Jmm. Senovilla et R. Vera, New family of inhomogeneous gamma-law cosmologies: Example of gravitational waves in a homogeneous p = rho/3 background - art. no. 084008, PHYS REV D, 6308(8), 2001, pp. 4008
We present an explicit three-parameter class of p = gamma rho (-1/3 less th
an or equal to gamma <1) cosmological models admitting a two-dimensional gr
oup G(2) of isometries acting on spacelike surfaces. The family is self-sim
ilar in the sense that it has a further homothetic vector held and it conta
ins subfamilies of both (previously unknown) tilted and nontilted Bianchi m
odels with that equation of state. This is the first algebraically general
class of solutions of this kind including dust inhomogeneous solutions. The
whole class presents a universal spacelike big-bang singularity in the fin
ite past. More interestingly, the case p = <rho>/3 constitutes a new two-pa
rameter inhomogeneous subfamily which can be viewed as a Bianchi type V bac
kground with a gravitational wave traveling orthogonally to the surfaces of
transitivity of the G(2) group. This wave generates the inhomogeneity of t
he spacetime and is related to the sound waves tilting the perfect fluid. I
t seems to be the first explicit exact trample of a gravitational wave trav
eling along a homogeneous background that has a realistic equation of state
p = rho /3.