Remember:
This is the system: We will see how it changes, and how we can represent the vector field, at different values of .
To have a better understanding on how you can calculate the vector field, and nullclines aslo refer to this other example.
First we represent , this is its vector field:
is a steady state
We can represent the flow of in its vector field:
- On the left of the steady state, we have that , then the flow will point to the right.
- On the right of the steady state, we have that , then the flow will point to the left.
- We can conclude that is a stable steady state.
Now we can study , for :
- Like before the vector field and so the flow are very similar.
Letβs combine this two solutions, and letβs draw the nullclines, so letβs find for and , so:For this case preatty simple, letβs draw the nullclines:
Then we can we can represent the flow (for ):
Note that:
- For we have that the flow will be parallel to the axis.
- For (the ss) we have that the flow will be parallel to the axis.
If we represent the βmotion of a family of particlesβ (the flow ):
- This form is becasue , so the velocity along is higher than the velocity along .
- The velocities we said can be seen as and .
If we take :
- The form slightly changes since now, the velocity along is lower than the velocity along .
Special case for :
- In all of these cases this steady state is called a βnodeβ.
- In this particular case, it is called a βnode starβ
Instead for :
This is an unstable steady state, since:
The nullclines changes:
If we represent for :
- All initial condition will diverge, except and initial condition such that it lies along the axis, so for .
- For the system will converge to .
- For the system will diverge .
- So one component converges and the other diverges, when that is the case we obtain this graph, called a βsaddleβ, name taken from the form of the vector field.
Another special case: for :
We cannot represent any arrow, and it said to be marginally stable. And the flow for :
- Called βline of steady statesβ.


- This is a special linear system, depends only on and depends only on .

- General case.
If we solve analytically we find:We can define:And we can find:However remeber, that we will not find analytic solutions.
We can represent the graph :
- is a steady state.
Letβs represent the flow:
On the right of the ss (steady state) the derivitave over time () is positive.
While on the left , so:
- As we can see is a stable steady state.
Now we can study , notice that can assume different values, mainly we will focus on and for .
For , basically the graph is the same as before (for ):
Letβs combine this two solutions, and letβs draw the nullclines, so letβs find for and , so:For this case preatty simple, letβs draw the nullclines:
Now we can represent the flow:
- For we have that the flow will be parallel to the axis.
- For (the ss) we have that the flow will be parallel to the axis.
If we represent the βmotion of a family of particlesβ (the flow ):
- This form is becasue , so the velocity along is higher than the velocity along .
- The velocities we said can be seen as and .
If we take :
Special case for :
- In all of these cases the node is called βnodeβ.
- In this particular case, it is called a βnode starβ
Letβs see what happens for :
- This is an unstable steady state, since:
The nullclines changes:
If we represent : 
- All initial condition will diverge, except and initial condition such that it lies along the axis, so for .
- For the system will converge to .
- For the system will diverge.
- So one component converges and another diverges, for this reason this graph is called a βsaddleβ, sincenot-sure-about-this
For :
- We cannot represent any arrow, and it said to be marginally stable.
And the flow for :
- Called βline of steady statesβ.
As a sneak-peak for the future, in this system we can define the eigenvalues as: and , the sign of the eigenvalues is strictly correleted to the stability of the steady states.