An unstable node has
Both linear modes grow forward in time. Nearby nonconstant orbits move away from the equilibrium, and approach it under reversed time; their local directions come from the two real eigenvectors.
A stable node has
Both exponential modes decay as , so the equilibrium is asymptotically stable. Generic linear orbits approach tangent to the eigenvector for the less negative eigenvalue; the eigenvector directions themselves are invariant straight lines. There is no rotation because both eigenvalues are real.
Suppose, towards a contradiction, that for some the punctured-disk image misses the open disk of radius about . Then
is holomorphic and bounded by on . Part (i) extends it to a holomorphic function on the full disk. If , then extends holomorphically at zero, making zero a removable singularity.
If , the function is not identically zero, since it is nonzero on the punctured disk. The Taylor series and identity theorem give a finite zero order , so with holomorphic and . Hence
has a pole of order . Both alternatives contradict an essential singularity. Consequently
This is the Casorati-Weierstrass theorem: every complex value can be approximated arbitrarily closely in every punctured neighbourhood of an essential singularity.
Take the Laurent series of on . For every integer , its coefficient of satisfies, on a circle of radius ,
The coefficient is independent of . Letting therefore gives for every . The Laurent series is a power series with no negative powers and supplies a holomorphic extension at zero. Thus zero is a removable singularity. This is the Riemann removable singularity theorem, with boundedness used to eliminate the entire principal part.
An essential singularity is an isolated singularity that is neither a removable singularity nor a pole. In its Laurent series, infinitely many coefficients of negative powers are nonzero. The alternatives follow because no negative terms give a removable singularity, while finitely many with a lowest nonzero power give a pole.
A pole of order means
Equivalently, the Laurent series has a finite nonzero principal part, with lowest power exactly . Thus extends holomorphically with nonzero value at ; using a smaller positive power would not remove the singularity.
The point is a removable singularity if assigning a value to makes holomorphic on a full neighbourhood of . Equivalently, its Laurent series has no nonzero coefficients of negative powers. The assigned value is its constant coefficient, or equivalently the finite limit .
An isolated singularity at means that some radius has holomorphic on the punctured disk , while is not initially defined as a holomorphic function at . The adjective isolated refers to the absence of other singularities in this punctured neighbourhood; it permits a removable singularity.
Either equality condition says that the holomorphic function from part (i) has modulus one at an interior point: at zero in the derivative case, or at the given nonzero point in the other case. Since everywhere, the maximum modulus principle makes a constant with . Therefore
These maps are rotations of the unit disk and do achieve both equalities, so this also identifies all equality cases of the Schwarz lemma.
Because , the Taylor series of at zero shows that
is holomorphic throughout the unit disk. Fix . On we have , and the maximum modulus principle on the closed disk of radius gives for . For any fixed inside the unit disk we may let increase to one, obtaining . Hence the Schwarz lemma inequalities are
The derivative bound is the same estimate at , using the holomorphic extension of the quotient.
The closed unit disk is a compact set, and is continuous on it because is holomorphic on an open neighbourhood. The extreme value theorem therefore supplies a point where its maximum is attained. If such a point is on the boundary, the conclusion follows. If it is in the interior, part (i) makes constant on the open disk; continuity then gives the same value on the boundary. Consequently
The assumption that the closed disk lies in is what makes the boundary values and the compactness argument available.
Write . The local maximum property gives a disk around on which , contained in the unit disk. If , then on that neighbourhood, and the identity theorem makes zero on the connected unit disk.
Otherwise multiply by the unit complex number , obtaining a holomorphic function with and nearby. Applying the Cauchy integral formula on any sufficiently small circle of radius gives the mean value property
Take real parts. The continuous function is nonnegative on the circle and has integral zero, so it vanishes everywhere there. Since , having real part forces imaginary part zero. Thus throughout the circle. The zeros of have an accumulation point inside its domain, so the identity theorem gives constant on the entire unit disk. This proves the local maximum modulus principle directly from the Cauchy integral formula.
Differentiating the transform with respect to gives
Applying this to also gives for .
