D E Vincent 1985 Class. Quantum Grav. 2 409 doi:10.1088/0264-9381/2/3/016
D E Vincent
Show affiliationsThe perfect-fluid energy-momentum tensor in the non-symmetric gravitation theory (NGT) is derived using a fluid variational technique. Two different approaches are used. The first involves conservation of rest mass as a fundamental fluid constraint in the total Lagrangian while the second involves the assumption of an equation of state P=P( rho 0). The relativistic fluid conservation equation and the Euler equation of motion for NGT are obtained using the derived fluid tensor.
04.40.Nr Einstein-Maxwell spacetimes, spacetimes with fluids, radiation or classical fields
83D05 Relativistic gravitational theories other than Einstein's, including asymmetric field theories
Issue 3 (May 1985)
D E Vincent 1985 Class. Quantum Grav. 2 409
J G Morley et al 1976 J. Phys. D: Appl. Phys. 9 1031
Annemie Bogaerts 1999 Plasma Sources Sci. Technol. 8 210
Allan Adams and Jarah Evslin JHEP02(2003)029
Masahito Hayashi 2007 New J. Phys. 9 284
Patrick J Windpassinger et al 2008 New J. Phys. 10 053032
Nathan Berkovits et al JHEP11(2004)038
Fabiola Gianotti 2007 New J. Phys. 9 332
S Odžak and D B Milošević 2009 J. Phys. B: At. Mol. Opt. Phys. 42 071001
J G Titus et al 2009 Environ. Res. Lett. 4 044008