No posts with label One wonders what a model with a single massive tensor dark matter particle with continuous range of masses from about 10^-26 eV to 10^-10 eV with masses distributed in a power law fitted to the distribution of gravitational wave strengths observed by gravitational wave detectors would look like. A galaxy length wave-length would be something on the order of 10^-24 Hertz, while some rare phenomena could generate gravitational waves with much shorter wave lengths as indicated in the chart shown below from Wikipedia:. Show all posts
No posts with label One wonders what a model with a single massive tensor dark matter particle with continuous range of masses from about 10^-26 eV to 10^-10 eV with masses distributed in a power law fitted to the distribution of gravitational wave strengths observed by gravitational wave detectors would look like. A galaxy length wave-length would be something on the order of 10^-24 Hertz, while some rare phenomena could generate gravitational waves with much shorter wave lengths as indicated in the chart shown below from Wikipedia:. Show all posts
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