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Prog. Theor. Phys. Vol. 107 No. 5 (2002) pp. 1085-1104
Holographic Renormalization Group Structure in Higher-Derivative Gravity
Masafumi Fukuma*,** and
So Matsuura***
Yukawa Institute for Theoretical Physics,
Kyoto University, Kyoto 606-8502, Japan
(Received December 12, 2001)
Abstract:
Classical higher-derivative gravity is investigated
in the context of the holographic renormalization group (RG).
We parametrize the Euclidean time such that
one step of time evolution in (d+1)-dimensional bulk gravity
can be directly interpreted as that of block spin transformation
of the d-dimensional boundary field theory.
This parametrization simplifies
the analysis of the holographic RG structure in gravity systems,
and conformal fixed points are always described by AdS geometry.
We find that higher-derivative gravity generically
induces extra degrees of freedom,
which acquire huge masses around stable fixed points
and thus are coupled to highly irrelevant operators at the boundary.
In the particular case of pure R2-gravity,
we show that some region of values of the coefficients
of the curvature-squared terms
allows us to have two fixed points (one is multicritical),
which are connected by a kink solution.
We further extend our analysis to Lorentzian metric
to investigate a model of expanding universe
described by the action with curvature-squared terms
and a positive cosmological constant.
We show that,
in any dimensionality but four,
there is a classical solution
that describes the time evolution from
one de Sitter geometry to another de Sitter geometry,
along which the Hubble parameter changes significantly.
URL :
http://ptp.ipap.jp/link?PTP/107/1085/
DOI : 10.1143/PTP.107.1085
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Citing Article(s) :
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Progress of Theoretical Physics Vol. 108 No. 2 (2002) pp. 375-382
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Comment on Field Redefinitions in the AdS/CFT Correspondence
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Masafumi Fukuma and So Matsuura
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Progress of Theoretical Physics Vol. 109 No. 4 (2003) pp. 489-562
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Holographic Renormalization Group
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Masafumi Fukuma, So Matsuura and Tadakatsu Sakai