A. Melchiorri
Researcher Next ID · RN-030273
Researcher · Physics and Astronomy
Istituto Nazionale di Fisica Nucleare, Sezione di Roma I
Rome, Italy
- Works count
- 589
- Citation count
- 104,407
- H-index
- 130
- i10-index
- 399
Research interests
Publications
The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics
Physics of the Dark Universe · 2025 · 10.1016/j.dark.2025.101965
Unfinished fabric of the three neutrino paradigm
Physical review. D/Physical review. D. · 2021 · 10.1103/physrevd.104.083031
Snowmass2021 - Letter of interest cosmology intertwined II: The hubble constant tension
Astroparticle Physics · 2021 · https://doi.org/10.1016/j.astropartphys.2021.102605
Cosmology intertwined III: f σ 8 and S 8
Astroparticle Physics · 2021 · 10.1016/j.astropartphys.2021.102604
Nonminimal dark sector physics and cosmological tensions
Physical review. D/Physical review. D. · 2020 · 10.1103/physrevd.101.063502
Planck 2018 results
Astronomy and Astrophysics · 2019 · https://doi.org/10.1051/0004-6361/201832618
Global constraints on absolute neutrino masses and their ordering
Physical review. D/Physical review. D. · 2017 · 10.1103/physrevd.95.096014
Can interacting dark energy solve the H0 tension?
Physical review. D/Physical review. D. · 2017 · 10.1103/physrevd.96.043503
Reconciling Planck with the local value of H 0 in extended parameter space
Physics Letters B · 2016 · 10.1016/j.physletb.2016.08.043
PRISM (Polarized Radiation Imaging and Spectroscopy Mission): an extended white paper
Journal of Cosmology and Astroparticle Physics · 2014 · https://doi.org/10.1088/1475-7516/2014/02/006
Indications of a Late-Time Interaction in the Dark Sector
Physical Review Letters · 2014 · 10.1103/physrevlett.113.181301
Probing Inflation with CMB Polarization
AIP conference proceedings · 2009 · 10.1063/1.3160885
CMB constraints on dark matter models with large annihilation cross section
Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · 2009 · 10.1103/physrevd.80.023505
CMBPol Mission Concept Study: Probing Inflation with CMB Polarization
Digital Access to Scholarship at Harvard (DASH) (Harvard University) · 2008 · 10.48550/arxiv.0811.3919
Large scale structure as a probe of gravitational slip
Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · 2008 · 10.1103/physrevd.77.103513
Cosmic microwave weak lensing data as a test for the dark universe
Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · 2008 · 10.1103/physrevd.77.123531
A Measurement of the CMB 〈EE〉 Spectrum from the 2003 Flight of BOOMERANG
The Astrophysical Journal · 2006 · 10.1086/505560
A Measurement of the Angular Power Spectrum of the CMB Temperature Anisotropy from the 2003 Flight of BOOMERANG
The Astrophysical Journal · 2006 · 10.1086/505559
The state of the dark energy equation of state
Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · 2003 · 10.1103/physrevd.68.043509
Cosmic structure formation with topological defects
Physics Reports · 2002 · 10.1016/s0370-1573(02)00014-5
Multiple Peaks in the Angular Power Spectrum of the Cosmic Microwave Background: Significance and Consequences for Cosmology
The Astrophysical Journal · 2002 · 10.1086/324298
Cosmological parameters from the first results of Boomerang
Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · 2001 · 10.1103/physrevd.63.042001
Cosmology from MAXIMA-1, BOOMERANG, and COBE DMR Cosmic Microwave Background Observations
Physical Review Letters · 2001 · 10.1103/physrevlett.86.3475
A Measurement of Ω from the North American Test Flight of Boomerang
The Astrophysical Journal · 2000 · https://doi.org/10.1086/312744
A Flat Universe from High-Resolution Maps of the Cosmic Microwave Background \nRadiation
eScholarship (California Digital Library) · 2000
Current projects
No projects listed.