Figure 20: The dominant quadrupolar component of the gravitational 
scalar for an equal-mass,
non-spinning NS binary with individual baryon masses of 
. The solid (black) curve refers
to GR, and the dashed (red) curve to a scalar-tensor theory with 
. Image
reproduced with permission from [73], copyright by APS.
scalar for an equal-mass,
non-spinning NS binary with individual baryon masses of . The solid (black) curve refers
to GR, and the dashed (red) curve to a scalar-tensor theory with . Image
reproduced with permission from [73], copyright by APS.Vitor Cardoso and Leonardo Gualtieri and Carlos Herdeiro and Ulrich Sperhake, "Exploring New Physics Frontiers Through Numerical
Relativity",
Living Rev. Relativity, 18 (2015), 1, doi:10.1007/lrr-2015-1, URL (accessed <date>): http://www.livingreviews.org/lrr-2015-1.![]()
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Living Rev. Relativity, 18 (2015), 1, doi:10.1007/lrr-2015-1, URL (accessed <date>): http://www.livingreviews.org/lrr-2015-1.