TY  - JOUR
AU  - Archidiacono, M.
AU  - Giusarma, E.
AU  - Melchiorri, A.
AU  - Mena, O.
PY  - 2013
DA  - 2013//
TI  - Neutrino and dark radiation properties in light of recent CMB observations
T2  - Phys. Rev. D
JO  - Physical Review D
SP  - 103519
EP  - 10pp
VL  - 87
IS  - 10
PB  - Amer Physical Soc
AB  - Recent cosmic microwave background measurements at high multipoles from the South Pole Telescope and from the Atacama Cosmology Telescope seem to disagree in their conclusions for the neutrino and dark radiation properties. In this paper we set new bounds on the dark radiation and neutrino properties in different cosmological scenarios combining the ACT and SPT data with the nine-year data release of the Wilkinson Microwave Anisotropy Probe (WMAP-9), baryon acoustic oscillation data, Hubble Telescope measurements of the Hubble constant, and supernovae Ia luminosity distance data. In the standard three massive neutrino case, the two high multipole probes give similar results if baryon acoustic oscillation data are removed from the analyses and Hubble Telescope measurements are also exploited. A similar result is obtained within a standard cosmology with N-eff massless neutrinos, although in this case the agreement between these two measurements is also improved when considering simultaneously baryon acoustic oscillation data and Hubble Space Telescope measurements. In the N-eff massive neutrino case the two high multipole probes give very different results regardless of the external data sets used in the combined analyses. When considering extended cosmological scenarios with a dark energy equation of state or with a running of the scalar spectral index, the evidence for neutrino masses found for the South Pole Telescope in the three neutrino scenario disappears for all the data combinations explored here. Again, adding Hubble Telescope data seems to improve the agreement between the two high multipole cosmic microwave background measurements considered here. In the case in which a dark radiation background with unknown clustering properties is also considered, SPT data seem to exclude the standard value for the dark radiation viscosity c(vis)(2) = 1/3 at the 2 sigma C.L., finding evidence for massive neutrinos only when combining SPT data with baryon acoustic oscillation measurements.
SN  - 1550-7998
UR  - http://arxiv.org/abs/1303.0143
UR  - https://doi.org/10.1103/PhysRevD.87.103519
DO  - 10.1103/PhysRevD.87.103519
LA  - English
N1  - WOS:000319254500004
ID  - Archidiacono_etal2013
ER  -