Abstract
The well known Jeans instability is studied for a viscoelastic gravitational fluid using generalized hydrodynamic equations of motions. It is found that the threshold for the onset of instability appears at higher wavelengths in a viscoelastic medium. Elastic effects playing a role similar to thermal pressure are found to lower the growth rate of the gravitational instability. Such features may manifest themselves in matter constituting dense astrophysical objects. © 2011 American Institute of Physics.
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CITATION STYLE
Janaki, M. S., Chakrabarti, N., & Banerjee, D. (2011). Jeans instability in a viscoelastic fluid. Physics of Plasmas, 18(1). https://doi.org/10.1063/1.3526685
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