Post-Newtonian Dynamics in Dense Star Clusters: Highly Eccentric, Highly Spinning, and Repeated Binary Black Hole Mergers.
Phys Rev Lett
; 120(15): 151101, 2018 Apr 13.
Article
in En
| MEDLINE
| ID: mdl-29756855
Full text:
1
Collection:
01-internacional
Database:
MEDLINE
Language:
En
Journal:
Phys Rev Lett
Year:
2018
Document type:
Article
Affiliation country:
United States
Country of publication:
United States