output
19922026
most citedObservation of Gravitational Waves from a Binary Black Hole Merger

14.2k citations

Showing 2021 · astro-ph.COShow all

37 papers · 2 filters

astro-ph.CO2021★ 70 cited

Gravitational waves from dark matter isocurvature

Guillem Domènech, Samuel Passaglia, Sébastien Renaux-Petel

The primordial fluctuations on large scales are adiabatic, but on smaller scales this need not be the case. Here we derive the general analytical framework to compute the stochasti…

astro-ph.CO2021★ 12 cited

Euclid: Covariance of weak lensing pseudo- estimates. Calculation, comparison to simulations, and dependence on survey geometry

R. E. Upham, M. L. Brown, L. Whittaker +102

An accurate covariance matrix is essential for obtaining reliable cosmological results when using a Gaussian likelihood. In this paper we study the covariance of pseudo- es…

astro-ph.CO2021

Gravitational background from dynamical binaries and detectability with 2G detectors

Carole Périgois, Filippo Santoliquido, Yann Bouffanais +5

We study the impact of young clusters on the gravitational wave background from compact binary coalescence. We simulate a catalog of sources from population I/II isolated binary st…

astro-ph.CO2021★ 9 cited

Were recently reported MHz events planet mass primordial black hole mergers?

Guillem Domènech

A bulk acoustic wave cavity as high frequency gravitational wave antenna has recently detected two rare events at MHz. Assuming that the detected events are due to gravitation…

astro-ph.CO2021★ 247 cited

Constraints on the cosmic expansion history from GWTC-3

The LIGO Scientific Collaboration, the Virgo Collaboration, the KAGRA Collaboration +1676

We use 47 gravitational-wave sources from the Third LIGO-Virgo-KAGRA Gravitational-Wave Transient Catalog (GWTC-3) to estimate the Hubble parameter , including its current va…

astro-ph.CO2021★ 22 cited

In-flight polarization angle calibration for LiteBIRD: blind challenge and cosmological implications

Nicoletta Krachmalnicoff, Tomotake Matsumura, Elena de la Hoz +67

We present a demonstration of the in-flight polarization angle calibration for the JAXA/ISAS second strategic large class mission, LiteBIRD, and estimate its impact on the measurem…

astro-ph.CO2021★ 15 cited

The RayGalGroupSims cosmological simulation suite for the study of relativistic effects: an application to lensing-matter clustering statistics

Y. Rasera, M-A. Breton, P-S. Corasaniti +8

General Relativistic effects on the clustering of matter in the universe provide a sensitive probe of cosmology and gravity theories that can be tested with the upcoming generation…

astro-ph.CO2021

Signatures of Primordial Gravitational Waves on the Large-Scale Structure of the Universe

Pritha Bari, Angelo Ricciardone, Nicola Bartolo +2

We study the generation and evolution of second-order energy-density perturbations arising from primordial gravitational waves. Such "tensor-induced scalar modes" approximately evo…

astro-ph.CO2021★ 3 cited

Breaking the Single Clock Symmetry: measuring single-field inflation non-Gaussian features

Daniele Bertacca, Raul Jimenez, Sabino Matarrese +1

The Universe is not just cold dark matter and dark energy, it also contains baryons, radiation and neutrinos. The presence of these components, beyond the pressure-less cold dark m…

astro-ph.CO2021★ 39 cited

Expansion history-dependent oscillations in the scalar-induced gravitational wave background

Lukas T. Witkowski, Guillem Domènech, Jacopo Fumagalli +1

Oscillations in the frequency profile of the scalar-induced contribution to the stochastic gravitational wave background are a characteristic signal for small-scale features during…

astro-ph.CO2021★ 10 cited

Leverage on small-scale primordial non-Gaussianity through cross-correlations between CMB -mode and -distortion anisotropies

Mathieu Remazeilles, Andrea Ravenni, Jens Chluba

Multi-field inflation models and non-Bunch-Davies vacuum initial conditions both predict sizeable non-Gaussian primordial perturbations and anisotropic -type spectral distortion…

astro-ph.CO2021★ 29 cited

Euclid: Forecast constraints on consistency tests of the CDM model

S. Nesseris, D. Sapone, M. Martinelli +112

The standard cosmological model is based on the fundamental assumptions of a spatially homogeneous and isotropic universe on large scales. An observational detection of a violation…

astro-ph.CO2021★ 47 cited

KiDS & Euclid: Cosmological implications of a pseudo angular power spectrum analysis of KiDS-1000 cosmic shear tomography

