Kenny Higginbotham
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qgkenny.bsky.social
Kenny Higginbotham
@qgkenny.bsky.social
Postdoc at Perimeter Institute • Using HEP theory and quantum info to understand quantum gravity • BS: Georgia Tech • PhD: CU Boulder
Thankful to have been on this list! I graduated in May, so you should give my spot to a current grad student. (Any chance there's a postdoc list going...?)
September 30, 2025 at 8:03 PM
This was recently recommended to me! I haven't gotten around to it yet, but it's on my list
July 10, 2025 at 4:07 PM
Possibly! This would certainly allow us to add a baby universe to a holographic map for de Sitter by allowing for post-selection. It would be interesting to construct a model like Antonini-Sasieta-Swingle and Antonini-Rath for de Sitter + baby!
July 10, 2025 at 4:04 PM
Oh no! What have we done!?
July 9, 2025 at 7:04 PM
I think so! I included success kid in the post, but not the paper.

But maybe it's also computationally difficult to determine if the post contains a meme...
July 9, 2025 at 5:25 PM
It’s been a great time so far! I’m especially looking forward to next week’s lectures.
June 11, 2025 at 1:22 AM
Congrats! See you in Boulder this summer!
April 4, 2025 at 3:42 AM
Either approach (HUZ's or ours) can be used to include observers in generic holographic maps for both open and closed universes in any dimension. I'm excited about the possibilities both proposals open up for studying observers in holographic maps! (9/9)
March 14, 2025 at 9:08 PM
Our approach: remove the part of the holographic map that acts on the observer. Thus the new non-trivial Hilbert space is given by the observer's Hilbert space AND the area of the boundary separating them from the rest of the universe. (8/9)
March 14, 2025 at 9:08 PM
No such holographic code has been proposed to match AAIL's rules for including an observer. We do just that! This allows a more thorough comparison between the two different approaches. (7/9)
March 14, 2025 at 9:08 PM
Their approach: clone the observer to a non-gravitational reference outside the closed universe. Thus the new non-trivial Hilbert space is given by the observer's Hilbert space. (6/9)
March 14, 2025 at 9:08 PM
HUZ also describes how their method can be used to include an observer in a non-isometric holographic map describing the closed universe. They show that this reproduces their results from the gravitational path integral. (5/9)
March 14, 2025 at 9:08 PM