  Gravitational wave detection in space promises to open a new window in
astronomy to study the strong field dynamics of gravitational physics in
astrophysics and cosmology. The present article is an extract of a report on a
feasibility study of gravitational wave detection in space, commissioned by the
National Space Science Center, Chinese Academy of Sciences almost a decade ago.
The objective of the study was to explore various possible mission options to
detect gravitational waves in space alternative to that of the (e)LISA mission
concept and look into the requirements on the technological fronts. On the
basis of relative merits and balance between science and technological
feasibility, a set of representative mission options were studied and in the
end a mission design was recommended as the starting point for research and
development in the Chinese Academy of Sciences. The mission design was
eventually adopted by the current TAIJI mission as the baseline parameters for
the project. Subject to technological constraints, the baseline parameters of
the TAIJI mission were designed in such a way to optimise the capability of a
spaceborne gravitational wave detector to probe high redshift light seed,
intermediate mass black holes and thereby shed important light on the structure
formation in early Universe.