A. Loureiro, L. Whittaker, A. Spurio Mancini +111

We present a tomographic weak lensing analysis of the Kilo Degree Survey Data Release 4 (KiDS-1000), using a new pseudo angular power spectrum estimator (pseudo-) under d…

astro-ph.CO2021★ 56 cited

Euclid preparation: XIX. Impact of magnification on photometric galaxy clustering

F. Lepori, I. Tutusaus, C. Viglione +183

We investigate the importance of lensing magnification for estimates of galaxy clustering and its cross-correlation with shear for the photometric sample of Euclid. Using updated s…

astro-ph.CO2021★ 22 cited

The paradigm of warm quintessential inflation and spontaneous baryogenesis

Soumen Basak, Sukannya Bhattacharya, Mayukh R. Gangopadhyay +3

In this paper, we consider a scenario of spontaneous baryogenesis in a framework of warm quintessential inflation where the residual inflaton field, left out after warm inflation,…

astro-ph.CO2021★ 70 cited

Search for subsolar-mass binaries in the first half of Advanced LIGO and Virgo's third observing run

The LIGO Scientific Collaboration, the Virgo Collaboration, the KAGRA Collaboration +1634

We report on a search for compact binary coalescences where at least one binary component has a mass between 0.2 and 1.0 in Advanced LIGO and Advanced Virgo dat…

astro-ph.CO2021★ 21 cited

Clustering of Gravitational Wave and Supernovae events: a multitracer analysis in Luminosity Distance Space

Sarah Libanore, Maria Celeste Artale, Dionysios Karagiannis +5

We study the clustering of Gravitational Wave (GW) merger events and Supernovae IA (SN), as cosmic tracers in Luminosity Distance Space. We modify the publicly available CAMB code…

astro-ph.CO2021★ 2 cited

Euclid: Constraining ensemble photometric redshift distributions with stacked spectroscopy

M. S. Cagliari, B. R. Granett, L. Guzzo +109

The ESA Euclid mission will produce photometric galaxy samples over 15000 square degrees of the sky that will be rich for clustering and weak lensing statistics. The accuracy of th…

astro-ph.CO2021★ 1 cited

The large-scale monopole of the power spectrum in a Euclid-like survey: wide-angle effects, lensing, and the `finger of the observer'

Mohamed Yousry Elkhashab, Cristiano Porciani, Daniele Bertacca

Radial redshift-space distortions due to peculiar velocities and other light-cone effects shape the maps we build of the Universe. We address the open question of their impact onto…

astro-ph.CO2021★ 68 cited

Euclid: Forecasts from redshift-space distortions and the Alcock-Paczynski test with cosmic voids

N. Hamaus, M. Aubert, A. Pisani +127

Euclid is poised to survey galaxies across a cosmological volume of unprecedented size, providing observations of more than a billion objects distributed over a third of the full s…

astro-ph.CO2021★ 72 cited

SKAO HI Intensity Mapping: Blind Foreground Subtraction Challenge

Marta Spinelli, Isabella P. Carucci, Steven Cunnington +5

Neutral Hydrogen Intensity Mapping (HI IM) surveys will be a powerful new probe of cosmology. However, strong astrophysical foregrounds contaminate the signal and their coupling wi…

astro-ph.CO2021

The Kaiser-Rocket effect: three decades and counting

Benedict Bahr-Kalus, Daniele Bertacca, Licia Verde +1

The peculiar motion of the observer, if not accurately accounted for, is bound to induce a well-defined clustering signal in the distribution of galaxies. This signal is related to…

astro-ph.CO2021★ 2 cited

Euclid Preparation: XIV. The Complete Calibration of the Color-Redshift Relation (C3R2) Survey: Data Release 3

Euclid Collaboration, S. A. Stanford, D. Masters +183

The Complete Calibration of the Color-Redshift Relation (C3R2) survey is obtaining spectroscopic redshifts in order to map the relation between galaxy color and redshift to a depth…

astro-ph.CO2021★ 33 cited

Gravitational waves HI intensity mapping: cosmological and astrophysical applications

Giulio Scelfo, Marta Spinelli, Alvise Raccanelli +3

Two of the most rapidly growing observables in cosmology and astrophysics are gravitational waves (GW) and the neutral hydrogen (HI) distribution. In this work, we investigate the…