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Periodic orbits are considered 'dense' if, for any point and any ε-neighborhood, there exists at least one periodic point within that neighborhood. Uniqueness of these periodic points is not required; multiple points can belong to the same orbit and still satisfy the density condition. Even if every neighborhood contains points from the same periodic orbit, the orbits are still deemed dense, as this condition is stronger than merely having a union of periodic orbits being dense. However, in the context of $\mathbb{R}^n$, a single periodic orbit cannot be dense, which differs in more general metric spaces. This discussion clarifies the nature of density in periodic orbits within dynamical systems.
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Loosely speaking, we say that periodic orbits are 'dense' if given any $\epsilon$-neighborhood, there exists at least one periodic point in that neighborhood for any $\epsilon > 0$.

Is there any requirement for these periodic points to be unique?

For example, what if every neighborhood contains a periodic point (that we know about) which is part of the same periodic orbit. Do we still say that orbits are dense? Or are they dense in a trivial sense.

Thanks!
 
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Joppy said:
Loosely speaking, we say that periodic orbits are 'dense' if given any $\epsilon$-neighborhood, there exists at least one periodic point in that neighborhood for any $\epsilon > 0$.
For concreteness, is your setting a discrete dynamical system represented by an iterated map $f$ on $\mathbb{R}^n$ or, more generally, on some complete metric space? It does not matter that much, though: For a flow, the ideas are similar.

Yes, periodic orbits of $f$ are dense if given any point $\mathbf{x} \in \mathbb{R}^n$ and any $\epsilon > 0$, there exists a periodic point $\mathbf{y} \in \mathbb{R}^n$ of $f$ (of course $\mathbf{y}$ lies on some periodic orbit) such that $\|\mathbf{x} - \mathbf{y}\| < \epsilon$. In other words, the set consisting of the union of all periodic orbits of $f$ is dense in $\mathbb{R}^n$ in the ordinary sense.

Joppy said:
Is there any requirement for these periodic points to be unique?
No, quite the opposite. Let $\mathbf{x}$ and $\epsilon > 0$ be given. Assume that $\mathbf{x}$ itself is not periodic. (This is always possible, unless the whole phase space consists of periodic points.) Suppose it happens that $\mathbf{y}$ is the unique periodic point in the $\epsilon$-ball centered at $\mathbf{x}$. Then the ball centered at $\mathbf{x}$ with radius $\frac{1}{2}\|\mathbf{x} - \mathbf{y}\| > 0$ does not contain any periodic points, which contradicts density.

Joppy said:
For example, what if every neighborhood contains a periodic point (that we know about) which is part of the same periodic orbit. Do we still say that orbits are dense? Or are they dense in a trivial sense.

Sure we still say that periodic orbits are dense. In fact, the property you mention now is stronger than what you mentioned at the beginning: Now, one periodic orbit has to do the job of being dense in the phase space, whereas before it was only required that all periodic orbits together form a dense union.

Addition: Note that for the case of $\mathbb{R}^n$, a single periodic orbit cannot be dense. (In the general metric case, it is different.)
 
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Thanks a lot for the informative response, and apologies for my late one!

Krylov said:
For concreteness, is your setting a discrete dynamical system represented by an iterated map $f$ on $\mathbb{R}^n$ or, more generally, on some complete metric space? It does not matter that much, though: For a flow, the ideas are similar.

Not quite $\mathbb{R}^n$, although I was assuming this in my question to make sure I see the other half of the story..

Krylov said:
No, quite the opposite. Let $\mathbf{x}$ and $\epsilon > 0$ be given. Assume that $\mathbf{x}$ itself is not periodic. (This is always possible, unless the whole phase space consists of periodic points.) Suppose it happens that $\mathbf{y}$ is the unique periodic point in the $\epsilon$-ball centered at $\mathbf{x}$. Then the ball centered at $\mathbf{x}$ with radius $\frac{1}{2}\|\mathbf{x} - \mathbf{y}\| > 0$ does not contain any periodic points, which contradicts density.

Sure we still say that periodic orbits are dense. In fact, the property you mention now is stronger than what you mentioned at the beginning: Now, one periodic orbit has to do the job of being dense in the phase space, whereas before it was only required that all periodic orbits together form a dense union.

Addition: Note that for the case of $\mathbb{R}^n$, a single periodic orbit cannot be dense. (In the general metric case, it is different.)

This makes sense! An easy to understand argument indeed. Thanks.
 
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