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--The Maintainers
_
producing NS-NS binaries with mass ratios different from one is a bit
problematic sometimes. There is this trick though that can help (if it was
not yet implemented in the current LORENE version):
In the file C++/Source/Binaire/binaire_orbite.C, there is a routine
fonc_binaire_axe on lines 799-854
Hi Jimmy
The lower mass that you are asking Lorene for is not realized for neutron stars
(lower mass limit >~1.0M_sun)
and would rather approach the mass for a brown dwarf. This lower mass and the
upper theoretical limit places an upper constraint
on the mass ratio to be around q~2. For initial