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Simulations of black-hole binaries with unequal masses or non-precessing spins: accuracy, physical properties, and comparison with post-Newtonian results (2010)

First Author: Hannam M

Attributed to: Black-hole-binary simulations for gravitational-wave astronomy funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.1007.4789

Publication URI: https://arxiv.org/abs/1007.4789

Type: Other