Jimmie Adriazola
    • Create new note
    • Create a note from template
      • Sharing URL Link copied
      • /edit
      • View mode
        • Edit mode
        • View mode
        • Book mode
        • Slide mode
        Edit mode View mode Book mode Slide mode
      • Customize slides
      • Note Permission
      • Read
        • Only me
        • Signed-in users
        • Everyone
        Only me Signed-in users Everyone
      • Write
        • Only me
        • Signed-in users
        • Everyone
        Only me Signed-in users Everyone
      • Engagement control Commenting, Suggest edit, Emoji Reply
    • Invite by email
      Invitee

      This note has no invitees

    • Publish Note

      Share your work with the world Congratulations! 🎉 Your note is out in the world Publish Note

      Your note will be visible on your profile and discoverable by anyone.
      Your note is now live.
      This note is visible on your profile and discoverable online.
      Everyone on the web can find and read all notes of this public team.
      See published notes
      Unpublish note
      Please check the box to agree to the Community Guidelines.
      View profile
    • Commenting
      Permission
      Disabled Forbidden Owners Signed-in users Everyone
    • Enable
    • Permission
      • Forbidden
      • Owners
      • Signed-in users
      • Everyone
    • Suggest edit
      Permission
      Disabled Forbidden Owners Signed-in users Everyone
    • Enable
    • Permission
      • Forbidden
      • Owners
      • Signed-in users
    • Emoji Reply
    • Enable
    • Versions and GitHub Sync
    • Note settings
    • Note Insights
    • Engagement control
    • Transfer ownership
    • Delete this note
    • Save as template
    • Insert from template
    • Import from
      • Dropbox
      • Google Drive
      • Gist
      • Clipboard
    • Export to
      • Dropbox
      • Google Drive
      • Gist
    • Download
      • Markdown
      • HTML
      • Raw HTML
Menu Note settings Versions and GitHub Sync Note Insights Sharing URL Create Help
Create Create new note Create a note from template
Menu
Options
Engagement control Transfer ownership Delete this note
Import from
Dropbox Google Drive Gist Clipboard
Export to
Dropbox Google Drive Gist
Download
Markdown HTML Raw HTML
Back
Sharing URL Link copied
/edit
View mode
  • Edit mode
  • View mode
  • Book mode
  • Slide mode
Edit mode View mode Book mode Slide mode
Customize slides
Note Permission
Read
Only me
  • Only me
  • Signed-in users
  • Everyone
Only me Signed-in users Everyone
Write
Only me
  • Only me
  • Signed-in users
  • Everyone
Only me Signed-in users Everyone
Engagement control Commenting, Suggest edit, Emoji Reply
  • Invite by email
    Invitee

    This note has no invitees

  • Publish Note

    Share your work with the world Congratulations! 🎉 Your note is out in the world Publish Note

