The absolute tensorial equations describing the dynamics of a superfluid in general relativity have been brought into the same form as the corresponding classical equations written in 3-vector forms. The expressions of the various forces acting on an element of a superfluid are explicitly displayed. In the Newtonian limit, these equations give the classical equations of motion of a superfluid in Galilean spacetime.
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Published in Astrofizika, Vol. 53, No. 4, pp. 623–628 (November 2010).
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Krikorian, R., Sedrakian, D.M. Dynamical equations of a superfluid in curved space-time and Cattaneo’s projection method. Astrophysics 53, 554–559 (2010). https://doi.org/10.1007/s10511-010-9147-4
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DOI: https://doi.org/10.1007/s10511-010-9147-4