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20062022
most citedThe Cosmological Analysis of the SDSS/BOSS data from the Effective Field Theory of Large-Scale Structure

456 citations · 4.3k across the 59 of their papers we have counts for

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31 papers · 1 filter

astro-ph.CO2022★ 32 cited

The one-loop bispectrum of galaxies in redshift space from the Effective Field Theory of Large-Scale Structure

Guido D'Amico, Yaniv Donath, Matthew Lewandowski +2

We derive the kernels and the Effective Field Theory of Large-Scale Structure counterterms for the one-loop bispectrum of dark matter and of biased tracers in real and redshift spa…

astro-ph.CO2022★ 47 cited

Constraints on modified gravity from the BOSS galaxy survey

Lorenzo Piga, Marco Marinucci, Guido D'Amico +3

We develop a pipeline to set new constraints on scale-independent modified gravity, from the galaxy power spectrum in redshift space of BOSS DR12. The latter is modelled using the…

astro-ph.CO2022★ 78 cited

The BOSS bispectrum analysis at one loop from the Effective Field Theory of Large-Scale Structure

Guido D'Amico, Yaniv Donath, Matthew Lewandowski +2

We analyze the BOSS power spectrum monopole and quadrupole, and the bispectrum monopole and quadrupole data, using the predictions from the Effective Field Theory of Large-Scale St…

astro-ph.CO2022★ 37 cited

Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies

Elcio Abdalla, Guillermo Franco Abellán, Amin Aboubrahim +200

In this paper we will list a few important goals that need to be addressed in the next decade, also taking into account the current discordances between the different cosmological…

astro-ph.CO2022★ 45 cited

Limits on primordial non-Gaussianities from BOSS galaxy-clustering data

Guido D'Amico, Matthew Lewandowski, Leonardo Senatore +1

We analyze the power spectrum and the bispectrum of BOSS galaxy-clustering data using the prediction from the Effective Field Theory of Large-Scale Structure at one-loop order for…

astro-ph.CO2021★ 1 cited

The Large Scale Structure Bootstrap: perturbation theory and bias expansion from symmetries

Guido D'Amico, Marco Marinucci, Massimo Pietroni +1

We investigate the role played by symmetries in the perturbative expansion of the large-scale structure. In particular, we establish which of the coefficients of the perturbation t…

astro-ph.CO2021★ 97 cited

BOSS Correlation Function Analysis from the Effective Field Theory of Large-Scale Structure

Pierre Zhang, Guido D'Amico, Leonardo Senatore +2

After calibrating the predictions of the Effective Field Theory of Large-Scale Structure against several sets of simulations, as well as implementing a new method to assert the sca…

astro-ph.CO2021★ 27 cited

Taming redshift-space distortion effects in the EFTofLSS and its application to data

Guido D'Amico, Leonardo Senatore, Pierre Zhang +1

Former analyses of the BOSS data using the Effective Field Theory of Large-Scale Structure (EFTofLSS) have measured that the largest counterterms are the redshift-space distortion…

astro-ph.CO2020★ 29 cited

Limits on Clustering and Smooth Quintessence from the EFTofLSS

Guido D'Amico, Yaniv Donath, Leonardo Senatore +1

We apply the Effective Field Theory of Large-Scale Structure (EFTofLSS) to analyze cosmological models with clustering quintessence, which allows us to consistently describe the pa…

astro-ph.CO2020★ 143 cited

The Hubble Tension in Light of the Full-Shape Analysis of Large-Scale Structure Data

Guido D'Amico, Leonardo Senatore, Pierre Zhang +1

The disagreement between direct late-time measurements of the Hubble constant from the SH0ES collaboration, and early-universe measurements based on the CDM model from the Planc…

astro-ph.CO2020★ 171 cited

Blinded challenge for precision cosmology with large-scale structure: results from effective field theory for the redshift-space galaxy power spectrum

