PHYS 3313-001, Fall 2013 Dr. Jaehoon Yu

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Properties of Valid Wave Functions Boundary conditions 1)  To avoid infinite probabilities, the wave function must be finite

everywhere. 2)  To avoid multiple values of the probability, the wave function must be

single valued. 3)  For finite potentials, the wave function and its derivative must be

continuous. This is required because the second-order derivative term in the wave equation must be single valued. (There are exceptions to this rule when V is infinite.)

4)  In order to normalize the wave functions, they must approach zero as x approaches infinity.

Solutions that do not satisfy these properties do not generally correspond to physically realizable circumstances.

Wednesday, Oct. 30, 2013 6 PHYS 3313-001, Fall 2013 Dr. Jaehoon Yu

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Infinite Square-Well Potential •  The simplest such system is that of a particle trapped in a

box with infinitely hard walls that the particle cannot penetrate. This potential is called an infinite square well and is given by

•  The wave function must be zero where the potential is

infinite. •  Where the potential is zero inside the box, the time

independent Schrödinger wave equation becomes where .

•  The general solution is . Wednesday, Oct. 30, 2013 7 PHYS 3313-001, Fall 2013

Dr. Jaehoon Yu

V x( ) = ∞ x ≤ 0, x ≥ L0 0 < x < L

⎧⎨⎩

d 2ψdx2

= − 2mE2

ψ k = 2mE 2

ψ x( ) = Asin kx + Bcoskx= −k2ψ

2

2md 2ψ x( )dx2

+V x( )ψ x( ) = Eψ x( )

Page 8: PHYS 3313 – Section 001 Lecture #14yu/teaching/fall13-3313-001/...Wednesday, Oct. 30, 2013 PHYS 3313-001, Fall 2013 Dr. Jaehoon Yu 2 Announcements • Homework #5 – CH6 end of

Quantization •  Since the wave function must be continuous, the boundary conditions

of the potential dictate that the wave function must be zero at x = 0 and x = L. These yield valid solutions for B=0, and for integer values of n such that kL = nπ è k=nπ/L

•  The wave function is now

•  We normalize the wave function

•  The normalized wave function becomes

•  These functions are identical to those obtained for a vibrating string

with fixed ends. Wednesday, Oct. 30, 2013 8 PHYS 3313-001, Fall 2013

Dr. Jaehoon Yu

ψ n x( ) =

ψn

* x( )ψ n x( )−∞

+∞

∫ dx = 1

ψ n x( ) =

A2 sin2 nπ xL

⎛⎝⎜

⎞⎠⎟0

L

∫ dx = 1

Asin nπ xL

⎛⎝⎜

⎞⎠⎟

2Lsin nπ x

L⎛⎝⎜

⎞⎠⎟

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Quantized Energy •  The quantized wave number now becomes •  Solving for the energy yields

•  Note that the energy depends on the integer values of n.

Hence the energy is quantized and nonzero. •  The special case of n = 1 is called the ground state energy.

Wednesday, Oct. 30, 2013 9 PHYS 3313-001, Fall 2013 Dr. Jaehoon Yu

kn x( ) = nπL

=

En =

E1 =

π 22

2mL2

E2 =

2π 22

mL2

E3 =

9π 22

2mL2

2mEn

2

n2 π 22

2mL2 n = 1,2,3,( )

ψ n x( ) =2Lsin nπ x

L⎛⎝⎜

⎞⎠⎟

ψ n*ψ n = ψ n

2 =

2Lsin2 nπ x

L⎛⎝⎜

⎞⎠⎟

= 4E1

= 9E1

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How does this correspond to Classical Mech.? •  What is the probability of finding a particle in a box of length L? •  Bohr’s correspondence principle says that QM and CM must

correspond to each other! When? –  When n becomes large, the QM approaches to CM

•  So when nà∞, the probability of finding a particle in a box of length L is

•  Which is identical to the CM probability!! •  One can also see this from the plot of P!

Wednesday, Oct. 30, 2013 10 PHYS 3313-001, Fall 2013 Dr. Jaehoon Yu

P x( ) =ψn

* x( )ψ n x( ) = ψ n x( ) = 2L⋅ 12= 1L

1L

2Llimn→∞sin2 nπ x

L⎛⎝⎜

⎞⎠⎟ ≈

2Lsin2 nπ x

L⎛⎝⎜

⎞⎠⎟ =

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Determine the expectation values for x, x2, p and p2 of a particle in an infinite square well for the first excited state.

Ex 6.8: Expectation values inside a box

Wednesday, Oct. 30, 2013 11 PHYS 3313-001, Fall 2013 Dr. Jaehoon Yu

What is the wave function of the first excited state? n=? 2 ψ n=2 x( ) =

x n=2 =

x2n=2

=

p n=2 =

p2n=2

=

E2 =

2Lsin 2π x

L⎛⎝⎜

⎞⎠⎟

ψn=2

* x( )xψ n=2 x( ) =−∞

+∞

∫2L

xsin2 2π xL

⎛⎝⎜

⎞⎠⎟0

L

∫ dx =L2

2L

x2 sin2 2π xL

⎛⎝⎜

⎞⎠⎟0

L

∫ dx =0.32L2

2L

sin 2π xL

⎛⎝⎜

⎞⎠⎟ −i( ) ∂

∂xsin nπ x

L⎛⎝⎜

⎞⎠⎟

⎡⎣⎢

⎤⎦⎥0

L

∫ dx = −i 2

L2πL

sin 2π xL

⎛⎝⎜

⎞⎠⎟ cos

2π xL

⎛⎝⎜

⎞⎠⎟0

L

∫ dx = 0

2L

sin 2π xL

⎛⎝⎜

⎞⎠⎟ −i( )2 ∂2

∂x2sin 2π x

L⎛⎝⎜

⎞⎠⎟

⎡⎣⎢

⎤⎦⎥0

L

∫ dx = 22L2πL

⎛⎝⎜

⎞⎠⎟2

sin2 2π xL

⎛⎝⎜

⎞⎠⎟0

L

∫ dx =

4π 22

L2

4π 22

2mL2=

p2n=2

2m

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A typical diameter of a nucleus is about 10-14m. Use the infinite square-well potential to calculate the transition energy from the first excited state to the ground state for a proton confined to the nucleus.

Ex 6.9: Proton Transition Energy

Wednesday, Oct. 30, 2013 12 PHYS 3313-001, Fall 2013 Dr. Jaehoon Yu

The energy of the state n is

n=1 En = n

2 π 22

2mL2

What is n for the ground state?

E1 =

π 22

2mL2= 1

mc2π 2 ⋅ 197.3eV ⋅nm( )2

2 ⋅ 105nm( ) = 1.92 ×1015eV 2

938.3×106eV= 2.0MeV

E2 = 2

2 π 22

2mL2=

ΔE = E2 − E1 = 6.0MeV

What is n for the 1st excited state? n=2

So the proton transition energy is

π 22c2

2mc2L2=

8.0MeV


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