Search Publications

The Complete Light-curve Sample of Spectroscopically Confirmed SNe Ia from Pan-STARRS1 and Cosmological Constraints from the Combined Pantheon Sample
DOI: 10.3847/1538-4357/aab9bb Bibcode: 2018ApJ...859..101S

Berger, E.; Kirshner, R. P.; Rest, A. +37 more

We present optical light curves, redshifts, and classifications for 365 spectroscopically confirmed Type Ia supernovae (SNe Ia) discovered by the Pan-STARRS1 (PS1) Medium Deep Survey. We detail improvements to the PS1 SN photometry, astrometry, and calibration that reduce the systematic uncertainties in the PS1 SN Ia distances. We combine the subs…

2018 The Astrophysical Journal
Planck eHST 2313
Elucidating ΛCDM: Impact of Baryon Acoustic Oscillation Measurements on the Hubble Constant Discrepancy
DOI: 10.3847/1538-4357/aaa1ed Bibcode: 2018ApJ...853..119A

Halpern, M.; Weiland, J. L.; Hinshaw, G. +3 more

We examine the impact of baryon acoustic oscillation (BAO) scale measurements on the discrepancy between the value of the Hubble constant (H 0) inferred from the local distance ladder and that from Planck cosmic microwave background (CMB) data. While the BAO data alone cannot constrain H 0, we show that combining the latest B…

2018 The Astrophysical Journal
Planck 240
Measurements of the Temperature and E-mode Polarization of the CMB from 500 Square Degrees of SPTpol Data
DOI: 10.3847/1538-4357/aa9ff4 Bibcode: 2018ApJ...852...97H

Ade, P. A. R.; Chiang, H. C.; Bleem, L. E. +64 more

We present measurements of the E-mode polarization angular auto-power spectrum (EE) and temperature-E-mode cross-power spectrum (TE) of the cosmic microwave background (CMB) using 150 GHz data from three seasons of SPTpol observations. We report the power spectra over the spherical harmonic multipole range 50< {\ell }≤slant 8000 and detect nine…

2018 The Astrophysical Journal
Planck 181
Evolution of the f σ8 tension with the Planck15 /Λ CDM determination and implications for modified gravity theories
DOI: 10.1103/PhysRevD.97.103503 Bibcode: 2018PhRvD..97j3503K

Kazantzidis, Lavrentios; Perivolaropoulos, Leandros

We construct an updated extended compilation of distinct (but possibly correlated) f σ8(z ) redshift space distortion (RSD) data published between 2006 and 2018. It consists of 63 datapoints and is significantly larger than previously used similar data sets. After fiducial model correction we obtain the best fit Ω0 m8<…

2018 Physical Review D
Planck 179
Reducing the H0 and σ8 tensions with dark matter-neutrino interactions
DOI: 10.1103/PhysRevD.97.043513 Bibcode: 2018PhRvD..97d3513D

Di Valentino, Eleonora; Bœhm, Céline; Bouchet, François R. +1 more

The introduction of dark matter-neutrino interactions modifies the cosmic microwave background (CMB) angular power spectrum at all scales, thus affecting the reconstruction of the cosmological parameters. Such interactions can lead to a slight increase of the value of H0 and a slight decrease of S8≡σ8√{Ωm

2018 Physical Review D
Planck 174
Implications of an extended dark energy cosmology with massive neutrinos for cosmological tensions
DOI: 10.1103/PhysRevD.97.123504 Bibcode: 2018PhRvD..97l3504P

Kamionkowski, Marc; Boddy, Kimberly K.; Poulin, Vivian +1 more

We perform a comprehensive analysis of the most common early- and late-universe solutions to the H0 , Ly -α , and S8 discrepancies. When considered on their own, massive neutrinos provide a natural solution to the S8 discrepancy at the expense of increasing the H0 tension. If all extensions are considere…

2018 Physical Review D
Planck 171
Vacuum phase transition solves the H0 tension
DOI: 10.1103/PhysRevD.97.043528 Bibcode: 2018PhRvD..97d3528D

Di Valentino, Eleonora; Melchiorri, Alessandro; Linder, Eric V.

Taking the Planck cosmic microwave background data and the more direct Hubble constant measurement data as unaffected by systematic offsets, the values of the Hubble constant H0 interpreted within the Λ CDM cosmological constant and cold dark matter cosmological model are in ∼3.3 σ tension. We show that the Parker vacuum metamorphosis (…

2018 Physical Review D
Planck 165
Using the full power of the cosmic microwave background to probe axion dark matter
DOI: 10.1093/mnras/sty271 Bibcode: 2018MNRAS.476.3063H

Hložek, Renée; Grin, Daniel; Marsh, David J. E.

The cosmic microwave background (CMB) places stringent constraints on models of dark matter (DM), and on the initial conditions of the Universe. The full Planck data set is used to test the possibility that some fraction of the DM is composed of ultralight axions (ULAs). This represents the first use of CMB lensing to test the ULA model. We find n…

2018 Monthly Notices of the Royal Astronomical Society
Planck 161
The Atacama Cosmology Telescope: The Two-season ACTPol Sunyaev-Zel’dovich Effect Selected Cluster Catalog
DOI: 10.3847/1538-4365/aaa6cb Bibcode: 2018ApJS..235...20H

Hilton, Matt; Hasselfield, Matthew; Sifón, Cristóbal +41 more

We present a catalog of 182 galaxy clusters detected through the Sunyaev-Zel’dovich (SZ) effect by the Atacama Cosmology Telescope in a contiguous 987.5 deg2 field. The clusters were detected as SZ decrements by applying a matched filter to 148 GHz maps that combine the original ACT equatorial survey with data from the first two observi…

2018 The Astrophysical Journal Supplement Series
Planck 159
Structure formation in f(T) gravity and a solution for H0 tension
DOI: 10.1088/1475-7516/2018/05/052 Bibcode: 2018JCAP...05..052N

Nunes, Rafael C.

We investigate the evolution of scalar perturbations in f(T) teleparallel gravity and its effects on the cosmic microwave background (CMB) anisotropy. The f(T) gravity generalizes the teleparallel gravity which is formulated on the Weitzenböck spacetime, characterized by the vanishing curvature tensor (absolute parallelism) and the non-vanishing t…

2018 Journal of Cosmology and Astroparticle Physics
Planck 156