#Psi(x,t) = sqrt(1/L)sin((pix)/L) e^-(iomega_1t ) + sqrt(1/L)sin((2pix)/L) e^-(iomega_2t )#new question?

a) Calculate the probability distribution #P(x,t) = |ψ(x,t)|^2#
b) What is the period T
of this superposition – i.e., after what time T will the system return to its original configuration?
c) Find the probability distribution P(x,t) evaluated at time# t_∗ = π /[2(E1−E0)].#
What fraction of T is #t_∗#?
d) What’s the probability that you find the particle in the left half of the well at
some arbitrary time t?
e) Find the expectation value #<x># of the particle’s position as a function of time
f) Show that the probability density P(x,t) at x = L/2 is independent of time.

1 Answer
Mar 4, 2018

#a)#

You just need to take #Psi^"*"Psi#.

#color(blue)(Psi^"*"Psi) = [sqrt(1/L)sin((pix)/L) e^-(iomega_1t ) + sqrt(1/L)sin((2pix)/L) e^-(iomega_2t)]^"*" [sqrt(1/L)sin((pix)/L) e^-(iomega_1t ) + sqrt(1/L)sin((2pix)/L) e^-(iomega_2t )]#

#= [sqrt(1/L)sin((pix)/L) e^(iomega_1t ) + sqrt(1/L)sin((2pix)/L) e^(iomega_2t)][sqrt(1/L)sin((pix)/L) e^-(iomega_1t ) + sqrt(1/L)sin((2pix)/L) e^-(iomega_2t)]#

#= 1/Lsin^2((pix)/L) + 1/L ((pix)/L)sin((2pix)/L)e^(i(omega_1-omega_2)t) + 1/L sin((pix)/L)sin((2pix)/L)e^(i(omega_2-omega_1)t) + 1/L sin^2((2pix)/L)#

#= color(blue)(1/L[sin^2((pix)/L) + sin^2((2pix)/L)] + 1/L sin((pix)/L)sin((2pix)/L)[e^(i(omega_1-omega_2)t) + e^(i(omega_2-omega_1)t)])#

#b)#

The period can be found with minimal effort, simply by first knowing the energies, which are constants of the motion.

The energy of #phi_1 = sqrt(1/L)sin((pix)/L)# is #E_1 = (1^2pi^2ℏ^2)/(4mL^2)#, and the energy of #phi_2# is #4E_1#. Therefore, the frequency #omega_2# of #phi_2# is four times that of #phi_1# (#omega_1#).

As a result, the period #T_1 = (2pi)/(omega_1)# of #phi_1# is four times that of #phi_2# (#T_2 = (2pi)/(omega_2)#, and is also a period of #phi_2#.

The period is thus #color(blue)(T = (2pi)/(omega_1))#.

#c)#

I'll let you plug this one in yourself as #t_"*" = pi /[2(E_2−E_1)]#. You don't need to do anything with it...

We know that #T = (2pi)/(omega_1)#, and that #(iEt)/ℏ = iomegat#, so

#E_n = omega_nℏ#.

As a result,

#pi/(2(E_2-E_1)) = pi/(2(omega_2-omega_1)ℏ)#

and

#color(blue)(t_"*"/T) = pi/(2(omega_2-omega_1)ℏ) cdot (omega_1)/(2pi)#

#= 1/(2(4omega_1-omega_1)ℏ) cdot (omega_1)/(2)#

#= omega_1/(4ℏ(3omega_1))#

#= color(blue)(1/(12ℏ))#

#d)#

The probability of finding the particle in #[0, L/2]# is given as

#int_(0)^(L/2) Psi^"*"Psidx#

#= 1/Lint_(0)^(L/2) sin^2((pix)/L) + sin^2((2pix)/L)dx + 1/Lint_(0)^(L/2) sin((pix)/L)sin((2pix)/L)[e^(-3iomega_1t) + e^(3iomega_1t)]dx#

#= 1/Lint_(0)^(L/2) sin^2((pix)/L) + sin^2((2pix)/L)dx + 1/Lint_(0)^(L/2) 2sin((pix)/L)sin((2pix)/L)cos(3omega_1t)dx#

The first two terms are symmetric with half the amplitude, and yield #50%# overall.

The third term would have a stationary state probability of #4/(3pi)#, and #cos# is an arbitrary phase factor. Thus, the overall probability is

#= color(blue)(0.50 + 4/(3pi) cos(3omega_1t))#

#e)#

#color(blue)(<< x >>) = << Psi | x | Psi >> = << xPsi|Psi >>#

#= 1/Lint_(0)^(L/2) xsin^2((pix)/L)dx + 1/Lint_(0)^(L/2) xsin^2((2pix)/L)dx + 1/Lint_(0)^(L/2) 2xsin((pix)/L)sin((2pix)/L)cos(3omega_1t)dx#

There is no trivial solution to this... This turns out to be:

#= L/(4pi^2) + L/8 + [(2L)/(3pi) - (8L)/(9pi^2)]cos(3omega_1t)#

#= color(blue)(((2 + pi^2)L)/(8pi^2) + [((6pi - 8)L)/(9pi^2)]cos(3omega_1t))#

#f)#

At #x = L/2#, the #sin# terms go to #sin(pi/2) = 1# and to #sin(pi) = 0#, respectively.

Since #sin(pi) = 0#, the time-dependent part of #Psi^"*"Psi# vanishes and the time-independent part retains #1/L# as the probability density.