Cosmology intertwined: A review of the particle physics, astrophysics, and cosmology associated with the cosmological tensions and anomalies
Abstract The standard Λ Cold Dark Matter (ΛCDM) cosmological model provides a good
description of a wide range of astrophysical and cosmological data. However, there are a …
description of a wide range of astrophysical and cosmological data. However, there are a …
On the Hubble constant tension in the SNe Ia Pantheon sample
MG Dainotti, B De Simone, T Schiavone… - The Astrophysical …, 2021 - iopscience.iop.org
On the Hubble Constant Tension in the SNe Ia Pantheon Sample - IOPscience This site uses
cookies. By continuing to use this site you agree to our use of cookies. To find out more, see …
cookies. By continuing to use this site you agree to our use of cookies. To find out more, see …
The Hubble constant tension: current status and future perspectives through new cosmological probes
M Dainotti, B De Simone, G Montani… - arxiv preprint arxiv …, 2023 - arxiv.org
The Hubble constant ($ H_0 $) tension is one of the major open problems in modern
cosmology. This tension is the discrepancy, ranging from 4 to 6$\sigma $, between the …
cosmology. This tension is the discrepancy, ranging from 4 to 6$\sigma $, between the …
On the evolution of the Hubble constant with the SNe Ia pantheon sample and baryon acoustic oscillations: a feasibility study for GRB-cosmology in 2030
MG Dainotti, B De Simone, T Schiavone, G Montani… - Galaxies, 2022 - mdpi.com
The difference from 4 to 6 σ in the Hubble constant (H 0) between the values observed with
the local (Cepheids and Supernovae Ia, SNe Ia) and the high-z probes (Cosmic Microwave …
the local (Cepheids and Supernovae Ia, SNe Ia) and the high-z probes (Cosmic Microwave …
Gamma-ray bursts, quasars, baryonic acoustic oscillations, and supernovae Ia: new statistical insights and cosmological constraints
The recent Hubble constant, H 0, tension is observed between the value of H 0 from the
cosmic microwave background (CMB) and Type Ia supernovae (SNe Ia). It is a decade since …
cosmic microwave background (CMB) and Type Ia supernovae (SNe Ia). It is a decade since …
Tensions with the flat ΛCDM model from high-redshift cosmography
G Bargiacchi, MG Dainotti… - Monthly Notices of the …, 2023 - academic.oup.com
The longstanding search for the cosmological model that best describes the Universe has
been made more intriguing since the recent discovery of the Hubble constant, H 0, tension …
been made more intriguing since the recent discovery of the Hubble constant, H 0, tension …
Using lower redshift, non-CMB, data to constrain the Hubble constant and other cosmological parameters
We use updated Hubble parameter and baryon acoustic oscillation data, as well as other
lower redshift Type Ia supernova, Mg ii reverberation-measured quasar, quasar angular …
lower redshift Type Ia supernova, Mg ii reverberation-measured quasar, quasar angular …
Optical and X-ray GRB Fundamental Planes as cosmological distance indicators
ABSTRACT Gamma-ray bursts (GRBs), can be employed as standardized candles,
extending the distance ladder beyond Type Ia supernovae (SNe Ia, z= 2.26). We …
extending the distance ladder beyond Type Ia supernovae (SNe Ia, z= 2.26). We …
The THESEUS space mission concept: science case, design and expected performances
THESEUS is a space mission concept aimed at exploiting Gamma-Ray Bursts for
investigating the early Universe and at providing a substantial advancement of multi …
investigating the early Universe and at providing a substantial advancement of multi …
Standardizing Platinum Dainotti-correlated gamma-ray bursts, and using them with standardized Amati-correlated gamma-ray bursts to constrain cosmological model …
We show that the Platinum gamma-ray burst (GRB) data compilation, probing the redshift
range 0.553≤ z≤ 5.0, obeys a cosmological-model-independent three-parameter …
range 0.553≤ z≤ 5.0, obeys a cosmological-model-independent three-parameter …