activity
20102026
most citedSpeeding up the universe using dust with pressure

130 citations · 1.6k across the 87 of their papers we have counts for

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23 papers · 1 filter

astro-ph.CO2026

No evidence for dynamical dark energy from the Combo correlation of GRBs

Marco Muccino, Massimo Della Valle, Luca Izzo +1

Recently, the Dark Energy Spectroscopic Instrument (DESI) collaboration has presented results indicating that dark energy may exhibit dynamical behavior. Calibrated gamma-ray burst…

astro-ph.CO2026

Tightening Cosmological Constraints Within and Beyond CDM Using Gamma-Ray Bursts Calibrated with Type Ia Supernovae

Wei Hong, Luca Izzo, Massimo Della Valle +3

Context. Gamma-ray bursts (GRBs) reach redshifts beyond Type Ia supernovae (SNe Ia) and can extend distance measurements into the early Universe, but their use as distance indicato…

astro-ph.CO2025★ 6 cited

Investigating the cosmic distance duality relation with gamma-ray bursts

Anna Chiara Alfano, Carlo Cafaro, Salvatore Capozziello +2

Deviations from the so-called {\it cosmic distance duality relation} may result from systematic errors in distance measurements or, more interestingly, hint at new physics. Further…

astro-ph.CO2025★ 1 cited

Exploring the cosmic microwave background dipole direction using gamma-ray bursts

Orlando Luongo, Marco Muccino, Francesco Sorrenti

We search for dipole variations in the Hubble constant using gamma-ray burst (GRB) data, as such anisotropies may shed light on the Hubble tension. We employ the most recent…

astro-ph.CO2025★ 7 cited

Addressing the tension through matter with pressure and no early dark energy

Youri Carloni, Orlando Luongo, Marco Muccino

We propose that the Hubble tension arises due to an unaccounted additional component, that behaves as \emph{matter with pressure}. We demonstrate that this fluid remains subdominan…

astro-ph.CO2024★ 3 cited

Characterizing the equivalence between dark energy and radiation using gamma-ray bursts

Orlando Luongo, Marco Muccino

Differently from the equivalence time between either matter and radiation or dark energy and matter, the equivalence between dark energy and radiation occurs between two subdominan…

astro-ph.CO2024★ 3 cited

Determining from distance sum rule combining gamma-ray bursts with observational Hubble data and strong gravitational lensing

Orlando Luongo, Marco Muccino

Model-independent bounds on the Hubble constant are important to shed light on cosmological tensions. We work out a model-independent analysis based on the sum rule, which is…

astro-ph.CO2024★ 17 cited

Dark energy reconstructions combining BAO data with galaxy clusters and intermediate redshift catalogs

Orlando Luongo, Marco Muccino

Cosmological parameters and dark energy (DE) behavior are generally constrained assuming \textit{a priori} models. We work out a model-independent reconstruction to bound the key c…

astro-ph.CO2024★ 1 cited

Dark energy constraints using gamma-ray burst correlations with DESI 2024 data

Anna Chiara Alfano, Orlando Luongo, Marco Muccino

Even though the Dark Energy Spectroscopic Instrument (DESI) mission does not exclude a dynamical dark energy evolution, the concordance paradigm, i.e., the CDM model, remains st…

astro-ph.CO2024★ 2 cited

Cosmological constraints from calibrated gamma-ray burst correlation by using DESI 2024 data release

Anna Chiara Alfano, Orlando Luongo, Marco Muccino

Recent outcomes by the DESI Collaboration have shed light on a possible slightly evolving dark energy, challenging the standard CDM paradigm. To better understand dark energy na…

astro-ph.CO2024★ 6 cited

Does dark energy really revive using DESI 2024 data?

