comoving rate density
(none)
Technical definition
a measure of the number of gamma-ray bursts (GRBs) per unit volume of the universe, calculated with respect to a hypothetical "comoving" observer moving with the expansion of the universe.
(none)
a measure of the number of gamma-ray bursts (GRBs) per unit volume of the universe, calculated with respect to a hypothetical "comoving" observer moving with the expansion of the universe.