Let be the time at which a right-running characteristic curve leaves the piston. The boundary velocity and the characteristic it emits are
With
these relations become
Because and , is single-valued and -periodic behind the wavefront. Ahead of the first characteristic, where , the fluid remains undisturbed and . The implicit relation is Kepler equation; unless , its inverse is not a pure sinusoid.
Series reversion gives
Expanding the cosine then gives
and hence
For
the adiabatic sound speed is
Since , choose invariants that vanish in the equilibrium state :
Consequently
In a right-moving simple wave with , the characteristic speed is therefore , independent of amplitude. The transport equation becomes , so the whole velocity profile translates rigidly at the equilibrium sound speed without nonlinear distortion.
A real transmitted normal wavenumber exists only if
so the critical angle for total internal reflection is
For , put
For incident amplitude , the transverse-electric Fresnel reflection coefficient and transmission coefficient are
A boundary-matched solution is
with each magnetic component obtained from , now using the complex transmitted wavevector . Since , the wave undergoes total internal reflection; the transmitted field is an evanescent wave that propagates parallel to the interface and decays exponentially into .
The condition , together with transversality , selects polarization along away from the normal-incidence degeneracy. Phase matching at a planar wave interface gives
The two dispersion relations give . Choosing propagation into therefore yields
Equivalently, this is Snell law for electromagnetic waves with refractive index proportional to because the two media have equal magnetic permeability.
For each , substitution of a complex plane electromagnetic wave in a linear medium into the source-free Maxwell equations in a linear medium requires
where and . The accompanying magnetic field is
The incident and transmitted waves have and , while the reflected wave has . Matching the fields at the stationary interface additionally imposes the phase matching at a planar wave interface conditions and equality of all tangential wavevector components.
For a time-independent field, Faraday's law gives . Integrating around a thin rectangular loop crossing and shrinking its height gives continuity of the tangential component:
A thin Gaussian pillbox and give continuity of the normal electric displacement field:
These are the electrostatic cases of the dielectric-interface boundary conditions.
For , the angular momentum operator gives
The probability density is proportional to
whose maximum occurs at
In a large disk of area , the states that fit inside satisfy . Thus the degeneracy of each Landau level is asymptotically
where is the magnetic flux. There is one state per magnetic flux quantum , up to boundary corrections.
Let be the kinetic momentum. The quantum Hamiltonian is
Assume and zero longitudinal momentum, as in the displayed states. Since
we have and
For ,
which annihilates every
with holomorphic. Hence all these states have
The Landau levels are for ; the arbitrary holomorphic function exhibits the degeneracy of the lowest level. For , the normalizable lowest-level states are anti-holomorphic instead.
These potentials give the uniform magnetic field and zero electric field. With the signed frequency , the Lorentz force law becomes
Thus
and explicitly
The transverse trajectory is a circle about the fixed guiding centre . The positive cyclotron frequency is
For , all orbits converge to one fixed point, and for every orbit is eventually fixed or period two, so no iterate has a horseshoe. For the symmetric tent map with slope magnitude , the topological entropy is . The interval-map positive-entropy horseshoe theorem says that a continuous interval map has positive topological entropy exactly when some iterate has a horseshoe. Hence
For this already follows from part (iii); for , a higher iterate supplies the horseshoe.
The map itself has a horseshoe only for . Indeed, its Lipschitz constant is . If two intervals form a horseshoe and their convex hull has length , then
which forces . At , take , and ; both map onto .
The Lipschitz constant of is , so the same length argument makes necessary for an horseshoe. It is sufficient. Put
For , one has . With
the two relevant monotone branches satisfy
Thus are disjoint and . Therefore
For , one iterate sends the whole interval into , where
This is a contraction mapping with unique fixed point
Every orbit converges to , alternating around it because the multiplier is .
For , the first iterate lies in and there. Hence is the identity on : is fixed, while every other point in that interval belongs to the period-two orbit .
The graph of is the symmetric tent with vertices
If , then and
so is an upward-pointing V with its minimum at and equal endpoint values .
If , the zeros of are and
Thus its five vertices are
An interval map has a horseshoe when there are an open interval and two disjoint open intervals such that
A finite linear combination of independent Gaussian random variables is Gaussian, so
Since , the characteristic functions converge pointwise:
The Lévy continuity theorem yields convergence in distribution to
On the given common probability space, the same variance calculation actually proves convergence in as well.
For every finite Rademacher sum, independence and the vanishing of odd moments give
The same calculation applied to shows that is Cauchy in , because the tail of tends to zero. Its limit agrees almost surely with its limit , since both modes imply convergence in probability. Passing to the limit gives
and therefore
For , independence and give
Thus is a Cauchy sequence in the complete L2 space and converges in to some random variable . The Cauchy-Schwarz inequality gives on a probability space, so the convergence also holds in . Finally, convergence in implies convergence in probability, which implies convergence in distribution.
For the tori in part (c), the distance from the origin is as large as , so condition (1) fails. Their surface areas are
so condition (2) fails as well.
False with the printed in the paper. Let the even-indexed surfaces be one fixed unit sphere and the odd-indexed surfaces one fixed ring torus. Then
but infinitely many surfaces are tori. The two fixed surfaces lie in one ball and have uniformly bounded area. Their injectivity radii have a positive common lower bound, and compactness gives a common bound on , hence on every radial derivative . Thus this alternating sequence satisfies all four additional conditions as well.
The intended statement becomes true if is replaced by
Here is the proof. Put , so . Choose maximizing distance from the centre of the fixed containing ball. The supporting-sphere curvature bound gives
Write and in geodesic polar coordinates. Choose a fixed sufficiently small and set . Conditions (3) and (4) allow to be chosen so that and
The Jacobi equation , with and , and the Sturm comparison theorem then give on this ball for a constant independent of . Consequently
Since elsewhere and ,
for all sufficiently large . Gauss-Bonnet forces , and the classification theorem for surfaces makes each such a sphere.
The preceding estimate makes equicontinuous, and
makes it uniformly bounded. The Arzelà-Ascoli theorem therefore supplies a subsequence converging uniformly to a continuous function . On every mesh interval,
including an endpoint by using the adjacent interval. Consequently uniformly along the same subsequence.
All and lie in one compact ball. The restriction of the continuous vector field to that ball is uniformly continuous, so uniformly. Passing to the limit in the defining equation gives
The fundamental theorem of calculus now makes differentiable and yields . This proves the required special case of the Peano existence theorem; uniqueness need not hold because was assumed continuous but not locally Lipschitz continuous.

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!
We have two killer features:
  1. topics: topics group articles by different users with the same title, e.g. here is the topic for the "Fundamental Theorem of Calculus" ourbigbook.com/go/topic/fundamental-theorem-of-calculus
    Articles of different users are sorted by upvote within each article page. This feature is a bit like:
    • a Wikipedia where each user can have their own version of each article
    • 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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    This way you can be sure that even if OurBigBook.com were to go down one day (which we have no plans to do as it is quite cheap to host!), your content will still be perfectly readable as a static site.
    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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    Figure 6.
    Dynamic article tree with infinitely deep table of contents
    .
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