    Your note will be visible on your profile and discoverable by anyone.
    Your note is now live.
    This note is visible on your profile and discoverable online.
    Everyone on the web can find and read all notes of this public team.
    See published notes
    Unpublish note
    Please check the box to agree to the Community Guidelines.
    View profile
    Engagement control
    Commenting
    Permission
    Disabled Forbidden Owners Signed-in users Everyone
    Enable
    Permission
    • Forbidden
    • Owners
    • Signed-in users
    • Everyone
    Suggest edit
    Permission
    Disabled Forbidden Owners Signed-in users Everyone
    Enable
    Permission
    • Forbidden
    • Owners
    • Signed-in users
    Emoji Reply
    Enable
    Import from Dropbox Google Drive Gist Clipboard
       owned this note    owned this note      
    Published Linked with GitHub
    Subscribed
    • Any changes
      Be notified of any changes
    • Mention me
      Be notified of mention me
    • Unsubscribe
    Subscribe
    # A Curious NLS Simulation Consider the following NLS equation with gain $$i\partial_t\psi=-\frac{1}{2}\partial_x^2\psi-|\psi|^2\psi-iV(t)\psi $$ where $x\in\mathbb{R},\ t\in[0,T],$ with a 4 parameter family of NLS soliton initial conditions given by $$ \psi(x,0)=2\lambda{\rm sech}\left(2\lambda(x-\xi)\right)e^{i(cx+\theta)}. $$ The time-dependent potential is a negative semi-definite bump in time, for example, like the one in the following figure: ![](https://i.imgur.com/jxvYMi0.png) For reasons that will become apparent later on in this note, the way I am building $V(t)$ is through a four parameter family of sigmoids $$ D(t)=A\mathrm{tanh}(w(t-\tau))+D_0 $$ so that $$ V(t)=\frac{\mathrm{d}}{\mathrm{d}t}\mathrm{ln}\left(D(t)\right) $$ The above $V(t)$ corresponds to $A=-60,\ w=1/32,\ \tau=80$ and $D_0=-75.$ Choosing soliton parameters $\theta=\frac{\pi}{4}, \ c=.01,$ and $\xi=0,$ we observe the following from a numerical simulation: ![](https://i.imgur.com/WIf4LQl.png) This picture is reminiscent of pictures one would see when performing a semi-classical study of a Schrodinger Equation. For example, this picture is taken from page 180 of P.D. Miller's asymptotic analysis book where he analyzes the dynamics of a free particle Schrodinger wave function via the method of stationary phase. ![](https://i.imgur.com/pOqsD1S.png) However, nonlinear interactions seem to complicate the dynamics. Indeed, a similar problem was studied by Biondini and Oregero two years ago. In their problem, discussed here https://arxiv.org/abs/2005.12708, there is no time-dependent scattering, but instead, periodic solutions are evolved according to an NLS, with Planck's constant $\hbar$ reinstated. That is, using scalings consistent with their work, they solve $$ i\varepsilon\partial_t\psi=-\varepsilon^2\partial_x^2\psi-2|\psi|^2\psi $$ Using the initial condition $$ \psi(x,0)=e^{-\sin^2(x)}. $$ and setting $\varepsilon=0.026,$ B. and O. observe the following: ![](https://i.imgur.com/eIRYQOY.png) A potential project is to study the scattering problem shown above first, via a combination of detailed numerical simulations and a WKB-type analysis or one facilitated by an inverse scattering formalism, in order to understand what connection this has with the work of B. and O. as well as how it connects to other work done on semi-classical limits of Schrodinger equations. ## Better Literature Review After a brief discussion with P. Kevrekidis, I now understand that these types of dynamics are well-understood from work due to Tovbis and Bertola, here: https://arxiv.org/abs/1004.1828. The interaction of the soliton with the time-dependent potential causes a gradient catastrophe. ![](https://i.imgur.com/dDwFhKb.png) A little more digging on my end, and I found one of the earliest papers on the topic due to P.D. Miller and S. Kamvissis http://www.math.lsa.umich.edu/~millerpd/docs/J18.pdf![](https://i.imgur.com/dSvDOeD.png) These earlier works differ from the more recent work of Biondini and Oregero in their assumptions on initial conditions, namely that B. and O. initial conditions are not localized in space. The situation at the top remains different still. It may be interesting to understand, and place into context, why the gradient catastrophe in the soliton scattering problem manifests a spatio-temporal pattern resembling that which referenced from papers on semi-classical NLS dynamics. ## Some Numerical Experiments I realized the parameters $c$ and $\theta$ don't really matter at all. Setting $c$ just transports the whole situation along some characteristic direction in space-time (please ignore incorrect labeling). ![](https://i.imgur.com/w5rJtgr.png) So with $c=\theta=\xi=0,$ and for a fixed potential, we can vary $\lambda.