Skip to content
GitLab
Explore
Sign in
Register
Primary navigation
Search or go to…
Project
L
lectures
Manage
Activity
Members
Labels
Plan
Issues
Issue boards
Milestones
Wiki
Code
Merge requests
Repository
Branches
Commits
Tags
Repository graph
Compare revisions
Snippets
Build
Pipelines
Jobs
Pipeline schedules
Artifacts
Deploy
Releases
Container Registry
Model registry
Operate
Environments
Monitor
Incidents
Service Desk
Analyze
Value stream analytics
Contributor analytics
CI/CD analytics
Repository analytics
Model experiments
Help
Help
Support
GitLab documentation
Compare GitLab plans
Community forum
Contribute to GitLab
Provide feedback
Keyboard shortcuts
?
Snippets
Groups
Projects
Show more breadcrumbs
Mathematics for Quantum Physics
lectures
Merge requests
!9
DifferentialEquationsLecture2
Code
Review changes
Check out branch
Download
Patches
Plain diff
Merged
DifferentialEquationsLecture2
DE2
into
master
Overview
0
Commits
41
Pipelines
23
Changes
1
Merged
Scarlett Gauthier
requested to merge
DE2
into
master
4 years ago
Overview
0
Commits
41
Pipelines
23
Changes
1
Expand
Add lecture notes from the second lecture on differential equations.
Edited
4 years ago
by
Michael Wimmer
0
0
Merge request reports
Viewing commit
7efa29ae
Prev
Next
Show latest version
1 file
+
54
−
2
Inline
Compare changes
Side-by-side
Inline
Show whitespace changes
Show one file at a time
7efa29ae
Finish example of page 6.
· 7efa29ae
Scarlett Gauthier
authored
4 years ago
src/differential_equations_2.md
+
54
−
2
Options
@@ -348,10 +348,62 @@ operator and $\phi(x)$ is the eigenfunction.
Notice that when stating the ordinary differential equation, it is specified
along with it's boundary conditions. Note that in contrast to an initial value
problem, a boundary value problem does not always have a solution.
problem, a boundary value problem does not always have a solution. For example,
in the figure below, regardless of the initial slope, the curves never reach $0$
when $x=L$.
<img
src=
"figures/DE2_1.png"
width=
"
70
0"
>
<img
src=
"figures/DE2_1.png"
width=
"
65
0"
>
For boundary value problems like this, there are only solutions for particular
eigenvalues $
\l
ambda$. Coming back to the example, it turns out that solutions
only exist for $
\l
ambda>0$ --this can be shown quickly, feel free to try it!
Define for simplicity $k^2:=
\f
rac{2m
\l
ambda}{
\h
bar^2}$. The equation then
reads
$$
\p
hi''(x)+k^2
\p
hi(x)=0.$$
Two linearly independent solutions to this equation are
$$
\p
hi_{1}(x)=sin(k x),
\ \p
hi_{2}(x) = cos(k x).$$
The solution to this homogeneous equation is then
$$
\p
hi(x)=c_1
\p
hi_1(x)+c_2
\p
hi_2(x).$$
The eigenvalue, $
\l
ambda$ as well as one of the constant coefficients can be
determined using the boundary conditions.
$$
\p
hi(0)=0
\ \R
ightarrow
\ \p
hi(x)=c_1 sin(k x),
\
c_2=0.$$
$$
\p
hi(L)=0
\ \R
ightarrow
\
0=c_1 sin(k L) .$$
In turn, using the properties of the $sin(
\c
dot)$ function, it is now possible
to find the allowed values of $k$ and hence also $
\l
ambda$. The previous
equation implies,
$$k L = n
\p
i,
\
n
\ \e
psilon
\ \m
athbb{N}$$
$$
\l
ambda_n =
\b
ig{(}
\f
rac{n
\p
i
\h
bar}{L}
\b
ig{)}^2.$$
The values $
\l
ambda_n$ are the eigenvalues. Now that we have determined
$
\l
ambda$, it enters into the time equation, $i
\h
bar
\d
ot{f}(t) =
\l
ambda f(t)$
only as a constant. We can hence simply solve,
$$
\d
ot{f}(t) = -i
\f
rac{
\l
ambda}{
\h
bar} f(t)$$
$$f(t) = A e^{
\f
rac{-i
\l
ambda t}{
\h
bar}}.$$
In the previous equation, the coefficient $A$ can be determined if the original
PDE was supplied with an initial condition.
Putting the solutions to the two ODEs together and redefining
$
\T
ilde{A}=A
\c
dot c_1$, we arrive at the solutions for theb PDE,
$
\p
si_n(x,t) =
\T
ilde{A} e^{-i
\f
rac{
\l
ambda_n t}{
\h
bar}} sin(
\f
rac{n
\p
i x}{L}).$
Notice that there is one solution $
\p
si_{n}(x,t)$ for each natural number $n$.
These are still very special solutions. We will begin discussing next how to
obtain the general solution in our example.
Loading