<?xml version="1.0" encoding="UTF-8"?>
<article>
    <title>Predicted Dynamic and Structural Criterion of Evaluation of Gravitational Waves</title>
    <authors>
        <author>M. Zhussupov</author>
    </authors>
    <affiliations>
        <affiliation>Science, Noosphereorder Co., London, UK</affiliation>
    </affiliations>
    <emails>
        <email>mjalmata@mail.ru</email>
    </emails>
    <journal>
        <name>International Journal of Fundamental Physical Sciences (IJFPS)</name>
        <volume>7</volume>
        <issue>1</issue>
        <pages>1-4</pages>
        <date>March, 2017</date>
        <issn>2231-8186</issn>
        <doi>https://doi.org/10.14331/ijfps.2017.330100</doi>
    </journal>
    <abstract>The cosmic (physical) vacuum is modeled as a material medium forming dynamic structures in interaction with celestial bodies. These structures are proposed to have a wave nature, contributing to gravitational wave phenomena. A key result is the derivation of a background gravitational wave frequency (~0.06 Hz) based on the density of vacuum and gravitational constant. The paper models gravitational waves across the solar system, evaluating their role in planetary motion and proposing a framework for the detection of gravitational waves from exoplanetary systems using instruments like LISA. It is concluded that the vacuum plays a decisive role in the structure and dynamics of observed systems.</abstract>
    <keywords>Cosmic Vacuum, Gravitational Waves, Frequency, Density Of Physical Vacuum, Exoplanets</keywords>
    <license>https://creativecommons.org/licenses/by/4.0/</license>
</article>
