Ivor Robinson 1997 Class. Quantum Grav. 14 A331 doi:10.1088/0264-9381/14/1A/025
Ivor Robinson
Show affiliationsA completely symmetrical form of the Bel - Robinson (BR) tensor is shown to give rise, in n-dimensional Lorentzian space, to a gravitational density. For n = 4, a physical identification is proposed.
Issue 1A (January 1997)
Ivor Robinson 1997 Class. Quantum Grav. 14 A331
M M El-Zaidia et al 1981 J. Phys. D: Appl. Phys. 14 2275
T Vestad et al 2004 J. Micromech. Microeng. 14 1503
M Hewitson et al 2005 Class. Quantum Grav. 22 4253
J J Luci et al 2007 Phys. Med. Biol. 52 N241
V I Donin et al 2003 J. Phys. D: Appl. Phys. 36 2366
I A Ivanov and A S Kheifets 2005 J. Phys. B: At. Mol. Opt. Phys. 38 2245
Martin Lepage et al 2007 Phys. Med. Biol. 52 N249
Jun Cui et al. 2005 ApJ 633 649
Franz Wegner 2006 J. Phys. A: Math. Gen. 39 8221