50 research outputs found
Radial coordinates for defect CFTs
We study the two-point function of local operators in the presence of a
defect in a generic conformal field theory. We define two pairs of cross
ratios, which are convenient in the analysis of the OPE in the bulk and defect
channel respectively. The new coordinates have a simple geometric
interpretation, which can be exploited to efficiently compute conformal blocks
in a power expansion. We illustrate this fact in the case of scalar external
operators. We also elucidate the convergence properties of the bulk and defect
OPE decompositions of the two-point function. In particular, we remark that the
expansion of the two-point function in powers of the new cross ratios converges
everywhere, a property not shared by the cross ratios customarily used in
defect CFT. We comment on the crucial relevance of this fact for the numerical
bootstrap.Comment: Matches journal version; the attached mathematica file (Bulk CB.nb +
rec.txt) computes the conformal blocks in the bulk channe
Decoding a Three-Dimensional Conformal Manifold
We study the one-dimensional complex conformal manifold that controls the
infrared dynamics of a three-dimensional supersymmetric theory
of three chiral superfields with a cubic superpotential. Two special points on
this conformal manifold are the well-known XYZ model and three decoupled copies
of the critical Wess-Zumino model. The conformal manifold enjoys a discrete
duality group isomorphic to and can be thought of as an orbifold of
. We use the expansion and the numerical
conformal bootstrap to calculate the spectrum of conformal dimensions of
low-lying operators and their OPE coefficients, and find a very good
quantitative agreement between the two approaches.Comment: 59 pages, 13 figure
Analytic and numerical bootstrap for the long-range Ising model
We combine perturbation theory with analytic and numerical bootstrap techniques to study the critical point of the long-range Ising (LRI) model in two and three dimensions. This model interpolates between short-range Ising (SRI) and mean-field behaviour. We use the Lorentzian inversion formula to compute infinitely many three-loop corrections in the two-dimensional LRI near the mean-field end. We further exploit the exact OPE relations that follow from bulk locality of the LRI to compute infinitely many two-loop corrections near the mean-field end, as well as some one-loop corrections near SRI. By including such exact OPE relations in the crossing equations for LRI we set up a very constrained bootstrap problem, which we solve numerically using SDPB. We find a family of sharp kinks for two- and three-dimensional theories which compare favourably to perturbative predictions, as well as some Monte Carlo simulations for the two-dimensional LRI
Perturbative RG flows in AdS: an \'etude
We discuss general properties of perturbative RG flows in AdS with a focus on
the treatment of boundary conditions and infrared divergences. In contrast with
flat-space boundary QFT, general covariance in AdS implies the absence of
independent boundary flows. We illustrate how boundary correlation functions
remain conformally covariant even if the bulk QFT has a scale. We apply our
general discussion to the RG flow between consecutive unitary diagonal minimal
models which is triggered by the operator. For these theories we
conjecture a flow diagram whose form is significantly simpler than that in
flat-space boundary QFT. In several stand-alone appendices we discuss
two-dimensional BCFTs in general and the minimal model BCFTs in particular.
These include both an extensive review as well as the computation of several
new BCFT correlation functions.Comment: v3: published versio
Bootstrapping line defects with global symmetry
We use the numerical bootstrap to study conformal line defects with
global symmetry. Our results are very general and capture in particular
conformal line defects originating from bulk CFTs with a continuous global
symmetry, which can either be preserved or partially broken by the presence of
the defect. We begin with an agnostic approach and perform a systematic
bootstrap study of correlation functions between two canonical operators on the
defect: the displacement and the tilt. We then focus on two interesting
theories: a monodromy line defect and a localized magnetic field line defect.
To this end, we combine the numerical bootstrap with the
-expansion, where we complement existing results in the literature
with additional calculations. For the monodromy defect our numerical results
are consistent with expectations, with known analytic solutions sitting inside
our numerical bounds. For the localized magnetic field line defect our plots
show a series of intriguing cusps which we explore.Comment: 54 pages, 11 figure
The acetyltransferase p300 is recruited in trans to multiple enhancer sites by lncSmad7
The histone acetyltransferase p300 (also known as KAT3B) is a general transcriptional coactivator that introduces the H3K27ac mark on enhancers triggering their activation and gene transcription. Genome-wide screenings demonstrated that a large fraction of long non-coding RNAs (lncRNAs) plays a role in cellular processes and organ development although the underlying molecular mechanisms remain largely unclear (1,2). We found 122 lncRNAs that interacts directly with p300. In depth analysis of one of these, lncSmad7, is required to maintain ESC self-renewal and it interacts to the C-terminal domain of p300. lncSmad7 also contains predicted RNA-DNA Hoogsteen forming base pairing. Combined Chromatin Isolation by RNA precipitation followed by sequencing (ChIRP-seq) together with CRISPR/Cas9 mutagenesis of the target sites demonstrate that lncSmad7 binds and recruits p300 to enhancers in trans, to trigger enhancer acetylation and transcriptional activation of its target genes. Thus, these results unveil a new mechanism by which p300 is recruited to the genome
MAORY for ELT: preliminary design overview
MAORY is one of the approved instruments for the European Extremely Large Telescope. It is an adaptive optics module, enabling high-angular resolution observations in the near infrared by real-time compensation of the wavefront distortions due to atmospheric turbulence and other disturbances such as wind action on the telescope. An overview of the instrument design is given in this paper