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Publications (24)
A class of inflationary scenarios for primordial black hole (PBH) formation include a small barrier in the slope of the potential. There, the inflaton slows down, generating an enhancement of primordial perturbations. Moreover, the background solution overcomes the barrier at a very low speed, and large backward quantum fluctuations can prevent cer...
A class of inflationary scenarios for primordial black hole (PBH) formation include a small barrier in the slope of the potential. There, the inflaton slows down, generating an enhancement of primordial perturbations. Moreoever, the background solution overcomes the barrier at a very low speed, and large backward quantum fluctuations can prevent ce...
Black holes binaries coming from a distribution of primordial black holes might exhibit a large merger rate up to large redshifts. Using a phenomenological model for the merger rate, we show that changes in its slope, up to redshifts z∼4, are constrained by current limits on the amplitude of the stochastic gravitational wave background from LIGO/Vi...
Black holes binaries coming from a distribution of primordial black holes might exhibit a large merger rate up to large redshifts. Using a phenomenological model for the merger rate, we show that changes in its slope, up to redshifts $z\sim 4$, are constrained by current limits on the amplitude of the stochastic gravitational wave background from L...
We give an explanation for the signal detected by NANOGrav as the stochastic gravitational wave background from binary mergers of primordial "Stupendously Large Black Holes"(SLABs) of mass M ∼ (1011-1012)M , and corresponding to roughly 0.1% of the dark matter. We show that the stringent bounds coming from μ distortions of the CMB can be surpassed...
We investigate in detail the spectrum of gravitational waves induced by a peaked primordial curvature power spectrum generated in single-field inflationary models. We argue that the f NL parameter can be inferred by measuring the high frequency spectral tilt of the induced gravitational waves. We also show that the intrinsically non-Gaussian impact...
We investigate in detail the spectrum of gravitational waves induced by a peaked primordial curvature power spectrum generated in single field inflationary models. We argue that the $f_{\rm NL}$ parameter can be inferred by measuring the high frequency spectral tilt of the induced gravitational waves. We also show that the intrinsically non-Gaussia...
We give an explanation for the signal detected by NANOGrav as the stochastic gravitational wave background from binary mergers of primordial "Stupendously Large Black Holes" (SLABs) of mass $M\sim(10^{11}-10^{12})M_{\odot}$, and corresponding to roughly $0.1\%$ of the dark matter. We show that the stringent bounds coming from $\mu$ distortions of t...
We discuss the effect of clustering for the determination of the merger rate of binary black holes in the LIGO/Virgo mass range. While for a Poissonian initial distribution, and assuming isolated binaries, the allowed fraction of Primordial Black Holes (PBHs) to dark matter (DM) is a few percent, we show that this bound can be relaxed if PBHs are c...
We discuss the effect of clustering for the determination of the merger rate of binary black holes in the LIGO mass range. While for a Poissonian initial distribution, and assuming isolated binaries, the allowed fraction of Primordial Black Holes (PBHs) to dark matter (DM) is a few percent, we show that this bound can be relaxed if PBHs are cluster...
Primordial black holes (PBHs) may result from high peaks in a random field of cosmological perturbations. In single field inflationary models, such perturbations can be seeded as the inflaton overshoots a small barrier on its way down the potential. PBHs are then produced through two distinct mechanisms, during the radiation era. The first one is t...
In the context of transient constant-roll inflation near a local maximum, we derive the non-perturbative field redefinition that relates a Gaussian random field with the true non-Gaussian curvature perturbation. Our analysis shows the emergence of a new critical amplitude ζ*, corresponding to perturbations that prevent the inflaton from overshootin...
We re-analyse current single-field inflationary models related to primordial black holes formation. We do so by taking into account recent developments on the estimations of their abundances and the influence of non-gaussianities. We show that, for all of them, the gaussian approximation, which is typically used to estimate the primordial black hol...
We re-analyse current single-field inflationary models related to primordial black holes formation. We do so by taking into account recent developments on the estimations of their abundances and the influence of non-gaussianities. We show that, for all of them, the gaussian approximation, which is typically used to estimate the primordial black hol...
In multi-field inflation one or more non-adiabatic modes may become light, potentially inducing large levels of isocurvature perturbations in the cosmic microwave background. If in addition these light modes are coupled to the adiabatic mode, they influence its evolution on super horizon scales. Here we consider the case in which a non-adiabatic mo...
In multi-field inflation one or more non-adiabatic modes may become light, potentially inducing large levels of isocurvature perturbations in the cosmic microwave background. If in addition these light modes are coupled to the adiabatic mode, they influence its evolution on super horizon scales. Here we consider the case in which a non-adiabatic mo...
The simplest two-field completion of natural inflation has a regime in which
both fields are active and in which its predictions are within the Planck
1-$\sigma$ confidence contour. We show this for the original model of natural
inflation, in which inflation is achieved through the explicit breaking of a
U(1) symmetry. We consider the case in which...
In the context of single field inflation, models with a quadratic potential
and models with a natural potential with subplanckian decay constant are in
tension with the Planck data. We show that, when embedded in a two-field model
with an additional super massive field, they can become consistent with
observations. Our results follow if the inflato...
We continue the study of mild transient reductions in the speed of sound of
the adiabatic mode during inflation, of their effect on the primordial power
spectrum and bispectrum, and of their detectability in the Cosmic Microwave
Background (CMB). We focus on the regime of {\it moderately sharp} mild
reductions in the speed of sound during uninterru...
We perform a search for localized oscillatory features in the Planck CMB
power spectrum, assuming they are caused by a transient reduction in the speed
of sound of the adiabatic mode during effectively single-field, uninterrupted
slow-roll inflation. We find several fits, for which we calculate the expected
correlated signal in the primordial bispe...
We study the realization of cosmic inflation in bigravity theories. By
analyzing the evolution of scalar, vector, and tensor perturbations in de
Sitter-like spacetimes, we find strong stability constraints on the class of
viable vacua offered by these theories. More specifically, the only stable de
Sitter vacua contain two nondecoupled gravitons (o...
We study the dynamics of two-field models of inflation characterized by a
hierarchy of masses between curvature and isocurvature modes. When the
hierarchy is large, a low energy effective field theory (EFT) exists in which
only curvature modes participate in the dynamics of perturbations. In this EFT
heavy fields continue to have a significant role...
We discuss and clarify the validity of effective single field theories of
inflation obtained by integrating out heavy degrees of freedom in the regime
where adiabatic perturbations propagate with a suppressed speed of sound. We
show by construction that it is indeed possible to have inflationary
backgrounds where the speed of sound remains suppress...