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20032026
most citedProspects for Fundamental Physics with LISA

401 citations · 2.9k across the 56 of their papers we have counts for

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26 papers · 1 filter

astro-ph.CO2026

Slowly Rolling on a Quantum Correction

Ido Ben-Dayan, Ayushi Srivastava, Amresh Verma

Recent advances in cosmological measurements such as DESI and ACT may indicate an increase in the preferred value of the spectral tilt such that it disfavors rather popular m…

astro-ph.CO2025

Disentangling the Origins of the NANOGrav Signal: Early Universe Models and Bounds

Ido Ben-Dayan, Utkarsh Kumar, Amresh Verma

We investigate whether an Early-Universe stochastic gravitational-wave background (SGWB) can account for the common spectrum process reported by NANOGrav, while also being consiste…

astro-ph.CO2025★ 299 cited

The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics

Eleonora Di Valentino, Jackson Levi Said, Adam Riess +533

The standard model of cosmology has provided a good phenomenological description of a wide range of observations both at astrophysical and cosmological scales for several decades.…

astro-ph.CO2024★ 6 cited

Impact of Low ell's on Large Scale Structure Anomalies

Ido Ben-Dayan, Utkarsh Kumar, Meir Shimon +1

We scrutinize the reported lensing anomaly of the CMB by considering several phenomenological modifications of the lensing consistency parameter, . Considering Planck sp…

astro-ph.CO2023

Theoretical Priors and the Dark Energy Equation of State

Ido Ben-Dayan, Utkarsh Kumar

We revisit the theoretical priors used for inferring Dark Energy (DE) parameters. Any DE model must have some form of a tracker mechanism such that it behaved as matter or radiatio…

astro-ph.CO2023

Requiem to "Proof of Inflation" or Sourced Fluctuations in a Non-Singular Bounce

Ido Ben-Dayan, Udaykrishna Thattarampilly

Popular wisdom suggests that measuring the tensor to scalar ratio on CMB scales is a "proof of inflation" since one generic prediction is a scale-invariant tensor spectrum whil…

astro-ph.CO2023★ 41 cited

Probing The Early Universe Cosmology With NANOGrav: Possibilities and Limitations

Ido Ben-Dayan, Utkarsh Kumar, Udaykrishna Thattarampilly +1

A stochastic gravitational wave background is a prediction of a number of astrophysical and cosmological phenomena including early Universe Cosmology. Recently, the NANOGrav Collab…

astro-ph.CO2023

Emergent Unparticles Dark Energy can restore cosmological concordance

Ido Ben-Dayan, Utkarsh Kumar

Addressing the discrepancy between the late and early time measurements of the Hubble parameter, , and the so-called parameter has been a challenge in precision cosmolog…

astro-ph.CO2022

Small Field models with ACTPol and BICEP3 data -- Likelihood analysis

Ira Wolfson, Utkarsh Kumar, Ido Ben-Dayan +1

We perform a Bayesian analysis for small field models of inflation, using the most recent datasets produced by Planck`18, ACTPol, and BICEP3. We employ Artificial Neural Networks (…

astro-ph.CO2022★ 359 cited

Cosmology with the Laser Interferometer Space Antenna

Pierre Auclair, David Bacon, Tessa Baker +177

The Laser Interferometer Space Antenna (LISA) has two scientific objectives of cosmological focus: to probe the expansion rate of the universe, and to understand stochastic gravita…

astro-ph.CO2021★ 7 cited

More on Emergent Dark Energy from Unparticles

Michał Artymowski, Ido Ben-Dayan, Utkarsh Kumar

In a recent paper \cite{Artymowski:2020zwy} we suggested the possibility that the present acceleration of the Universe is due to thermodynamical behavior of unparticles. The model…

astro-ph.CO2019★ 1 cited

Spectral Distortions of the CMB as a Probe of Inflation, Recombination, Structure Formation and Particle Physics