$ Setting $\lambda=1/130$ we see similar dynamics just on a slower time-scale. ![](https://i.imgur.com/YvN4EqA.png) Setting $\lambda=1/70,$ things start to look different: ![](https://i.imgur.com/UpJfF9O.png) Setting $\lambda=1/50,$ we see some kind of periodic envelope emerge, ![](https://i.imgur.com/yKO5F22.png) And at $\lambda=1/40,$ I see this: ![](https://i.imgur.com/uXTVjmx.png) I'm very unsure of what "this" is. Perhaps this is a trivial rescaling of the dynamics and this is slightly obfuscated by the way I am plotting things. Here's more one more picture about the nearly-periodic behavior of the dynamics, but when $\lambda=1/90$ and on a longer time-scale: ![](https://i.imgur.com/vcnxZ8v.png) ## Where to go next? From a brief discussion, P. Miller brings up a good point: "...if you don't have V(t), but still take the sech initial condition, as you mentioned you can assume that c=0 without loss of generality in this case, in which case the square modulus of the solution is exactly periodic in time, with a period that is increasing in the limit $\varepsilon\to$ 0. So I think that might explain the recurrence you see in your simulations. " An analytical result we would like to see is that for a given initial soliton condition, the *shape* of $D(t)$ doesn’t affect microstructure, that is, the oscillations in the support of the solution. Here are two supporting numerical examples: This ![](https://i.imgur.com/f2RcyUs.png) gives rise to ![](https://i.imgur.com/CTCH664.png) while this ![](https://i.imgur.com/tgeqp8G.png) does almost exactly the same thing ![](https://i.imgur.com/3Nlremf.png) There is a similar result for the KdV equation, due to Tappert and Zabusky: https://journals.aps.org/prl/abstract/10.1103/PhysRevLett.27.1774 that confirms the experimental results of Madsen and Mei: https://www.cambridge.org/core/journals/journal-of-fluid-mechanics/article/transformation-of-a-solitary-wave-over-an-uneven-bottom/4D5A97D39CA331D3BFBEBC22AF885807 The idea there is that given only a KdV soliton initial condition and the depth of potential appearing in that context, one can predict the number of solitons that will fission off of the initial condition. That is, the shape of the potential matters very little. Roy Goodman and I confirmed this numerically some years ago. There is also something similar due to W. Choi for the Benjamin-Ono equation: https://royalsocietypublishing.org/doi/10.1098/rspa.1997.0094 Somehow, the analogous situation for the NLS is much more complex than KdV or Benjamin-Ono. (Pun not intended) ## Toward Understanding the Dynamics ### Removing the Gain Panos K., Alex T., and I met mid-October to try to understand more about the simulations above. The first observation made is that the gain term essentially "kicks" the soliton initial condition into something we are calling a non-equilibrium state. It seems reasonable to attempt to fit a hyperbolic secant to the profile. One question is: when? With all scalings the same as above and with $\lambda=1/90$, I chose $T=110$ time units by examining the imaginary part of $\psi(x,T).$ I'm sure there are other ways to have decided which $T$ to use, but this is what I did. Observe the following picture: ![](https://i.imgur.com/DERyt7j.png) Notice that $T=105$ is a bit early, and at $T=115,$ the top looks a little flat. By $T=120,$ the wavefunction now has three critical points. I insist that if you look at the real part or absolute value of $\psi,$ you wouldn't be able to detect such a hint as to when to perform the fit as easily. So the least-squares fit of the intensity profile, $|\psi|^2$, at $T=110$ with $$\psi_{\rm fit}=C_1\mathrm{sech}(C_2x) $$ looks like this ![](https://i.imgur.com/INKzZZY.png) where $(C_1,C_2)$ is found to be $(0.2305,.0226).$ Hey, not bad. The next question is, what do the dynamics look like? Here is what a soliton kicked by the gain looks like: ![](https://i.imgur.com/kKh1Sgc.png) and here is the above fitted state with no gain ![](https://i.imgur.com/mVlRmkW.png) It's absolutely clear now that we can remove the gain from the problem and investigate this problem with hyperbolic secant initial conditions of the above form evolving according to the usual NLS equation. However, it seems like we are a bit "far" from a soliton to do anything pertrubatively since the fited wavefunction looks something like $\psi=2\lambda\mathrm{sech}(2\lambda(1-\varepsilon)x),$ where $\varepsilon\approx 0.9$. Something we can consider small with regards to the setup is nowhere to be found. This might be a point of discussion for us. # Investigating the Spectrum Sorry for the confusing notation, but let's use $\lambda$ to denote an eigenvalue of the Zakharov-Shabat system Recall, the inverse scattering formalism associates a linear eigenvalue problem, called the Zakharov-Shabat system, with a potential given by an integrable nonlinear wave equation. For the homogeneous NLS, the Zakharov-Shabat eigenvalue problem is given by $$ \partial_{\xi}\varphi=-i\lambda\varphi +\psi(\xi,\zeta)\phi,\\ $$ $$ \partial_{\xi}\phi=i\lambda \phi-\psi^{*}(\xi,\zeta)\varphi. $$ To find $\lambda$, I used a spectral collocation method I found in Jianke Yang's book on nonlinear waves. Here are synchronized movies of the wavefunction's intensity and the spectrum of the ZS system below it (slightly out of sync). ![](https://i.imgur.com/1gIgElG.gif) ![](https://i.imgur.com/5MaSUnJ.gif) What we see is that, when the soliton interacts with the gain, we go from one pair of imaginary eigenvalues to 11.

