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gwpv v0.3.0
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Gallery¶

Here are a few images and movies produced with this software package, and their appearances in media and scientific journals.

Visualization of GW190412¶

Numerical simulation of two black holes that inspiral and merge, emitting gravitational waves. One black hole is 3.5x more massive than the other and spins, which makes the orbit precess. The simulated gravitational-wave signal is consistent with the observation made by the LIGO and Virgo gravitational-wave detectors on April 12th, 2019 (GW190412).

GW190412 PanoramaLargeScaleNoTail_frame.000023

GW190412 CloseupSlowdownWithSpins_frame.000003

GW190412 FaceOnMerger

  • More images and citation: DOI

  • Source: nilsvu/gw190412-movie

  • Video:

    GW190412 video

  • Selected media coverage:

    • https://www.nature.com/articles/d41586-020-01153-7

    • https://www.sciencenews.org/article/gravitational-waves-unevenly-sized-black-holes-ligo-virgo

    • https://www.aei.mpg.de/213678/a-signal-like-none-before

    • https://www.ligo.org/detections/GW190412

    • https://www.ligo.caltech.edu/news/ligo20200420

    • https://www.spektrum.de/news/neuartiges-gravitationswellensignal/1725506

  • Appearances in scientific publications:

    • A Horizon Study for Cosmic Explorer: Science, Observatories, and Community, arXiv:2109.09882

    • The Next Generation Global Gravitational Wave Observatory: The Science Book, arXiv:2111.06990

    • Lovelace, G. Computational challenges in numerical relativity in the gravitational-wave era, Nat Comput Sci 1, 450–452 (2021)

  • Magazines:

    • Sky & Telescope June 2022 (cover)

      _images/ST_cover_june2022.png
  • Prizes:

    • Figure 1a scientific art exhibition 2021

Visualization of GW190814¶

Visualisation of the coalescence of two black holes that inspiral and merge, emitting gravitational waves. One black hole is 9.2x more massive than the other and both objects are non-spinning. The high mass-ratio amplifies gravitational-wave overtones in the emitted signal. The gravitational-wave signal produced is consistent with the observation made by the LIGO and Virgo gravitational-wave detectors on August 14th, 2019 (GW190814).

GW190814 MergerFaceOnAllModes

GW190814 PanoramaModesCompositionFaceOn_frame.000003

GW190814 PanoramaAllModesFaceOn_frame.000006

  • More images and citation: DOI

  • Source: nilsvu/gw190814-movie

  • Video:

    GW190814 video

  • Selected media coverage:

    • https://www.aei.mpg.de/267070/a-black-hole-with-a-puzzling-companion

    • https://www.ligo.org/detections/GW190814

    • https://www.space.com/smallest-black-hole-biggest-neutron-stary-mystery-object.html

    • https://www.dailymail.co.uk/sciencetech/article-8451939/Mysterious-cosmic-object-lighter-black-hole-heavier-neutron-star-discovered.html

Visualization of GW190521¶

Numerical simulation of two black holes that inspiral and merge, emitting gravitational waves. The black holes have large and nearly equal masses, with one only 3% more massive than the other. The simulated gravitational wave signal is consistent with the observation made by the LIGO and Virgo gravitational wave detectors on May 21st, 2019 (GW190521).

GW190521 FaceOn.000003

GW190521 Serene

  • More images and citation: DOI

  • Source: nilsvu/gw190521-movie

  • Video:

    GW190521 video

  • Selected media coverage:

    • https://www.aei.mpg.de/296843/ligo-and-virgo-catch-their-biggest-fish-so-far

    • https://www.ligo.caltech.edu/news/ligo20200902

    • https://aasnova.org/2020/09/02/ligo-virgos-newest-merger

Visualization of a black hole scattering and capture orbit¶

Numerical simulation of two black holes that scatter and then merge, emitting gravitational waves. Simulation with the SpEC code and wave extraction with the SpECTRE code by Oliver Long.

bbh-capture

  • More images and citation: DOI

  • Source: nilsvu/bbh-capture-movie

  • Video:

    bbh-capture-video

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  • Gallery
    • Visualization of GW190412
    • Visualization of GW190814
    • Visualization of GW190521
    • Visualization of a black hole scattering and capture orbit