107 research outputs found
Constraints from Conformal Symmetry on the Three Point Scalar Correlator in Inflation
Using symmetry considerations, we derive Ward identities which relate the
three point function of scalar perturbations produced during inflation to the
scalar four point function, in a particular limit. The derivation assumes
approximate conformal invariance, and the conditions for the slow roll
approximation, but is otherwise model independent. The Ward identities allow us
to deduce that the three point function must be suppressed in general, being of
the same order of magnitude as in the slow roll model. They also fix the three
point function in terms of the four point function, upto one constant which we
argue is generically suppressed. Our approach is based on analyzing the wave
function of the universe, and the Ward identities arise by imposing the
requirements of spatial and time reparametrization invariance on it.Comment: 35 pages; Extra references and comments added, The version published
in JHE
Ward Identities for Scale and Special Conformal Transformations in Inflation
We derive the general Ward identities for scale and special conformal
transformations in theories of single field inflation. Our analysis is model
independent and based on symmetry considerations alone. The identities we
obtain are valid to all orders in the slow roll expansion. For special
conformal transformations, the Ward identities include a term which is
non-linear in the fields that arises due to a compensating spatial
reparametrization. Some observational consequences are also discussed.Comment: 42 Pages. v3: Section on checks of the Ward identities added. The
JHEP accepted versio
Interpolating from Bianchi Attractors to Lifshitz and AdS Spacetimes
We construct classes of smooth metrics which interpolate from Bianchi
attractor geometries of Types II, III, VI and IX in the IR to Lifshitz or
geometries in the UV. While we do not obtain these metrics
as solutions of Einstein gravity coupled to a simple matter field theory, we
show that the matter sector stress-energy required to support these geometries
(via the Einstein equations) does satisfy the weak, and therefore also the
null, energy condition. Since Lifshitz or geometries can in
turn be connected to spacetime, our results show that there is no
barrier, at least at the level of the energy conditions, for solutions to arise
connecting these Bianchi attractor geometries to spacetime. The
asymptotic spacetime has no non-normalizable metric deformation turned
on, which suggests that furthermore, the Bianchi attractor geometries can be
the IR geometries dual to field theories living in flat space, with the
breaking of symmetries being either spontaneous or due to sources for other
fields. Finally, we show that for a large class of flows which connect two
Bianchi attractors, a C-function can be defined which is monotonically
decreasing from the UV to the IR as long as the null energy condition is
satisfied. However, except for special examples of Bianchi attractors
(including AdS space), this function does not attain a finite and non-vanishing
constant value at the end points.Comment: 37 pages, 12 figures, The comment regarding the behavior of
C-function for general Bianchi Types appearing in IR or UV clarified, the
relation of Type IX with for made more precise
and a comment regarding type V added in the conclusio
Modeling the Impact of Process Variation on Resistive Bridge Defects
Recent research has shown that tests generated without taking process variation into account may lead to loss of test quality. At present there is no efficient device-level modeling technique that models the effect of process variation on resistive bridges. This paper presents a fast and accurate technique to model the effect of process variation on resistive bridge defects. The proposed model is implemented in two stages: firstly, it employs an accurate transistor model (BSIM4) to calculate the critical resistance of a bridge; secondly, the effect of process variation is incorporated in this model by using three transistor parameters: gate length (L), threshold voltage (V) and effective mobility (ueff) where each follow Gaussian distribution. Experiments are conducted on a 65-nm gate library (for illustration purposes), and results show that on average the proposed modeling technique is more than 7 times faster and in the worst case, error in bridge critical resistance is 0.8% when compared with HSPICE
On Improving Reliability of SRAM-Based Physically Unclonable Functions
Physically unclonable functions (PUFs) have been touted for their inherent resistance to invasive attacks and low cost in providing a hardware root of trust for various security applications. SRAM PUFs in particular are popular in industry for key/ID generation. Due to intrinsic process variations, SRAM cells, ideally, tend to have the same start-up behavior. SRAM PUFs exploit this start-up behavior. Unfortunately, not all SRAM cells exhibit reliable start-up behavior due to noise susceptibility. Hence, design enhancements are needed for improving reliability. Some of the proposed enhancements in literature include fuzzy extraction, error-correcting codes and voting mechanisms. All enhancements involve a trade-off between area/power/performance overhead and PUF reliability. This paper presents a design enhancement technique for reliability that improves upon previous solutions. We present simulation results to quantify improvement in SRAM PUF reliability and efficiency. The proposed technique is shown to generate a 128-bit key in ≤0.2 μ\u27\u3eμμ s at an area estimate of 4538 μ\u27\u3eμμ m 2\u27\u3e22 with error rate as low as 10−6\u27\u3e10−610−6 for intrinsic error probability of 15%
Extremal Horizons with Reduced Symmetry: Hyperscaling Violation, Stripes, and a Classification for the Homogeneous Case
Classifying the zero-temperature ground states of quantum field theories with
finite charge density is a very interesting problem. Via holography, this
problem is mapped to the classification of extremal charged black brane
geometries with anti-de Sitter asymptotics. In a recent paper [1], we proposed
a Bianchi classification of the extremal near-horizon geometries in five
dimensions, in the case where they are homogeneous but, in general,
anisotropic. Here, we extend our study in two directions: we show that Bianchi
attractors can lead to new phases, and generalize the classification of
homogeneous phases in a way suggested by holography. In the first direction, we
show that hyperscaling violation can naturally be incorporated into the Bianchi
horizons. We also find analytical examples of "striped" horizons. In the second
direction, we propose a more complete classification of homogeneous horizon
geometries where the natural mathematics involves real four-algebras with three
dimensional sub-algebras. This gives rise to a richer set of possible
near-horizon geometries, where the holographic radial direction is
non-trivially intertwined with field theory spatial coordinates. We find
examples of several of the new types in systems consisting of reasonably simple
matter sectors coupled to gravity, while arguing that others are forbidden by
the Null Energy Condition. Extremal horizons in four dimensions governed by
three-algebras or four-algebras are also discussed.Comment: 58 pages, 1 figure and 1 cartoon. v2: references adde
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