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PHYS-3301 Lecture 11 HW4 (due 10/5) Chapter4 13, 15, 20 ...

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PHYS-3301 Oct. 3, 2017 Lecture 11 Announcement Course webpage http://www.phys.ttu.edu/~slee/3301/ Textbook HW4 (due 10/5) Chapter 4 13, 15, 20, 31, 36, 41, 48, 53, 63, 66 Exam 1 (10/5) Chapters 2, 3, & 4 Chapter. 5 Bound States: Simple Case Purpose: To make QM useful in real application, we must have a way to account for the effects of external forces** Let’s start with the Schrödinger eq. to include these effects. ** interaction of object with its surrounding Rainer Weiss Kip S. Thorne Barry C. Barish "for decisive contributions to the LIGO detector and the observation of gravitational waves"
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Page 1: PHYS-3301 Lecture 11 HW4 (due 10/5) Chapter4 13, 15, 20 ...

PHYS-3301

Oct. 3, 2017

Lecture 11

Announcement

Course webpage

http://www.phys.ttu.edu/~slee/3301/

Textbook

HW4 (due 10/5)

Chapter 413, 15, 20, 31, 36, 41, 48, 53, 63, 66

Exam 1 (10/5) Chapters 2, 3, & 4

Chapter. 5Bound States: Simple Case

Purpose:

• To make QM useful in real application,• we must have a way to account for the effects of

external forces**Let’s start with the Schrödinger eq. to include theseeffects.

** interaction of object with its surroundingRainer Weiss Kip S. Thorne Barry C. Barish

"for decisive contributions to the LIGO detector and the observation of gravitational waves"

Page 2: PHYS-3301 Lecture 11 HW4 (due 10/5) Chapter4 13, 15, 20 ...

Chapter. 5Bound States: Simple Case

Outline:

• The Schrödinger Equation (for interacting particles)• Stationary States• Physics Conditions: Well-Behaved Functions• A Review of Classical Bound States• Case 1: Particles in a Box – The Infinite Well• Case 2: The Finite Well• Case 3: The Simple Harmonic Oscillator• Expectation Values, Uncertainties, and Operators

Page 3: PHYS-3301 Lecture 11 HW4 (due 10/5) Chapter4 13, 15, 20 ...

The Schrodinger Equation

for Interacting Particles

A Particle Interacting

With What?

F=mg

The Schrodinger Equation

for Interacting Particles

A Particle Interacting

With What?

Simplification:

The Concept of Potential(replaces all individual

particle-particle interactions

with a single smooth potential)Why? – see next page

Smooth & Stationary

Function

Energy vs. Position for a mass connected to a spring

Page 4: PHYS-3301 Lecture 11 HW4 (due 10/5) Chapter4 13, 15, 20 ...

In Quantum Mechanics –

Bound States are Standing

Waves

Bound states is one in which a particle's motion is restricted by an external force to finite region of space

In Quantum Mechanics –

Bound States are Standing

Waves

Not

forbidden

In Quantum Mechanics –

Bound States are Standing

Waves

Not

forbidden

The

“Ground state”

the lowest

energy state

is not

at E=0

The

“Ground state”

- the lowest

energy state

is not

at E=0

Consistent with the

Uncertainty Relations:

2

!!""

xpx

Page 5: PHYS-3301 Lecture 11 HW4 (due 10/5) Chapter4 13, 15, 20 ...

Bound SystemsA bound system: any system of interacting particles where the nature of the interactions between the particles keeps their relative separation limited. Classical example: the solar system.

Classical bound system: ( ) ( ) ( )E x K x U x= +

Classically allowed region:

( ) ( )E x U x<

( ) ( )E x U x>

Classically forbidden region:

( ) 0K x >

( ) ( )E x U x=

In general, the problem is very difficult.

Simplification: motion of a single particle that moves in a fixed potential energy field U(x). The mass of the particle is small compared to the total mass of the system (e.g. heavy nucleus - light electron).

Δx

The Infinite Square Wella particle in the potential is completely free, except at the two ends where an infinite force prevents it from escaping

Outside the well: ( ) 0xψ = - the probability of finding the particle =0

Inside the well:( ) ( )

22

22d x

E xm dx

ψψ− =

h

( ) ( )2

22

d xk x

dxψ

ψ= − 2mEk ≡h

- the harmonic oscillator equation

( ) sin cosx A kx B kxψ = + - constants A and B are fixed by boundary conditions

( ) ( )0 0Lψ ψ= =Continuity of the wave function: ( )0 sin 0 cos 0 0A k B k Bψ = + = =

( ) sinx A kxψ =

General solution:

Thus, ( ) sin 0L A kLψ = = 0, , 2 ,...kL π π= ± ±

, 1,2,...nnk nLπ

= =

n – quantum number (1D motion ischaracterized by a single q.n., for 2D motionwe need two quantum numbers, etc.)

See later for details

The Schrodinger Equation

for Interacting Particles

Try to add potential energy U(x)

For free

particles

Aei(kx-wt) or in the absence of external forces

Schrödinger eq. is based on E accounting - w/o external interactions

Adding P.E.

èTime-dependent Schrödinger Eq.è To determine the behavior of particle

in (1) CM: solve F = m(d2r/dt2) for r, given knowledge of Net external F on particlein (2) QM: solve the Schrödinger eq. for ψ(x,t), given knowledge of P.E., U(x)

Page 6: PHYS-3301 Lecture 11 HW4 (due 10/5) Chapter4 13, 15, 20 ...

The Schrodinger Equation

for Interacting Particles

and for

Stationary Potentials

)(

)(

tUU

xUU

!

=

Key Assumption:

Factorization of the wave function

Spatial Part Temporal Part

What happens with the Schrodinger equation?

Standard Math. Technique;

“Separation of variables”Wave function may be

express as a product of …

Q: Why?, A: allows us to break a differential eq. with 2 independent variables (x,t) into simpler eqs. For position & time, separately!!

… and factoring out terms constant w.r.t. the partial derivatives …

Divide both sides by ψ(x)φ(t)

Variables are separate now!!

t and x are independent

Separation ConstantConsider only case in which P.E. is time-independent

Solution(see Appendix K) Aei(kx-ωt) ~ Ae-iωt , ω = C/h

The Temporal Part, φ(t)

Page 7: PHYS-3301 Lecture 11 HW4 (due 10/5) Chapter4 13, 15, 20 ...

Temporal part

Total wave

function

Temporal part

Total wave

function

The probability density is

time-independentStationary

States

Oops!! Its time dependence disappears!!

i.e. the whereabouts of the particle don’t change with time in any observable way

Temporal part

Total wave

function

The probability density is

time-independentStationary

States

Oops!! Its time dependence disappears!!

Quantum Mechanically, electron is not an accelerating charged particles, but rather a stationary “cloud”

The spatial part of !(!(!(!(x,t)

The time-independent

Schrodinger equation:

!(!(!(!(x) is Real,

but !(!(!(!(x,t) is Complex, because

"("("("(t)=e-i####t

NOTE:

Spatial part

Replace C by E, multiply both sides by ψ(x);


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