Loading [MathJax]/extensions/mml2jax.js
Skip to main content
Library homepage
 

Text Color

Text Size

 

Margin Size

 

Font Type

Enable Dyslexic Font
Physics LibreTexts

Search

  • Filter Results
  • Location
  • Classification
    • Article type
    • Author
    • Cover Page
    • License
    • Show TOC
    • Transcluded
    • OER program or Publisher
    • Student Analytics
    • Autonumber Section Headings
    • License Version
    • Print CSS
      • Screen CSS
      • PrintOptions
    • Include attachments
    Searching in
    About 3 results
    • https://phys.libretexts.org/Bookshelves/Thermodynamics_and_Statistical_Mechanics/Book%3A_Thermodynamics_and_Statistical_Mechanics_(Arovas)/06%3A_Classical_Interacting_Systems/6.04%3A_Liquid_State_Physics
      The virial expansion is typically applied to low-density systems. When the density is high, where a is a typical molecular or atomic length scale, the virial expansion is impractical. There are to m...The virial expansion is typically applied to low-density systems. When the density is high, where a is a typical molecular or atomic length scale, the virial expansion is impractical. There are to many terms to compute, and to make progress one must use sophisticated resummation techniques to investigate the high density regime. To elucidate the physics of liquids, it is useful to consider the properties of various correlation functions.
    • https://phys.libretexts.org/Bookshelves/Thermodynamics_and_Statistical_Mechanics/Essential_Graduate_Physics_-_Statistical_Mechanics_(Likharev)/05%3A_Fluctuations/5.08%3A_Back_to_the_correlation_function
      On the other hand, since the average \(\langle f(t)f(t +\tau )\rangle\) of a stationary process should not depend on \(t\), instead of \(W_m(0)\) we may take the stationary probability distribution \(...On the other hand, since the average \(\langle f(t)f(t +\tau )\rangle\) of a stationary process should not depend on \(t\), instead of \(W_m(0)\) we may take the stationary probability distribution \(W_m(\infty )\), independent of the initial conditions, which may be found as the same special solution, but at time \(\tau \rightarrow \infty \).
    • https://phys.libretexts.org/Bookshelves/Thermodynamics_and_Statistical_Mechanics/Essential_Graduate_Physics_-_Statistical_Mechanics_(Likharev)/05%3A_Fluctuations/5.04%3A_Fluctuations_as_functions_of_time
      \[\left\langle f_{\omega} f_{\omega^{\prime}}^{*}\right\rangle=\frac{1}{(2 \pi)^{2}} \int_{-\infty}^{+\infty} d t \int_{-\infty}^{+\infty} d \tau K_{f}(\tau) e^{i\left(\omega-\omega^{\prime}\right) t}...\[\left\langle f_{\omega} f_{\omega^{\prime}}^{*}\right\rangle=\frac{1}{(2 \pi)^{2}} \int_{-\infty}^{+\infty} d t \int_{-\infty}^{+\infty} d \tau K_{f}(\tau) e^{i\left(\omega-\omega^{\prime}\right) t} e^{i \omega^{\prime} \tau} \equiv \frac{1}{(2 \pi)^{2}} \int_{-\infty}^{+\infty} K_{f}(\tau) e^{i \omega^{\prime} \tau} d \tau \int_{-\infty}^{+\infty} e^{i\left(\omega-\omega^{\prime}\right) t} d t . \label{56}\]

    Support Center

    How can we help?