Youri Carloni, Orlando Luongo, Marco Muccino

We investigate the impact of the Dark Energy Spectroscopic Instrument (DESI) 2024 data on dark energy scenarios. We thus analyze three typologies of models, the first in which the…

astro-ph.CO2024★ 1 cited

Model independent cosmographic constraints from DESI 2024

Orlando Luongo, Marco Muccino

In this study, we explore model independent constraints on the universe kinematics up to the snap and jerk hierarchical terms. To do so, we consider the latest Baryon Acoustic Osci…

astro-ph.CO2024

Cosmological transition epoch from gamma-ray burst correlations

Anna Chiara Alfano, Salvatore Capozziello, Orlando Luongo +1

The redshift and the jerk parameter of the transition epoch are constrained by using two model-independent approaches involving the direct expansion of the Hubble rate…

astro-ph.CO2023★ 10 cited

Breaking the baryon-dark matter degeneracy in a model-independent way through the Sunyaev-Zeldovich effect

Anna Chiara Alfano, Orlando Luongo, Marco Muccino

We propose a model-independent \textit{Bézier parametric interpolation} to alleviate the degeneracy between baryonic and dark matter abundances by means of intermediate-redshift da…

astro-ph.CO2022★ 41 cited

Constraints on the transition redshift from the calibrated Gamma-ray Burst - correlation

Marco Muccino, Orlando Luongo, Deepak Jain

We constrain the deceleration-acceleration epoch, namely the transition redshift , adopting model-independent techniques that utilize a calibrated -…

astro-ph.CO2022

Intermediate redshift calibration of Gamma-ray Bursts and cosmic constraints in non-flat cosmology

Orlando Luongo, Marco Muccino

We propose how to calibrate long gamma-ray burst (GRB) correlations employing intermediate redshift data sets, instead of limiting to catalogs. To do so, we examine the…

astro-ph.CO2021★ 96 cited

On Larger Values in the CMB Dipole Direction

Orlando Luongo, Marco Muccino, Eoin Ó Colgáin +2

On the assumption that quasars (QSO) and gamma-ray bursts (GRB) represent \textit{standardisable candles}, we provide evidence that the Hubble constant adopts larger values i…

astro-ph.CO2021★ 92 cited

Do gamma-ray burst measurements provide a useful test of cosmological models?

Narayan Khadka, Orlando Luongo, Marco Muccino +1

We study eight different gamma-ray burst (GRB) data sets to examine whether current GRB measurements -- that probe a largely unexplored part of cosmological redshift () space --…

astro-ph.CO2021★ 25 cited

Testing generalized logotropic models with cosmic growth

Kuantay Boshkayev, Talgar Konysbayev, Orlando Luongo +2

We check the dynamical and observational features of four typologies of logotropic dark energy models, leading to a \emph{thermodynamic cosmic speed up} fueled by a single fluid th…

astro-ph.CO2020★ 51 cited

Tracing dark energy history with gamma ray bursts

M. Muccino, L. Izzo, O. Luongo +5

Observations of gamma-ray bursts up to are best suited to study the possible evolution of the Universe equation of state at intermediate redshifts. We apply the Combo-rel…

astro-ph.CO2020★ 60 cited

Model independent calibrations of gamma ray bursts using machine learning

Orlando Luongo, Marco Muccino

We alleviate the circularity problem, whereby gamma-ray bursts are not perfect distance indicators, by means of a new model-independent technique based on Bézier polynomials. To do…

astro-ph.CO2020★ 54 cited

Kinematic constraints beyond using calibrated GRB correlations

Orlando Luongo, Marco Muccino

The dynamics of the Universe are revised using high-redshift data from gamma-ray bursts to constrain cosmographic parameters by means of model-independent techniques. Considering s…

astro-ph.CO2015★ 68 cited

New measurements of from gamma-ray bursts

Luca Izzo, Marco Muccino, Elena Zaninoni +2

Context: Data from cosmic microwave background radiation (CMB), baryon acoustic oscillations (BAO), and supernovae Ia (SNe-Ia) support a constant dark energy equation of state with…