Learn · CERN

Talk45 min

Hydrodynamisation and entanglement entropy in expanding spacetimes

Wilke Van Der Schee · CERN

Watch At CERN

About

This talk will be about hydrodynamisation in an FRW universe and entanglement entropy in empty 4-dimensional de Sitter spacetime of a non-conformal QFT [1]. I will first briefly describe the set-up and show how a hydrodynamic plasma dilutes and falls out of equilibrium due to expansion towards empty de Sitter spacetime. Interestingly, in the empty setting we can show that extremal surfaces in the holographic dual of spherical entangling regions on the boundary QFT probe beyond the dual event horizon if and only if the entangling region is larger than the cosmological horizon. Finally, I will show new results on hydrodynamisation when including dynamical gravity on the boundary.

[1] Jorge Casalderrey-Solana, Christian Ecker, David Mateos and WS, Strong-coupling dynamics and entanglement in de Sitter space, 2011.08194.

0:00:00 Slide 1

0:04:25 Slide 2

0:08:49 Slide 3

0:13:13 Slide 4

0:17:38 Slide 5

0:22:02 Slide 6

0:26:26 Slide 7

0:30:51 Slide 8

0:35:15 Slide 9

0:39:39 Slide 10

The talk

  1. Hydrodynamisation and entanglement entropy in expanding spacetimes 2021-07-26 · 45 min · CERN's player

Credits and licence

Institution
CERN
Department
Conferences & Workshops
Speaker
Wilke Van Der Schee
Year
2021
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