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Dive into the research topics where Sera Cremonini is active.

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Featured researches published by Sera Cremonini.


Journal of High Energy Physics | 2013

On the IR completion of geometries with hyperscaling violation

Jyotirmoy Bhattacharya; Sera Cremonini; Annamaria Sinkovics

A bstractWe study solutions to Einstein-Maxwell-dilaton gravity with a constant magnetic flux which describe, in the holographic AdS/CFT framework, field theories characterized by a dynamical critical exponent and a hyperscaling violation exponent. Such solutions are known to be IR-incomplete due to the presence of a running dilaton, which drives the theory towards strong coupling in the IR, where quantum corrections become important. After introducing generic corrections, in this note we examine the conditions for the emergence of an AdS2 ×R2 region close to the horizon, which provides an IR-completion for the hyperscaling violating solutions. In the presence of these corrections, we construct explicit numerical solutions where the geometry flows from AdS4 in the UV to AdS2 × R2 in the deep IR, with an intermediate region which exhbits both hyperscaling violation and Lifshitz-like scaling. We also provide constraints on the structure of Einstein-Maxwell-dilaton theories that admit such solutions, as well as an emergent AdS2 × R2 region in the infrared.


Journal of Cosmology and Astroparticle Physics | 2011

Strongly Coupled Perturbations in Two-Field Inflationary Models

Sera Cremonini; Zygmunt Lalak; Krzysztof Turzyński

We study models of inflation with two scalar fields and non-canonical kinetic terms, focusing on the case in which the curvature and isocurvature perturbations are strongly coupled to each other. In the regime where a heavy mode can be identified and integrated out, we clarify the passage from the full two-field model to an effectively single-field description. However, the strong coupling sets a new scale in the system, and affects the evolution of the perturbations as well as the beginning of the regime of validity of the effective field theory. In particular, the predictions of the model are sensitive to the relative hierarchy between the coupling and the mass of the heavy mode. As a result, observables are not given unambiguously in terms of the parameters of an effectively single field model with non-trivial sound speed. Finally, the requirement that the sound horizon crossing occurs within the regime of validity of the effective theory leads to a lower bound on the sound speed. Our analysis is done in an extremely simple toy model of slow-roll inflation, which is chosen for its tractability, but is non-trivial enough to illustrate the richness of the dynamics in non-canonical multi-field models.


Journal of Cosmology and Astroparticle Physics | 2012

Decoupling survives inflation: a critical look at effective field theory violations during inflation

Anastasios Avgoustidis; Sera Cremonini; Anne-Christine Davis; Raquel H. Ribeiro; Krzysztof Turzyński; Scott Watson

We investigate the validity of effective field theory methods and the decoupling of heavy fields during inflation. Considering models of inflation in which the inflaton is coupled to a heavy (super-Hubble) degree of freedom initially in its vacuum state, we find that violations of decoupling are absent unless there is a breakdown of the slow-roll conditions. Next we allow for a temporary departure from inflation resulting in a period of non-adiabaticity during which effective field theory methods are known to fail. We find that the locality of the event and energy conservation lead to a tight bound on the size of the effects of the heavy field. We discuss the implications for the power spectrum and non-gaussianity, and comment on the connection with recent studies of the dynamics of multi-field inflation models. Our results further motivate the use of effective field theory methods to characterize cosmic inflation, and focus the question of observability of additional degrees of freedom during inflation to near the Hubble scale or below — as anticipated from the Wilsonian notions of decoupling and naturalness.


Journal of High Energy Physics | 2010

Correlation Functions and Hidden Conformal Symmetry of Kerr Black Holes

Melanie Becker; Sera Cremonini; Waldemar Schulgin

Extremal scalar three-point correlators in the near-NHEK geometry of Kerr black holes have recently been shown to agree with the result expected from a holographically dual non-chiral two-dimensional conformal field theory. In this paper we extend this calculation to extremal three-point functions of scalars in a general Kerr black hole which need not obey the extremality condition


Journal of High Energy Physics | 2014

Spatially Modulated Instabilities of Geometries with Hyperscaling Violation

Sera Cremonini; Annamaria Sinkovics

M = \sqrt {J}


Journal of High Energy Physics | 2011

Extremal three-point correlators in Kerr/CFT

Melanie Becker; Sera Cremonini; Waldemar Schulgin

. It was recently argued that for low frequency scalars in the Kerr geometry there is a dual conformal field theory description which determines the interactions in this regime. Our results support this conjecture. Furthermore, we formulate a recipe for calculating finite-temperature retarded three-point correlation functions which is applicable to a large class of (even non-extremal) correlators, and discuss the vanishing of the extremal couplings.


Journal of High Energy Physics | 2010

Higher derivative corrections to R-charged black holes: boundary counterterms and the mass-charge relation

Sera Cremonini; James T. Liu; Phillip Szepietowski

A bstractWe perform a study of possible instabilities of the infrared AdS2 ×


Journal of Cosmology and Astroparticle Physics | 2012

The importance of slow-roll corrections during multi-field inflation

Anastasios Avgoustidis; Sera Cremonini; Anne-Christine Davis; Raquel H. Ribeiro; Krzysztof Turzyński; Scott Watson

{{\mathbb{R}}^2}


Journal of High Energy Physics | 2010

Viscosity bound and causality in superfluid plasma

Alex Buchel; Sera Cremonini

region of solutions to Einstein-Maxwell-dilaton systems which exhibit an intermediate regime of hyperscaling violation and Lifshitz scaling. Focusing on solutions that are magnetically charged, we probe the response of the system to spatially modulated fluctuations, and identify regions of parameter space in which the infrared AdS2 geometry is unstable to perturbations. The conditions for the existence of instabilities translate to restrictions on the structure of the gauge kinetic function and scalar potential. In turn, these can lead to restrictions on the dynamical critical exponent z and on the amount of hyperscaling violation θ. Our analysis thus provides further evidence for the notion that the true ground state of ‘scaling’ solutions with hyperscaling violation may be spatially modulated phases.


Journal of High Energy Physics | 2015

Intermediate scalings in holographic RG flows and conductivities

Jyotirmoy Bhattacharya; Sera Cremonini; Blaise Goutéraux

We compute three-point correlation functions in the near-extremal, near-horizon region of a Kerr black hole, and compare to the corresponding finite-temperature conformal field theory correlators. For simplicity, we focus on scalar fields dual to operators

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