J. Chluba, A. Kogut, S. P. Patil +98

Following the pioneering observations with COBE in the early 1990s, studies of the cosmic microwave background (CMB) have focused on temperature and polarization anisotropies. CMB…

astro-ph.CO2019★ 54 cited

Constraints on Scalar and Tensor spectra from

Ido Ben-Dayan, Brian Keating, David Leon +1

At the linear level, the gravitational wave (GW) spectrum predicted by inflation, and many of its alternatives, can have arbitrarily small amplitude and consequently an unconstrain…

astro-ph.CO2016★ 32 cited

Gravitational Waves in Bouncing Cosmologies from Gauge Field Production

Ido Ben-Dayan

We calculate the gravitational waves (GW) spectrum produced in various Early Universe scenarios from gauge field sources, thus generalizing earlier inflationary calculations to bou…

astro-ph.CO2015★ 14 cited

Constraints on small-scale cosmological fluctuations from SNe lensing dispersion

Ido Ben-Dayan, Ryuichi Takahashi

We provide predictions on small-scale cosmological density power spectrum from supernova lensing dispersion. Parameterizing the primordial power spectrum with running and runni…

astro-ph.CO2014★ 16 cited

On Soft Limits of Large-Scale Structure Correlation Functions

Ido Ben-Dayan, Thomas Konstandin, Rafael A. Porto +1

We study soft limits of correlation functions for the density and velocity fields in the theory of structure formation. First, we re-derive the (resummed) consistency conditions at…

astro-ph.CO2014★ 4 cited

Lensing dispersion of SNIa and small scales of the primordial power spectrum

Ido Ben-Dayan

Probing the primordial power spectrum at small scales is crucial for discerning inflationary models, especially if BICEP2 results are confirmed. We demonstrate this necessity by br…

astro-ph.CO2014★ 105 cited

The value of H_0 in the inhomogeneous Universe

Ido Ben-Dayan, Ruth Durrer, Giovanni Marozzi +1

Local measurements of the Hubble expansion rate are affected by structures like galaxy clusters or voids. Here we present a fully relativistic treatment of this effect, studying ho…

astro-ph.CO2013★ 18 cited

Constraining the primordial power spectrum from SNIa lensing dispersion

Ido Ben-Dayan, Tigran Kalaydzhyan

The (absence of detecting) lensing dispersion of Supernovae type Ia (SNIa) can be used as a novel and extremely efficient probe of cosmology. In this preliminary example we analyze…

astro-ph.CO2013★ 83 cited

Average and dispersion of the luminosity-redshift relation in the concordance model

I. Ben-Dayan, M. Gasperini, G. Marozzi +2

Starting from the luminosity-redshift relation recently given up to second order in the Poisson gauge, we calculate the effects of the realistic stochastic background of perturbati…

astro-ph.CO2012★ 75 cited

The second-order luminosity-redshift relation in a generic inhomogeneous cosmology

Ido Ben-Dayan, Giovanni Marozzi, Fabien Nugier +1

After recalling a general non-perturbative expression for the luminosity-redshift relation holding in a recently proposed "geodesic light-cone" gauge, we show how it can be transfo…

astro-ph.CO2012★ 100 cited

Do stochastic inhomogeneities affect dark-energy precision measurements?

Ido Ben-Dayan, Maurizio Gasperini, Giovanni Marozzi +2

The effect of a stochastic background of cosmological perturbations on the luminosity-redshift relation is computed to second order through a recently proposed covariant and gauge-…

astro-ph.CO2012★ 62 cited

Backreaction on the luminosity-redshift relation from gauge invariant light-cone averaging

Ido Ben-Dayan, Maurizio Gasperini, Giovanni Marozzi +2

Using a recently proposed gauge invariant formulation of light-cone averaging, together with adapted "geodesic light-cone" coordinates, we show how an "induced backreaction" effect…

astro-ph.CO2012★ 289 cited

Probing the inflaton: Small-scale power spectrum constraints from measurements of the CMB energy spectrum

Jens Chluba, Adrienne L. Erickcek, Ido Ben-Dayan

In the early Universe, energy stored in small-scale density perturbations is quickly dissipated by Silk-damping, a process that inevitably generates mu- and y-type spectral distort…