Now put , and . Transforming each term of the differential equation, and using the derivative identities, gives
The initial-value terms cancel, leaving
Integrating once yields . Partial fractions give
The transform pairs therefore imply, on writing ,
For the final parameter count, the differential equation is the derivative of : it says . Integrating gives . A regular solution at has finite and , forcing . Thus is first order and leaves only one constant. Equivalently, the original equation at zero requires , so the two usual initial values cannot be chosen independently. The displayed solution satisfies this constraint and verifies the original equation directly.
Integration by parts, where the transform boundary term at infinity vanishes, gives
For a sufficiently regular function with the required exponential growth bounds, apply this again to to deduce
These identities hold in a right half-plane where the displayed transforms converge; the regular solutions obtained below satisfy those requirements.
The Laplace transform is
A sufficient condition is that be piecewise continuous on each bounded interval and of exponential order , meaning for all sufficiently large . Then the integral is absolutely convergent for , by comparison with .
For the constant function, direct integration gives
The same quotient is unbounded near , so the uniform Lipschitz hypothesis again fails. Two explicit solutions through the initial point are
For the second, put . Then , and . The real power here means the square of the real cube root, so the identity also holds when is negative. Both functions are differentiable through their zeros. Thus uniqueness fails in this case as well.
No rectangle of positive width around has a uniform Lipschitz constant in . For any nonzero in such a rectangle,
The vanishing factor at the single initial point does not control neighbouring -values. The failure of the hypothesis is accompanied by actual nonuniqueness: both
satisfy the equation and have value zero at . Direct differentiation gives , including the zero point by continuity.
First prove the general uniqueness claim. The bound prevents a solution from leaving the dependent-variable interval before : up to any first exit, . Let be two solutions with the same initial value. Their integral equations and the Lipschitz condition give, for ,
Since their difference is bounded by , repeated substitution into this inequality proves, for every integer ,
The same argument with reversed limits works for . Letting forces the difference to zero on the whole interval. This proves at most one solution without assuming that .
For case (i), choose a rectangle around that stays in . There is bounded, giving a uniform Lipschitz constant by the mean value theorem. For example works: and . Separate variables using , obtaining . The initial condition gives , hence
It remains positive for all real , so the same local uniqueness argument continues along this solution.
For each triangle compactly contained in , part (i) permits the interchange of the series and its boundary integral. Cauchy's integral theorem makes every term zero. The uniform limit is continuous, so Morera's theorem yields that is holomorphic on .
For the final application, each function is holomorphic away from its pole. Fix a positive integer . For and ,
The numerical series converges, so the Weierstrass M-test gives uniform convergence of the tail on . Adding the finitely many initial terms preserves uniform convergence. Those initial terms need not be bounded near their excluded poles; only the tail needs the uniform bound. By the first conclusion, the full sum is holomorphic on each . Their union is , hence

Pinned article: Introduction to the OurBigBook Project

Welcome to the OurBigBook Project! Our goal is to create the perfect publishing platform for STEM subjects, and get university-level students to write the best free STEM tutorials ever.
Everyone is welcome to create an account and play with the site: ourbigbook.com/go/register. We belive that students themselves can write amazing tutorials, but teachers are welcome too. You can write about anything you want, it doesn't have to be STEM or even educational. Silly test content is very welcome and you won't be penalized in any way. Just keep it legal!
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    • a Q&A website like Stack Overflow, where multiple people can give their views on a given topic, and the best ones are sorted by upvote. Except you don't need to wait for someone to ask first, and any topic goes, no matter how narrow or broad
    This feature makes it possible for readers to find better explanations of any topic created by other writers. And it allows writers to create an explanation in a place that readers might actually find it.
    Figure 1.
    Screenshot of the "Derivative" topic page
    . View it live at: ourbigbook.com/go/topic/derivative
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    Figure 5. . You can also edit articles on the Web editor without installing anything locally.
    Video 3.
    Edit locally and publish demo
    . Source. This shows editing OurBigBook Markup and publishing it using the Visual Studio Code extension.
  3. https://raw.githubusercontent.com/ourbigbook/ourbigbook-media/master/feature/x/hilbert-space-arrow.png
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