Takahiro Nishimichi, Guido D'Amico, Mikhail M. Ivanov +5

An accurate theoretical template for the galaxy power spectrum is a key for the success of ongoing and future spectroscopic surveys. We examine to what extent the Effective Field T…

astro-ph.CO2020★ 166 cited

Limits on CDM from the EFTofLSS with the PyBird code

Guido D'Amico, Leonardo Senatore, Pierre Zhang

We apply the Effective Field Theory of Large-Scale Structure to analyze the CDM cosmological model. By using the full shape of the power spectrum and the BAO post-reconstruction…

astro-ph.CO2019★ 170 cited

Efficient Cosmological Analysis of the SDSS/BOSS data from the Effective Field Theory of Large-Scale Structure

Thomas Colas, Guido D'Amico, Leonardo Senatore +2

The precision of the cosmological data allows us to accurately approximate the predictions for cosmological observables by Taylor expanding up to a low order the dependence on the…

astro-ph.CO2019★ 456 cited

The Cosmological Analysis of the SDSS/BOSS data from the Effective Field Theory of Large-Scale Structure

Guido D'Amico, Jérôme Gleyzes, Nickolas Kokron +5

The Effective Field Theory of Large-Scale Structure (EFTofLSS) is a formalism that allows us to predict the clustering of Cosmological Large-Scale Structure in the mildly non-linea…

astro-ph.CO2019★ 12 cited

Inflation and Dark Energy from spectroscopy at

Simone Ferraro, Michael J. Wilson, Muntazir Abidi +140

The expansion of the Universe is understood to have accelerated during two epochs: in its very first moments during a period of Inflation and much more recently, at , when D…

astro-ph.CO2019★ 54 cited

Primordial Non-Gaussianity

P. Daniel Meerburg, Daniel Green, Muntazir Abidi +175

Our current understanding of the Universe is established through the pristine measurements of structure in the cosmic microwave background (CMB) and the distribution and shapes of…

astro-ph.CO2019★ 45 cited

Messengers from the Early Universe: Cosmic Neutrinos and Other Light Relics

Daniel Green, Mustafa A. Amin, Joel Meyers +136

The hot dense environment of the early universe is known to have produced large numbers of baryons, photons, and neutrinos. These extreme conditions may have also produced other lo…

astro-ph.CO2019★ 3 cited

Dark Matter Science in the Era of LSST

Keith Bechtol, Alex Drlica-Wagner, Kevork N. Abazajian +177

Astrophysical observations currently provide the only robust, empirical measurements of dark matter. In the coming decade, astrophysical observations will guide other experimental…

astro-ph.CO2018★ 21 cited

Black hole formation in the context of dissipative dark matter

M. A. Latif, A. Lupi, D. R. G. Schleicher +3

Black holes with masses of dwell in the centers of most galaxies, but their formation mechanisms are not well known. A subdominant dissipative component o…

astro-ph.CO2018★ 113 cited

Bounds on Dark Matter annihilations from 21 cm data

Guido D'Amico, Paolo Panci, Alessandro Strumia

The observation of an absorption feature in the 21 cm spectrum at redshift implies bounds on Dark Matter annihilations for a broad range of masses, given that signifi…

astro-ph.CO2017★ 51 cited

Massive Black Holes from Dissipative Dark Matter

Guido D'Amico, Paolo Panci, Alessandro Lupi +2

We show that a subdominant component of dissipative dark matter resembling the Standard Model can form many intermediate-mass black hole seeds during the first structure formation…

astro-ph.CO2016★ 45 cited

Weakening Gravity on Redshift-Survey Scales with Kinetic Matter Mixing

Guido D'Amico, Zhiqi Huang, Michele Mancarella +1

We explore general scalar-tensor models in the presence of a kinetic mixing between matter and the scalar field, which we call Kinetic Matter Mixing. In the frame where gravity is…

astro-ph.CO2015★ 9 cited

Anisotropies in Non-Thermal Distortions of Cosmic Light from Photon-Axion Conversion

Guido D'Amico, Nemanja Kaloper

Ultralight axions which couple sufficiently strongly to photons can leave imprints on the sky at diverse frequencies by mixing with cosmic light in the presence of background magne…

astro-ph.CO2014★ 8 cited

Non-Gaussianity after BICEP2

Guido D'Amico, Matthew Kleban

We analyze primordial non-Gaussianity in single field inflationary models when the tensor/scalar ratio is large. Our results show that detectable levels of non-Gaussianity $f_{NL}…