    Import from clipboard

    Paste your markdown or webpage here...

    Advanced permission required

    Your current role can only read. Ask the system administrator to acquire write and comment permission.

    This team is disabled

    Sorry, this team is disabled. You can't edit this note.

    This note is locked

    Sorry, only owner can edit this note.

    Reach the limit

    Sorry, you've reached the max length this note can be.
    Please reduce the content or divide it to more notes, thank you!

    Import from Gist

    Import from Snippet

    or

    Export to Snippet

    Are you sure?

    Do you really want to delete this note?
    All users will lose their connection.

    Create a note from template

    Create a note from template

    Oops...
    This template has been removed or transferred.
    Upgrade
    All
    • All
    • Team
    No template.

    Create a template

    Upgrade

    Delete template

    Do you really want to delete this template?
    Turn this template into a regular note and keep its content, versions, and comments.

    This page need refresh

    You have an incompatible client version.
    Refresh to update.
    New version available!
    See releases notes here
    Refresh to enjoy new features.
    Your user state has changed.
    Refresh to load new user state.

    Sign in

    Forgot password

    or

    By clicking below, you agree to our terms of service.

    Sign in via Facebook Sign in via Twitter Sign in via GitHub Sign in via Dropbox Sign in with Wallet
    Wallet ( )
    Connect another wallet

    New to HackMD? Sign up

    Help

    • English
    • 中文
    • Français
    • Deutsch
    • 日本語
    • Español
    • Català
    • Ελληνικά
    • Português
    • italiano
    • Türkçe
    • Русский
    • Nederlands
    • hrvatski jezik
    • język polski
    • Українська
    • हिन्दी
    • svenska
    • Esperanto
    • dansk

    Documents

    Help & Tutorial

    How to use Book mode

    Slide Example

    API Docs

    Edit in VSCode

    Install browser extension

    Contacts

    Feedback

    Discord

    Send us email

    Resources

    Releases

    Pricing

    Blog

    Policy

    Terms

    Privacy

    Cheatsheet

    Syntax Example Reference
    # Header Header 基本排版
    - Unordered List
    • Unordered List
    1. Ordered List
    1. Ordered List
    - [ ] Todo List
    • Todo List
    > Blockquote
    Blockquote
    **Bold font** Bold font
    *Italics font* Italics font
    ~~Strikethrough~~ Strikethrough
    19^th^ 19th
    H~2~O H2O
    ++Inserted text++ Inserted text
    ==Marked text== Marked text
    [link text](https:// "title") Link
    ![image alt](https:// "title") Image
    `Code` Code 在筆記中貼入程式碼
    ```javascript
    var i = 0;
    ```
    var i = 0;
    :smile: :smile: Emoji list
    {%youtube youtube_id %} Externals
    $L^aT_eX$ LaTeX
    :::info
    This is a alert area.
    :::

    This is a alert area.

    Versions and GitHub Sync
    Get Full History Access

    • Edit version name
    • Delete

    revision author avatar     named on  

    More Less

    Note content is identical to the latest version.
    Compare
      Choose a version
      No search result
      Version not found
    Sign in to link this note to GitHub
    Learn more
    This note is not linked with GitHub
     

    Feedback

    Submission failed, please try again

    Thanks for your support.

    On a scale of 0-10, how likely is it that you would recommend HackMD to your friends, family or business associates?

    Please give us some advice and help us improve HackMD.

     

    Thanks for your feedback

    Remove version name

    Do you want to remove this version name and description?

    Transfer ownership

    Transfer to
      Warning: is a public team. If you transfer note to this team, everyone on the web can find and read this note.

        Link with GitHub

        Please authorize HackMD on GitHub
        • Please sign in to GitHub and install the HackMD app on your GitHub repo.
        • HackMD links with GitHub through a GitHub App. You can choose which repo to install our App.
        Learn more  Sign in to GitHub

        Push the note to GitHub Push to GitHub Pull a file from GitHub

          Authorize again
         

        Choose which file to push to

        Select repo
        Refresh Authorize more repos
        Select branch
        Select file
        Select branch
        Choose version(s) to push
        • Save a new version and push
        • Choose from existing versions
        Include title and tags
        Available push count

        Pull from GitHub

         
        File from GitHub
        File from HackMD

        GitHub Link Settings

        File linked

        Linked by
        File path
        Last synced branch
        Available push count

        Danger Zone

        Unlink
        You will no longer receive notification when GitHub file changes after unlink.

        Syncing

        Push failed

        Push successfully