Holographic Complexity for Systems with Defects
It from Qubit School and Workshop YITP, Kyoto 23 June 2019
Giuseppe Policastro Dongsheng Ge
Universiteit van Amsterdam
Shira Chapman – University of Amsterdam
hep-th/1811.12549
Holographic Complexity for Systems with Defects Universiteit van - - PowerPoint PPT Presentation
Holographic Complexity for Systems with Defects Universiteit van Amsterdam Shira Chapman University of Amsterdam It from Qubit School and Workshop YITP, Kyoto 23 June 2019 Dongsheng Ge hep-th/1811.12549 Giuseppe Policastro Quantum
Giuseppe Policastro Dongsheng Ge
Universiteit van Amsterdam
hep-th/1811.12549
Complexity=Volume of a maximal spacelike slice anchored at the boundary time slice at which the state is defined (Stanford & Susskind)
patch – union of all such spacelike slices
(Brown, Roberts, Swingle, Susskind & Zhao)
In many cases the two proposals yield very similar results
Structure of divergences (Carmi, Myers, Rath; Reynolds, Ross)
(Stanford, Susskind; Brown, Roberts, Swingle, Susskind, Zhao)
Chaotic evolution with Lyapunov exponent
evolution after
∗
We want to understand cases where the proposals are not equivalent.
Exact Solution Including Backreaction
(Azeyanagi, Karch, Takayanagi and Thompson) folding trick
(Abt, Erdmenger, Hinrichsen, Melby-Thompson, Meyer, Northe, Reyes)
Fixing the Cutoff in the defect region along a line of constant r – connects smoothly across the defect
Defect Contribution
the Einstein Hilbert term
Null surface contributions
counter-term length scale).
∗
𝑑 = 3𝑀 2𝐻
The complexity is proportional to the maximal volume enclosed between the boundary subregion and its Ryu-Takayanagi surface (Alishahiha)
Matching the RT surface across the defect – minimize total length
is continuous
∗
(Azeyanagi, Karch, Takayanagi and Thompson)
∗
(D. Carmi, R. C. Myers and P. Rath)
Focus on the symmetric case
cancels, additional log divergence
Matching conditions (Bachas, de Boer, Dijkgraaf, Ooguri)
Marrochio, Pastawski). Use the spectrum assuming that the QFT formula
naively generalizes (the boundary size is
)
and we recover the
vacuum result. Log contribution does not depend on the defect parameter – favors CA Zero modes for compact boson?
Δ ≡ 1 𝜌 tan 𝜇𝜇 − 1 𝜇 + 𝜇 𝜕 = Λ e reference state frequency
Higher Dimensions? Other holographic defects? Janus Solution Different codimension defects? Asymmetric defects? Zero modes? Complexity in CFT?