Caption: A video of a computer simulation of a black hole binary undergoing a black hole merger and emitting gravitational waves. See also the Youtube version Warped Spacetime and Horizons of GW150914 | 1:13.
But show the classroom the GREATEST EVER black hole merger video (i.e., Gravitational waves: GW20150904: LIGO video 2016feb11 | 2:55), hereafter just referred to as the video.
The image-linked video is NOT as good (i.e., Video simulation of the changing gravitational field, and gravitational waves, during the final inspiral, merger and ringdown of GW150914 | 1:13). CLICK on the link just given or on the image and then click on the start button to play the linked video.
Features:
The emitted gravitational waves carry away kinetic energy of the orbital motion, and thus the orbital decay i.e., inspiral to merger.
Since curved 3-dimensional space is hard for humans to visualize, it is usually represented as curved 2-dimensional space which humans can visualize.
In the video, the gravitational field (representative curved 2-dimensional space) is shown below the visualized black hole binary.
LIGO is a major US project dedicated to the detection gravitational waves from astrophysical sources.
The likeliest source is the merger of compact remnants (excluding white dwarfs): i.e., black hole mergers, neutron star mergers, and black hole neutron star mergers.
Another source is the collapse of a nearby massive star core in a core-collapse supernova. How nearby? Probably only one in the Local Group???? or we would already have a detection of such an event???.
Only sources like these might produce gravitational waves strong enough to be detected with the current-state-of-the-art detectors.
According to the Λ-CDM model of cosmology, the luminosity distance is 1.4(6) Gly ≅ 0.440(170) Gpc and the lookback time 1.4(6) Gyr which corresponds to cosmic time 12.4(6) Gyr after the Big Bang (see Wikipedia: Age of the observable universe = 13.797(23) Gyr (Planck 2018)).
The analysis suggests that merging black hole binary pair had masses 35(4) M_☉ 30(4) M_☉. The merged black hole had mass 62(4) M_☉ (see Wikipedia: GW150914: Astrophysical origin).
These black holes are stellar-mass black holes since their masses are below the ∼ 100--10**6 M_☉ range of intermediate-mass black holes and the range ∼> 10**6 M_☉ for supermassive black holes.
The observation of gravitational waves is a major verification of GR to add to all the others.
There remain competitor theories to general relativity, but none are favored over GR and some may be strongly disfavored or even ruled out---maybe by the current known gravitational wave events.
However, since GR is NOT consistent quantum mechanics, almost everyone believes that there is quantum gravity theory whose macroscopic limit is GR (or a competitor). Thus, GR emerges from a lower-in-the-hierarchy emergent theory.
PSR B1913+16 loses gravitational potential energy and mechanical energy exactly as predicted by GR via gravitational waves within uncertainty.
This is because the gravitational wave signals from the observed black hole mergers are exactly as predicted by GR within uncertainty.
The predictions do have free parameters (e.g., the masses black hole axial angular momentum), but these are just due to the peculiarities of the black hole binary systems and NOT in GR itself.
Since the gravitational wave signals are strong evidence for black holes, they are strong evidence for event horizons.
After GW150914: the first observation of gravitational waves, there was only a little doubt of event horizons.
Then in 2019, the EHT image of the M87 supermassive black hole (M87*) showed just what was expected from computer simulations for a supermassive black hole (SMBH) surrounded by an accretion disk. (see M87 Supermassive Black Hole First Image).
After these pieces of evidence, the existence of event horizons is very certain.
There are other theories for the observations, but they seem very improbable. In fact, one seldom absolutely rules out low-probability theories. But if their probability gets too low, they become uninteresting for people to consider any further unless they get revived by some astonishing new data---which occasionally happens. Almost all scientific verifications of theories allow that low-probability theories are NOT absolutely ruled out and this often goes without saying so.
Until this paradox is resolved, there is a major uncertainty about the nature of event horizons.
EOF
php require("/home/jeffery/public_html/astro/black_hole/black_hole_keywords.html");?>