Abstract
Intermediate-mass black holes (IMBHs), with masses in the range ∼102–4 M⊙, would be unique sources of gravitational waves for LISA. Here we discuss their context as well as specific characteristics of IMBH–IMBH and IMBH–supermassive black hole mergers and how these would allow sensitive tests of the predictions of general relativity in strong gravity.
Full Text 
Sign-in/Register to access full text options
Sign-in/Register to access full text options 
Published version (
Free)
Free) 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a call
