Untitled attachment
https://files.mastodon.social/media_attachments/files/111/410/670/963/138/608/original/71260b52b81dd89b.png
Outside the black hole (r > 2M) there are two sorts of radial null geodesics: light rays can follow a path that moves outward (towards larger r) or one that moves inward (towards smaller r).
Inside (r < 2M) the two sorts of null geodesics both head inwards, towards smaller r.
Notice that at each point along the infalling observer's worldline, they find themself inside a "light cone" defined by the two sort of radial null geodesics emitted at their previous location, the instant before.
Chirp! is a social network. It runs on GNU social, version 2.0.1-beta0, available under the GNU Affero General Public License.
All Chirp! content and data are available under the Creative Commons Attribution 3.0 license.