You're welcome, happy to help!

In summary, periodic orbits are considered 'dense' if given any $\epsilon$-neighborhood, there exists at least one periodic point in that neighborhood for any $\epsilon > 0$. There is no requirement for these periodic points to be unique. In fact, it is stronger to have one periodic orbit that is dense in the phase space rather than all periodic orbits together forming a dense union. However, for the case of $\mathbb{R}^n$, a single periodic orbit cannot be dense, but this may be possible in a general metric space.
  • #1
Joppy
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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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  • #2
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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  • #3
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.
 

FAQ: You're welcome, happy to help!

What are dense periodic orbits?

Dense periodic orbits refer to a type of orbit in a dynamical system that passes through a given point in space infinitely many times in a finite period of time. This means that the orbit is densely packed around the point, with no gaps or breaks.

What is the significance of dense periodic orbits?

Dense periodic orbits play a crucial role in chaotic systems, as they can act as attractors and help to determine the behavior of nearby trajectories. They also provide insights into the overall structure and dynamics of the system.

How do dense periodic orbits differ from regular periodic orbits?

Regular periodic orbits are closed and repeat the same path over and over again, while dense periodic orbits do not have a fixed path and can pass through any point infinitely many times. Additionally, regular periodic orbits occur in a finite number, while dense periodic orbits are infinite in number.

Can dense periodic orbits exist in all types of dynamical systems?

Yes, dense periodic orbits can exist in a wide range of dynamical systems, including discrete and continuous systems, as well as chaotic and non-chaotic systems. They can also be found in both two-dimensional and higher-dimensional systems.

How are dense periodic orbits studied and analyzed?

Dense periodic orbits can be identified and analyzed using various techniques, such as Poincaré sections, Lyapunov exponents, and bifurcation diagrams. These techniques help to visualize and understand the complex behavior of the orbits and their role in the overall dynamics of the system.

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