exact path integral for 3d quantum gravityhome.kias.re.kr/mkg/upload/kiasyitp2015/terashima.pdf ·...
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![Page 1: Exact Path Integral for 3D Quantum Gravityhome.kias.re.kr/MKG/upload/KIASYITP2015/Terashima.pdf · 2015-09-23 · 3d pure gravity 3d Chern-Simons theory 3d SUSY Chern-Simons . 8 3d](https://reader034.vdocuments.us/reader034/viewer/2022050308/5f7043969b0e0d1ff561c473/html5/thumbnails/1.jpg)
Exact Path Integral
for 3D Quantum Gravity
Seiji Terashima (YITP)
16 September 2015 at KIAS-YITP workshop
based on the paper collaborated with Norihiro Iizuka and Akinori Tanaka: arXiv:1504.05991
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Introduction
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Quantum Gravity:
Difficulties:
• Perturbatively unrenormalizable
• Un-boundedness of action
• Summations over different topologies
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Dual CFT (for QG with asymptotic AdS)
Renormalizable, Positive definite action,
No geometries (for finite N).
However, no proof of the equivalence
Maldacena
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In this talk,
we will try to compute QG partition function
from bulk theory.
(Is it possible?)
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3d pure gravity (with negative cosmological constant)
Simplest theory with “black holes”
(although no gravitons)
They are called BTZ black holes,
which have horizons and nonzero entropies
Banados-Teitelboim-Zanelli
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We will use following relations:
3d pure gravity
3d Chern-Simons theory
3d SUSY Chern-Simons
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3d SUSY Chern-Simons theory
We can use localization technique
to compute exact partition function (with some assumptions)
The result for c=24 is
which is Z for Frenkel-Lepowsky-Meurman’s CFT,
as Witten proposed before!
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•Introduction
•Review of 3d gravity
•Previous results
•Exact partition function using localization
Plan
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Review of 3d gravity
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3d pure gravity
What we want to compute is
with
where
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Central charge of dual CFT
from classical 3d gravity
Asymptotic symmetry of 3d QG with asymptotic AdS_3
is
Virasoro algebra with the central charge:
Using this and Cardy formula,
we can reproduce
entropy of BTZ black hole (leading order).
Strominger
Brown-Henneaux
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3d pure QG 3D Chern-Simons
(classical)
Achucarro-Townsend, Witten
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3d pure QG 3D Chern-Simons
(classical)
Therefore,
Achucarro-Townsend, Witten
Witten
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Previous results
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What we will compute:
Partition function of Euclidian 3d gravity with
asymptoric AdS with torus boundary.
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Important facts of the theory:
only solutions of e.o.m. are
AdS space and BTZ black holes.
all of them are topologically solid torus
but, contractable cycles of torus are different.
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Important facts of the theory:
Moreover, they are related by SL(2,Z) action
and the on-shell action is
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3d pure QG 2d extremal CFT
From CS description, Witten suggest that
partition function of 3d gravity may be
holomorphically factorized:
For c=24, there is unique CFT by FLM with
Frenkel-Lepowsky-Meurman
Witten
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J-function as a (classical) partition function
Manschot
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J-function as a (classical) partition function
Manschot
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J-function as a (classical) partition function
Manschot
However,
we do not know
why there is no loop corrections,
nor,
why including non-geometric contributions
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Partition function (classical + 1-loop) Maloney-Witten
Perturbatively, 3d gravity is 1-loop exact,
and for AdS background we have
Witten
Giombi-Maloney-Yin
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Partition function (classical + 1-loop) Maloney-Witten
Thus, naively
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Partition function (classical + 1-loop) Maloney-Witten
Even if we assume holomorphic factorized one
We can not have J-function for c=24
because of
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So, there are many mysteries…
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Path-integral of 3D Gravity
using localization
Iizuka-Tanaka-ST
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We will use following relations:
3d pure gravity
3d Chern-Simons theory
3d SUSY Chern-Simons
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3d SUSY Chern-Simons theory
Let us consider
with the SUSY action
where additional fermion and bosons
are auxiliary fields.
Therefore,
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SUSY CS theory on solid torus
The solid torus
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Partition functions are related as
This will be justified by the localization
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Using localization technique Sugishita-ST
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Saddle points equation:
this corresponds to e.o.m. of gravity
the solution (BTZ) is
Note that
the solutions of e.o.m. should have
solid torus topology.
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The partition function:
Other contributions are obtained
by SL(2,Z) action
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Rademacher sum:
For c=24, we have
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How about the Virasoro decendants modes?
We have seen that
which can be rewritten as
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SUSY CS has extra fermion modes:
Using doubling trick:
we will define
Then, the mass term is
domain wall type mass term,
massless “edge” modes on x=0
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SUSY CS has extra fermion modes:
These fermion modes strictly localized
at the boundary and then
completely decoupled from other modes
for t → 0
Thus, we can think the theory essentially describe
3d pure gravity
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• “exact” partition function of 3d pure
gravity
• Using SUSY extension and localziation
Conclusion
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Fin.
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