Abstract
The problem of gravitational instability of an infinite homogenous fluid has been considered in the presence of a non-vertical magnetic field. A non-linear relation between the magnetic field and the magnetic induction proposed by P.H. Roberts (1981) in the context of neutron stars has been used. The dispersion relations have been obtained. It has been found that Jeans's criterion for instability is unaffected by this non-linear relationship even if the effect due to rotation is considered in the presence of a non-vertical magnetic field.
Similar content being viewed by others
References
Bora, M. and K. Nayyar: 1991,Astrophys. Space. Sci. 179, 313–320.
Chandrasekhar, S. and E. Fermi: 1953,Astrophys. J. 118, 116–141.
Chandrasekhar, S.: 1954,Astrophys. J. 119, 7–9.
Chhajlani, R. and M. Vyas: 1988,Astrophys. Space. Sci. 145, 223–240.
Muzikar, P. and C.J. Peth: 1981,Phys. Rev. B 24, 2533–2539.
Roberts, P.: 1981,Q. J. Mech. Appl. Math. 34, 327–343.
Sharma, R. and T. Chand: 1991,Astrophys. Space Sci. 183, 215–224.
Sharma, R. and A. Rajput: 1992,Astrophys. Space. Sci., 105–111.
Sharma, R. and B. Singh: 1988,Astrophys. Space Sci. 143, 233–239.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Abdullah, A.A. Gravitational instability of a non-linear magnetic fluid. Astrophys Space Sci 204, 289–295 (1993). https://doi.org/10.1007/BF00658031
Received:
Issue Date:
DOI: https://doi.org/10.1007/BF00658031