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From the 1 of 19 linked papers with an AI index.

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20242026
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19 papers

gr-qc2026

Cosmological consequences of scale-dependent Barrow-Tsallis entropy

Giuseppe Gaetano Luciano, Orlando Luongo, Marco Muccino

The paper explores a cosmological model with a scale‑dependent Barrow‑Tsallis entropy, deriving modified Friedmann equations and confronting the model with various early‑ and late‑…

gr-qc2026

The macroscopic precession model of quasi-periodic oscillations for rotating compact objects

Orlando Luongo, Marco Muccino

The relativistic precession model (RPM) interprets the twin kilohertz quasi-periodic oscillations (QPOs) as geodesic frequencies of test particles orbiting in the spacetime of X-ra…

astro-ph.GA2026

Testing dark matter density profiles based on Padé approximants of different orders

Talgar Konysbayev, Orlando Luongo, Marco Muccino +5

We investigate whether low-order Padé rational functions can be used as empirical density profiles for modeling dark matter halos from galaxy RCs. We introduce three parameterizat…

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…

gr-qc2025

The macroscopic precession model: describing quasi-periodic oscillations including internal structures of test bodies

Gabriele Bianchini, Orlando Luongo, Marco Muccino

The relativistic precession model (RPM) is widely-considered as a benchmark framework to interpret quasi-periodic oscillations (QPOs), albeit several observational inconsistencies…