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Physics 130b: Lecture Time Evolution § Time Evolution Observables The state vector Spin precession

Physics 130b: Lecture Time Evolution

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Page 1: Physics 130b: Lecture Time Evolution

Physics 130b: LectureTime Evolution

§Time Evolution–Observables–The state vector–Spin precession

Page 2: Physics 130b: Lecture Time Evolution

Spin Angular Momentum

𝑆!| ⟩𝑠 𝑚 = ℏ!𝑠 𝑠 + 1 | ⟩𝑠 𝑚

𝑆"| ⟩𝑠 𝑚 = ℏ𝑚| ⟩𝑠 𝑚

𝑆±| ⟩𝑠 𝑚 = ℏ 𝑠 𝑠 + 1 −𝑚 𝑚 ± 1 | ⟩𝑠 𝑚 ± 1

𝑆± = 𝑆$ ± 𝑖𝑆%

Page 3: Physics 130b: Lecture Time Evolution

Clicker Question 1

Page 4: Physics 130b: Lecture Time Evolution

Clicker Question 2

Page 5: Physics 130b: Lecture Time Evolution

Matrix Representation of Operators

𝐴 ≐ ↑ 𝐴 ↑ ↑ 𝐴 ↓↓ 𝐴 ↑ ↓ 𝐴 ↓

↑ 𝐴 ↑

Page 6: Physics 130b: Lecture Time Evolution

Student Questions§ I'm not clear on what equation 2.4 is listing, the "explicit labelling of the

rows.”

Page 7: Physics 130b: Lecture Time Evolution

Let’s find 𝑆-𝑆!| ⟩↑ = ℏ

#| ⟩↑ 𝑆!| ⟩↓ = -

ℏ#| ⟩↓

Page 8: Physics 130b: Lecture Time Evolution

Let’s find 𝑆-𝑆!| ⟩↑ = ℏ

#| ⟩↑ 𝑆!| ⟩↓ = -

ℏ#| ⟩↓

An operator is always diagonal in it’s own basis. Eigenvectors are unit vectors in their own basis.

Page 9: Physics 130b: Lecture Time Evolution

Phys3220, U.Colorado at Boulder151

The raising operator operating on the up and down spin states:

0, =­­=¯ ++ SS !

What is the matrix form of the operator S+ ?

A) B) C)÷÷ø

öççè

æ0110

! ÷÷ø

öççè

æ0010

! ÷÷ø

öççè

æ0100

!

D) E) None of these÷÷ø

öççè

æ1110

!

Clicker Question 3

Page 10: Physics 130b: Lecture Time Evolution

Phys3220, U.Colorado at Boulder149

In spin space, the basis states (eigenstates of S2,

Sz ) are orthogonal:

Are the following matrix elements zero or non-zero?

A) Both are zeroB) Neither are zeroC) The first is zero; second is non-zeroD) The first is non-zero; second is zero

.0=¯­

¯­¯­ zSS 2Clicker

Question 4

Page 11: Physics 130b: Lecture Time Evolution
Page 12: Physics 130b: Lecture Time Evolution

Example

Page 13: Physics 130b: Lecture Time Evolution

𝑆!| ⟩𝑠 𝑚 = ℏ!𝑠 𝑠 + 1 | ⟩𝑠 𝑚

𝑆"| ⟩𝑠 𝑚 = ℏ𝑚| ⟩𝑠 𝑚

Page 14: Physics 130b: Lecture Time Evolution

Rules of Quantum Mechanics6) The time evolution of a quantum system is determined

by the Hamiltonian of total energy operator 𝐻 𝑡 through the Schrodinger equation

𝑖ℏ !!"| ⟩𝜓 𝑡 = 𝐻 𝑡 | ⟩𝜓 𝑡

Page 15: Physics 130b: Lecture Time Evolution

SE

𝐻 | ⟩𝐸# = 𝐸# | ⟩𝐸#

𝑖ℏ !!"| ⟩𝜓 𝑡 = 𝐻 | ⟩𝜓 𝑡

| ⟩𝜓 𝑡 =,#

𝑐#𝑒$%&&"/ℏ| ⟩𝐸#

Page 16: Physics 130b: Lecture Time Evolution

Time-dependent RecipeBelow is the recipe for solving a standard time-

dependent quantum mechanics problem with a time dependent Hamiltonian.

Given1. Diagonalize 𝐻 to determine the energy eigenvectors

and energy eigenvalues2. Write in terms of the energy eigenvectors:3. Multiply each eigenvector by 4. Calculate (prob. of various observables)

)0(y

)0(y!/tiEne-

Page 17: Physics 130b: Lecture Time Evolution

General Procedure (for time independent potentials)

Given V(x) and Y(x,0)1. Solve TISE and find eigenfunctions yn (x) and

eigenvalues En associated with V(x) 2. Write in Y(x,0) terms of the eigenstates:

3. Multiply each eigenfunction by to get

4. Calculate (prob. of various observables)

!/tiEne-å¥

=

=Y1

)()0,(n

nn xcx y

å¥

=

-=Y1

/)(),(n

tiEnn

nexctx !y

Page 18: Physics 130b: Lecture Time Evolution

Electron in Uniform B-Field

Page 19: Physics 130b: Lecture Time Evolution

An electron in a magnetic field 𝐵 = 𝐵!�̂� is initially in a spin state ⟩|χ(0) = 𝑎 ⟩|↑ " + 𝑏 ⟩|↓ ". Which of the following equations correctly

represents the state ⟩|χ(𝑡) of the electron after time t? The Hamiltonian operator is 1𝐻 = −𝛾𝐵! 5𝑆".

A. ⟩|χ(𝑡) = 𝑒#$%!&/( 𝑎 ⟩|↑ " + 𝑏 ⟩|↓ "

B. ⟩|χ(𝑡) = 𝑒)#$%!&/( 𝑎 ⟩|↑ " + 𝑏 ⟩|↓ "

C. ⟩|χ(𝑡) = 𝑒#$%!&/( (𝑎 + 𝑏) ⟩|↑ " + (𝑎 − 𝑏) ⟩|↓ "

D. ⟩|χ(𝑡) = 𝑎𝑒#$%!&/( ⟩|↑ " + 𝑏𝑒)#$%!&/( ⟩|↓ "

E. None of the above

Clicker Question 5: