Dynamical equations of a superfluid in curved space-time and Cattaneo's projection method

Details Dynamical equations of a superfluid in curved space-time and Cattaneo's projection method Dynamical equations of a superfluid in curved space-time and Cattaneo's projection method

Dec 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010ap.....53..554k&link_type=abstract

Astrophysics, Volume 53, Issue 4, pp.554-559

Astronomy and Astrophysics

Astrophysics

Superfluid, Dynamical Equations, General Relativity

Scientific paper

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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