scholarly journals Merging stellar and intermediate-mass black holes in dense clusters: implications for LIGO, LISA, and the next generation of gravitational wave detectors

Author(s):  
M. Arca Sedda ◽  
P. Amaro-Seoane ◽  
X. Chen
2014 ◽  
Vol 89 (10) ◽  
Author(s):  
J. Aasi ◽  
B. P. Abbott ◽  
R. Abbott ◽  
T. Abbott ◽  
M. R. Abernathy ◽  
...  

2011 ◽  
Vol 20 (10) ◽  
pp. 2081-2086
Author(s):  
BALA R IYER

Over the last decade gravitational waveforms of binary black holes have been investigated using a variety of approaches like the Multipolar post-Minkowskian formalism, Numerical Relativity and the Effective-One-Body method. We review these complementary approaches and summarize the current status of these investigations of relevance to construct the best templates for the next generation Advanced gravitational wave detectors.


2008 ◽  
Vol 686 (2) ◽  
pp. 829-837 ◽  
Author(s):  
Kelly Holley‐Bockelmann ◽  
Kayhan Gültekin ◽  
Deirdre Shoemaker ◽  
Nicolas Yunes

2020 ◽  
Vol 897 (1) ◽  
pp. 46 ◽  
Author(s):  
Giacomo Fragione ◽  
Abraham Loeb ◽  
Kyle Kremer ◽  
Frederic A. Rasio

2021 ◽  
Vol 2021 (11) ◽  
pp. 039
Author(s):  
Valerio De Luca ◽  
Gabriele Franciolini ◽  
Paolo Pani ◽  
Antonio Riotto

Abstract The next generation of gravitational-wave experiments, such as Einstein Telescope, Cosmic Explorer and LISA, will test the primordial black hole scenario. We provide a forecast for the minimum testable value of the abundance of primordial black holes as a function of their masses for both the unclustered and clustered spatial distributions at formation. In particular, we show that these instruments may test abundances, relative to the dark matter, as low as 10-10.


2007 ◽  
Vol 3 (S246) ◽  
pp. 359-360
Author(s):  
B. Devecchi ◽  
M. Colpi ◽  
M. Mapelli ◽  
A. Possenti

AbstractGlobular clusters (GCs) are rich of millisecond pulsars (MSPs) and might also host single or binary intermediate–mass black holes (IMBHs). We simulate 3- and 4-body encounters in order to test the possibility that an IMBH captures a MSP. The newly formed system could be revealed from the timing signal of the MSP, providing an unambiguous measure of the BH mass. In current surveys, the number of expected [IMBH,MSP] binaries in the Milky Way is ~0.1. If next-generation radio telescopes (e.g. SKA) will detect ~10 times more MSPs in GCs, we expect to observe at least one [IMBH,MSP] binary.


2012 ◽  
Vol 425 (1) ◽  
pp. 460-469 ◽  
Author(s):  
B. McKernan ◽  
K. E. S. Ford ◽  
W. Lyra ◽  
H. B. Perets

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