![Universe | Free Full-Text | Jeans Instability of Dissipative Self-Gravitating Bose–Einstein Condensates with Repulsive or Attractive Self-Interaction: Application to Dark Matter | HTML Universe | Free Full-Text | Jeans Instability of Dissipative Self-Gravitating Bose–Einstein Condensates with Repulsive or Attractive Self-Interaction: Application to Dark Matter | HTML](https://www.mdpi.com/universe/universe-06-00226/article_deploy/html/images/universe-06-00226-g007.png)
Universe | Free Full-Text | Jeans Instability of Dissipative Self-Gravitating Bose–Einstein Condensates with Repulsive or Attractive Self-Interaction: Application to Dark Matter | HTML
![Universe | Free Full-Text | Jeans Instability of Dissipative Self-Gravitating Bose–Einstein Condensates with Repulsive or Attractive Self-Interaction: Application to Dark Matter | HTML Universe | Free Full-Text | Jeans Instability of Dissipative Self-Gravitating Bose–Einstein Condensates with Repulsive or Attractive Self-Interaction: Application to Dark Matter | HTML](https://www.mdpi.com/universe/universe-06-00226/article_deploy/html/images/universe-06-00226-g005.png)
Universe | Free Full-Text | Jeans Instability of Dissipative Self-Gravitating Bose–Einstein Condensates with Repulsive or Attractive Self-Interaction: Application to Dark Matter | HTML
![general relativity - Jeans Instability in an Expanding Universe, Understanding the perturbation - Physics Stack Exchange general relativity - Jeans Instability in an Expanding Universe, Understanding the perturbation - Physics Stack Exchange](https://i.stack.imgur.com/tNiOf.png)
general relativity - Jeans Instability in an Expanding Universe, Understanding the perturbation - Physics Stack Exchange
![Figure 6 | Effect of Radiative Heat-Loss Function and Finite Larmor Radius Corrections on Jeans Instability of Viscous Thermally Conducting Self-Gravitating Astrophysical Plasma Figure 6 | Effect of Radiative Heat-Loss Function and Finite Larmor Radius Corrections on Jeans Instability of Viscous Thermally Conducting Self-Gravitating Astrophysical Plasma](https://static-02.hindawi.com/articles/isrn/volume-2012/420938/figures/420938.fig.006.jpg)
Figure 6 | Effect of Radiative Heat-Loss Function and Finite Larmor Radius Corrections on Jeans Instability of Viscous Thermally Conducting Self-Gravitating Astrophysical Plasma
![Modified Jeans instability of magnetized viscous spin 1/2 quantum plasma with resistive effects and Hall current | SpringerLink Modified Jeans instability of magnetized viscous spin 1/2 quantum plasma with resistive effects and Hall current | SpringerLink](https://media.springernature.com/lw685/springer-static/image/art%3A10.1007%2Fs10509-014-1879-x/MediaObjects/10509_2014_1879_Fig1_HTML.gif)
Modified Jeans instability of magnetized viscous spin 1/2 quantum plasma with resistive effects and Hall current | SpringerLink
![The growth rate of the Jeans instability versus k/k J for different... | Download Scientific Diagram The growth rate of the Jeans instability versus k/k J for different... | Download Scientific Diagram](https://www.researchgate.net/publication/320371258/figure/fig2/AS:669286515372042@1536581748498/The-growth-rate-of-the-Jeans-instability-versus-k-k-J-for-different-values-of-the-EiBI.png)
The growth rate of the Jeans instability versus k/k J for different... | Download Scientific Diagram
![general relativity - Jeans Instability in an Expanding Universe, Understanding the perturbation - Physics Stack Exchange general relativity - Jeans Instability in an Expanding Universe, Understanding the perturbation - Physics Stack Exchange](https://i.stack.imgur.com/QHY4V.png)