About
Recent development of quantum technologies suggest an exciting new direction of the study of quantum gravity: We might be able to create black holes! More precisely, we might be able to use quantum devices to simulate (seemingly) non-gravitational systems that are equivalent to quantum black holes via holography. For such a purpose, the D0-brane matrix model is probably the simplest target that has well-controlled limit that describes weakly-coupled gravity.
In this talk, we show the latest results of numerical simulations of the D0-brane matrix model. The duality between the matrix model and type IIA superstring theory is confirmed with a good precision, including stringy corrections. Furthermore, we find a new low-energy phase (confined phase) and suggest that this phase describes M-theory. We further argue that the matrix model can describe the eleven-dimensional Schwarzschild black hole.
If time permits, we will provide a rough resource estimate for quantum simulation. .
0:00:00 Slide 1
0:01:15 Slide 2
0:04:16 Slide 3
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0:09:00 Slide 6
0:12:51 Slide 7
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0:15:20 Slide 9
The talk
Credits and licence
- Institution
- CERN
- Department
- Theory Colloquia
- Speaker
- Masanori Hanada
- Year
- 2023
- Language
- English
- Source
- CERN
- Licence
- CERN, as CERN states it. CERN's terms
- Attribution
- © CERN. CERN provides its audiovisual media free of charge for educational and informational use, credited to CERN; this lecture is shown in CERN's own player.
- Who can watch
- CERN gives no rating. Invisible Network shows it to Teens profiles and older, judged from what the source says about it. How courses are placed