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20082026
most citedCosmology with the Laser Interferometer Space Antenna

359 citations · 3.2k across the 86 of their papers we have counts for

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Showing 2020Show all

6 papers · 1 filter

astro-ph.CO2020★ 19 cited

Machine Learning and cosmographic reconstructions of quintessence and the Swampland conjectures

Rubén Arjona, Savvas Nesseris

We present model independent reconstructions of quintessence and the Swampland conjectures (SC) using both Machine Learning (ML) and cosmography. In particular, we demonstrate how…

astro-ph.CO2020★ 10 cited

Cosmological constraints with the Effective Fluid approach for Modified Gravity

Wilmar Cardona, Rubén Arjona, Alejandro Estrada +1

Cosmological constraints of Modified Gravity (MG) models are seldom carried out rigorously. First, even though general MG models evolve differently (i.e., background and perturbati…

astro-ph.CO2020★ 32 cited

Machine learning forecasts of the cosmic distance duality relation with strongly lensed gravitational wave events

Rubén Arjona, Hai-Nan Lin, Savvas Nesseris +1

We use simulated strongly lensed gravitational wave events from the Einstein Telescope to demonstrate how the luminosity and angular diameter distances, and respe…

astro-ph.CO2020★ 1 cited

Is there any measurable redshift dependence on the SN Ia absolute magnitude?

Domenico Sapone, Savvas Nesseris, Carlos A. P. Bengaly

We test the cosmological implications of a varying absolute magnitude of Type Ia supernovae using the Pantheon compilation, by reconstructing different phenomenological approaches…

astro-ph.CO2020★ 60 cited

The clustering dynamics of primordial black boles in -body simulations

Manuel Trashorras, Juan García-Bellido, Savvas Nesseris

We explore the possibility that Dark Matter (DM) may be explained by a non-uniform background of approximately stellar-mass clusters of Primordial Black Holes (PBHs), by simulating…

astro-ph.CO2020★ 25 cited

Cosmological constraints on non-adiabatic dark energy perturbations

Rubén Arjona, Juan García-Bellido, Savvas Nesseris

The exact nature of dark energy is currently unknown and its cosmological perturbations, when dark energy is assumed not to be the cosmological constant, are usually modeled as adi…