surrkick

Black-hole kicks from numerical-relativity surrogate models

Binary black holes radiate linear momentum in gravitational waves as they merge. Recoils imparted to the black-hole remnant can reach thousands of km/s, thus ejecting black holes from their host galaxies. We exploit recent advances in gravitational waveform modeling to quickly and reliably extract recoils imparted to generic, precessing, black hole binaries. Our procedure uses a numerical-relativity surrogate model to obtain the gravitational waveform given a set of binary parameters, then from this waveform we directly integrate the gravitational-wave linear momentum flux. This entirely bypasses the need of fitting formulae which are typically used to model black-hole recoils in astrophysical contexts. We provide a thorough exploration of the black-hole kick phenomenology in the parameter space, summarizing and extending previous numerical results on the topic. Our extraction procedure is made publicly available as a module for the Python programming language named surrkick. Kick evaluations take 0.1s on a standard off-the-shelf machine, thus making our code ideal to be ported to large-scale astrophysical studies.

Credits

When using surrkick in any published work, please cite the paper describing its implementation:

The code is developed and maintained by Davide Gerosa, Francois Hebert and Leo Stein. We thank Jonathan Blackman, Chad Galley, Mark Scheel, Ulrich Sperhake, Saul Teukolsky and Vijay Varma for various discussions and technical help.

Releases

DOI Stable version released together with the first arxiv submission of arXiv:1802.04276.

Installation

surrkick is a python module, uploaded to the Python Package index. Installation is as easy as

pip install surrkick

The SXS surrogate model NRSur7dq2 and a few other dependencies will be installed together with surrkick. If you don’t have it already, you might need to manually install numpy beforehand (that’s pip install numpy). You can try some functionalities with

import surrkick
surrkick.plots.minimal()

Main functions

The core of the code consists of a single class, surrkick, whose methods allow to extract radiated energy, linear momentum (kicks) and angular momentum from the underlying waveform approximant. The main methods are:

The class plots contains script to reproduce all figures and results in arXiv:1802.04276. You can explore its methods with, e.g. help(surrkick.plots).

Test

The source code for the surrkick.plots.minimal() method mentioned above is

import surrkick
import matplotlib.pyplot as plt
sk=surrkick.surrkick(q=0.5,chi1=[0.8,0,0],
    chi2=[-0.8,0,0])
print 'vk/c=', sk.kick
plt.plot(sk.times,sk.voft[:,0],label='x')
plt.plot(sk.times,sk.voft[:,1],label='y')
plt.plot(sk.times,sk.voft[:,2],label='z')
plt.plot(sk.times,surrkick.project(sk.voft,
    sk.kickdir),label='vk')
plt.xlim(-100,100)
plt.legend()
plt.show()

If you try it, you should get a printout that reads vk/c= 0.00384... and this plot: minimal

Results

Here are some animations produced with surrkick.