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20022026
most citedThe Herschel ATLAS

596 citations · 7.4k across the 241 of their papers we have counts for

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Showing 2023 · astro-ph.COShow all

6 papers · 2 filters

astro-ph.CO2023

Dark Matter in Fractional Gravity III: Dwarf Galaxies Kinematics

F. Benetti, A. Lapi, G. Gandolfi +4

Recently we put forward a framework where the dark matter (DM) component within virialized halos is subject to a non-local interaction originated by fractional gravity (FG) effects…

astro-ph.CO2023★ 1 cited

Little Ado about Everything: CDM, a Cosmological Model with Fluctuation-driven Acceleration at Late Times

Andrea Lapi, Lumen Boco, Marcos M. Cueli +4

[abridged] We propose a model of the Universe (dubbed CDM) featuring a stochastic evolution of the cosmological quantities, that is meant to render small deviations from homogen…

astro-ph.CO2023

Dark Matter in Fractional Gravity II: Tests in Galaxy Clusters

Francesco Benetti, Andrea Lapi, Giovanni Gandolfi +2

[abridged] Recently, in Benetti et al. (Astrophys. J. 2023, 949, 65), we suggested that the dark matter (DM) component in galaxies may originate fractional gravity. In such a frame…

astro-ph.CO2023★ 12 cited

Looking for Traces of Non-minimally Coupled Dark Matter in the X-COP Galaxy Clusters Sample

Giovanni Gandolfi, Balakrishna Sandeep Haridasu, Stefano Liberati +1

We look for possible evidence of a non-minimal coupling (NMC) between dark matter (DM) and gravity using data from the X-COP compilation of galaxy clusters. We consider a theoretic…

astro-ph.CO2023★ 1 cited

Methodological refinement of the submillimeter galaxy magnification bias. I. Cosmological analysis with a single redshift bin

Marcos M. Cueli, Joaquín González-Nuevo, Laura Bonavera +3

The main goal of this work, the second in a three-paper series, is to test the impact of a methodological improvement in measuring the magnification bias signal on a sample of subm…

astro-ph.CO2023★ 12 cited

Constraining Chameleon screening using galaxy cluster dynamics

Yacer Boumechta, Balakrishna S. Haridasu, Lorenzo Pizzuti +3

We constrain the Chameleon \textit{screening} mechanism in galaxy clusters, essentially obtaining limits on the coupling strength and the asymptotic value of the field $ϕ_{\inf…