Binary black holes

Binary black holes

These images are the result of the numerical simulation of two inspiralling black holes that merge to form a new black hole. They show the apparent horizons and the gravitational waves produced. Shown is the real part of the curvature scalar Psi4.

Credits

© C. Reisswig (Max Planck Institute for Gravitational Physics), L. Rezzolla (Max Planck Institute for Gravitational Physics & Institute for Theoretical Physics, Frankfurt), M. Koppitz (Max Planck Institute for Gravitational Physics & Zuse Institute Berlin)

Note: Publication of these images requires proper credits and written permission. Please contact aei_zib_images@aei.mpg.de in advance of publication.

Fig. 1
Fig. 2
Fig. 3
Fig. 4
Fig. 5
Fig. 6
Fig. 7
Fig. 8
Fig. 9
Fig. 10
Fig. 11
Fig. 12

These images are the result of the numerical simulation of two inspiralling black holes that merge to form a new black hole. They show the apparent horizons and the gravitational waves produced. Shown are the real and imaginary parts of the curvature scalar Psi4.

Credits

© C. Reisswig (Max Planck Institute for Gravitational Physics), L. Rezzolla (Max Planck Institute for Gravitational Physics & Institute for Theoretical Physics, Frankfurt), M. Koppitz (Max Planck Institute for Gravitational Physics & Zuse Institute Berlin)

Note: Publication of these images requires proper credits and written permission. Please contact aei_zib_images@aei.mpg.de in advance of publication.

Fig. 1
Fig. 2
Fig. 3
Fig. 4
Fig. 5
Fig. 6
Fig. 7
Fig. 8
Fig. 9
Fig. 10
Fig. 11
Fig. 12

These images are the result of the numerical simulation of two inspiralling black holes that merge to form a new black hole. They show the apparent horizons and the gravitational waves produced. Shown are the real and imaginary part of the curvature scalar Psi4 (showing two polarizations side by side).

Credits

© C. Reisswig (Max Planck Institute for Gravitational Physics), L. Rezzolla (Max Planck Institute for Gravitational Physics & Institute for Theoretical Physics, Frankfurt), M. Koppitz (Max Planck Institute for Gravitational Physics & Zuse Institute Berlin)

Note: Publication of these images requires proper credits and written permission. Please contact aei_zib_images@aei.mpg.de in advance of publication.

Fig. 2
Fig. 3
Fig. 4
Fig. 5
Fig. 6
Fig. 7
Fig. 8
Fig. 9
Fig. 10
Fig. 11
Fig. 12

Numerical simulation of two inspiralling black holes that merge to form a new black hole

The images show the apparent horizons and the gravitational waves that are produced.

Credits

© C. Reisswig (Max Planck Institute for Gravitational Physics), L. Rezzolla (Max Planck Institute for Gravitational Physics & Institute for Theoretical Physics, Frankfurt), R. Kähler (Max Planck Institute for Gravitational Physics & Zuse Institute Berlin)

Note: Publication of these images requires proper credits and written permission. Please contact aei_zib_images@aei.mpg.de in advance of publication.

Fig. 2
Fig. 3
Fig. 4
Fig. 5
Fig. 6
Fig. 7
Fig. 8
Fig. 9
Fig. 10
Fig. 11
Fig. 12
Web-View
Print Page
Open in new window
Estimated DIN-A4 page-width
Go to Editor View