  If multiple thermal weakly interacting massive particle (WIMP) dark matter
candidates exist, then their capture and annihilation dynamics inside a massive
stars such as Sun could change from conventional method of study. With a simple
correction to time evolution of dark matter (DM) number abundance inside the
Sun for multiple dark matter candidates, significant changes in DM annihilation
flux depending on annihilation, direct detection cross-section, internal
conversion and their contribution to relic abundance are reported in present
work.
