About
Understanding quantum gravity is one of the biggest intellectual challenges of modern science. String theory and the related AdS/CFT correspondence provide a rigorous theoretical laboratory to address some aspects of quantum gravity, and a few semi-classical quantum gravity effects, notably the existence of Hawking radiation, are well-established and understood. However we are strongly handicapped by the inability to perform experiments that probe quantum gravity effects directly. In recent years a series of results have established a promising pathway towards exhibiting and exploring genuine quantum gravity effects in a laboratory setting. This pathway exploits what appears to be a fundamental relationship between the connectedness of spacetime and quantum entanglement, as well as the holographic duality between certain bulk gravity phenomena and non-gravitational quantum systems. Both ideas are realized in the phenomenon of traversable wormholes, which have been shown in the rigorous context of AdS/CFT to be a feature of semi-classical quantum gravity. Such wormholes are rendered traversable by a quantum effect involving a flux of negative energy, similar to the quantum phenomenon that enables Hawking radiation. Furthermore these wormholes have a holographic dual description as a new form of quantum teleportation, which can be explicitly realized in the dynamics of the SYK model with N interacting Majorana fermions. There is considerable evidence that N~100 should be good enough to exhibit the key properties of traversable wormholes in a laboratory setting, e.g., by producing the dynamics on a quantum processor. I will describe how such experiments might be performed and what we could learn from them. .
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The talk
Credits and licence
- Institution
- CERN
- Department
- Theory Colloquia
- Speaker
- Joseph Lykken
- Year
- 2022
- Language
- English
- Subjects
- Physics
- 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 Tweens profiles and older, judged from what the source says about it. How courses are placed