What Happens in Black Holes: The Edge of All We Know?
The complete story of Black Holes: The Edge of All We Know, from the first scene to the last, in 479 words (about 2 minutes). Spoilers throughout.
Spoilers ahead
At the Large Millimeter Telescope (LMT) on Sierra Negra, Mexico, scientists working on the Event Horizon Telescope (EHT) discuss how to troubleshoot problems to prepare for the next day’s observation. They are working to take the first image of a black hole and have decided to focus their lenses at two: Sagittarius A*, the supermassive black hole in the center of the Milky Way galaxy, and the M87*, the Messier 87 galaxy’s supermassive black hole. These observations are a tedious process because many observatories all around the globe have to observe simultaneously and may face setbacks, such as weather problems. After five full days of recording, collecting a total of 1.5 petabytes of data per day, the EHT teams are done with all of their observations of Sagittarius A*.
After collecting the data, the EHT team must analyze it. To avoid problems of bias, the analysis team has been split into four groups, each of whom cannot see what the other groups are working on. Analysts, including computer scientist and engineer Katie Bouman, work on imaging algorithms to combine the data from the different telescopes into one cohesive image. After some time, each member of each team generates their own images and they compare and analyze their pictures to refine and combine their ideas into a single image while still keeping everything secret from the other teams. After each team has created their own image, they meet at a workshop to compare their four images, using an algorithm to determine the images’ similarity. Finally, on April 10, 2019, the EHT collaboration reveals the first image of a black hole to the whole world.
Meanwhile, Andrew Strominger, Malcolm Perry, and Sasha Haco discuss Hawking radiation and the black hole information paradox. They have been working with Stephen Hawking on a potential solution to the paradox. Strominger, Perry, and Haco go to a house to meet with Hawking and discuss their potential solution: Specific diffeomorphisms create additional degrees of freedom on the black hole’s horizon, which they term soft hair. They are trying to see if the soft hair’s charge will be enough to contain all the entropy of a black hole as predicted by Bekenstein and Hawking. Despite the difficulty of solving the paradox, they are optimistic about their chances. Unfortunately, while they are still working on the problem, Hawking dies. Despite this setback, they still manage to make progress by using computers and new approaches to refine the equation they are using to calculate the total information storage of the soft hair. Finally, they finish solving their equation and publish their paper, determining that soft hair can indeed store all of the information inside a black hole.
Between the dual storylines of the EHT collaboration and the scientists working on soft hair, other work in black hole physics is discussed, including water-based simulations and LIGO’s work on gravitational waves.
