Search Publications

Cosmic microwave background limits on accreting primordial black holes
DOI: 10.1103/PhysRevD.95.043534 Bibcode: 2017PhRvD..95d3534A

Kamionkowski, Marc; Ali-Haïmoud, Yacine

Interest in the idea that primordial black holes (PBHs) might comprise some or all of the dark matter has recently been rekindled following LIGO's first direct detection of a binary-black-hole merger. Here we revisit the effect of accreting PBHs on the cosmic microwave background (CMB) frequency spectrum and the angular temperature and polarizatio…

2017 Physical Review D
Planck 427
Can interacting dark energy solve the H0 tension?
DOI: 10.1103/PhysRevD.96.043503 Bibcode: 2017PhRvD..96d3503D

Di Valentino, Eleonora; Melchiorri, Alessandro; Mena, Olga

The answer is yes. We indeed find that interacting dark energy can alleviate the current tension on the value of the Hubble constant H0 between the cosmic microwave background anisotropies constraints obtained from the Planck satellite and the recent direct measurements reported by Riess et al. 2016. The combination of these two data se…

2017 Physical Review D
Planck 383
Unveiling ν secrets with cosmological data: Neutrino masses and mass hierarchy
DOI: 10.1103/PhysRevD.96.123503 Bibcode: 2017PhRvD..96l3503V

Ho, Shirley; Mena, Olga; Gerbino, Martina +4 more

Using some of the latest cosmological data sets publicly available, we derive the strongest bounds in the literature on the sum of the three active neutrino masses, Mν, within the assumption of a background flat Λ CDM cosmology. In the most conservative scheme, combining Planck cosmic microwave background temperature anisotropies and ba…

2017 Physical Review D
Planck 364
Global constraints on absolute neutrino masses and their ordering
DOI: 10.1103/PhysRevD.95.096014 Bibcode: 2017PhRvD..95i6014C

Di Valentino, Eleonora; Melchiorri, Alessandro; Capozzi, Francesco +3 more

Within the standard three-neutrino framework, the absolute neutrino masses and their ordering (either normal, NO, or inverted, IO) are currently unknown. However, the combination of current data coming from oscillation experiments, neutrinoless double beta (0 ν β β ) decay searches, and cosmological surveys, can provide interesting constraints for…

2017 Physical Review D
Planck 285
CMB bounds on disk-accreting massive primordial black holes
DOI: 10.1103/PhysRevD.96.083524 Bibcode: 2017PhRvD..96h3524P

Calore, Francesca; Kohri, Kazunori; Poulin, Vivian +2 more

Stellar-mass primordial black holes (PBH) have been recently reconsidered as a dark matter (DM) candidate after the aLIGO discovery of several binary black hole (BH) mergers with masses of tens of M . Matter accretion on such massive objects leads to the emission of high-energy photons, capable of altering the ionization and thermal hi…

2017 Physical Review D
Planck 244
General constraints on dark matter decay from the cosmic microwave background
DOI: 10.1103/PhysRevD.95.023010 Bibcode: 2017PhRvD..95b3010S

Slatyer, Tracy R.; Wu, Chih-Liang

Precise measurements of the temperature and polarization anisotropies of the cosmic microwave background can be used to constrain the annihilation and decay of dark matter. In this work, we demonstrate via principal component analysis that the imprint of dark matter decay on the cosmic microwave background can be approximately parametrized by a si…

2017 Physical Review D
Planck 229
Echo of interactions in the dark sector
DOI: 10.1103/PhysRevD.96.103511 Bibcode: 2017PhRvD..96j3511K

Nunes, Rafael C.; Kumar, Suresh

We investigate the observational constraints on an interacting vacuum energy scenario with two different neutrino schemes (with and without a sterile neutrino) using the most recent data from cosmic microwave background (CMB) temperature and polarization anisotropy, baryon acoustic oscillations (BAO), type Ia supernovae from JLA sample and structu…

2017 Physical Review D
Planck 217
Constraining dark energy dynamics in extended parameter space
DOI: 10.1103/PhysRevD.96.023523 Bibcode: 2017PhRvD..96b3523D

Di Valentino, Eleonora; Melchiorri, Alessandro; Silk, Joseph +1 more

Dynamical dark energy has been recently suggested as a promising and physical way to solve the 3 sigma tension on the value of the Hubble constant H0 between the direct measurement of Riess et al. (2016) (R16, hereafter) and the indirect constraint from cosmic microwave anisotropies obtained by the Planck satellite under the assumption …

2017 Physical Review D
Planck 192
Two-season Atacama Cosmology Telescope polarimeter lensing power spectrum
DOI: 10.1103/PhysRevD.95.123529 Bibcode: 2017PhRvD..95l3529S

Hasselfield, Matthew; Battaglia, Nicholas; Aiola, Simone +43 more

We report a measurement of the power spectrum of cosmic microwave background (CMB) lensing from two seasons of Atacama Cosmology Telescope polarimeter (ACTPol) CMB data. The CMB lensing power spectrum is extracted from both temperature and polarization data using quadratic estimators. We obtain results that are consistent with the expectation from…

2017 Physical Review D
Planck 126
Evidence for interacting dark energy from BOSS
DOI: 10.1103/PhysRevD.95.043520 Bibcode: 2017PhRvD..95d3520F

Ferreira, Elisa G. M.; Quintin, Jerome; Costa, André A. +2 more

The result presented by the BOSS-SDSS Collaboration measuring the baryon acoustic oscillations of the Lyman-alpha forest from high-redshift quasars indicates a 2.5 σ departure from the standard Λ -cold-dark-matter model. This is the first time that the evolution of dark energy at high redshifts has been measured, and the current results cannot be …

2017 Physical Review D
Planck 121