Search Publications

Indirect dark matter signatures in the cosmic dark ages. I. Generalizing the bound on s -wave dark matter annihilation from Planck results
DOI: 10.1103/PhysRevD.93.023527 Bibcode: 2016PhRvD..93b3527S

Slatyer, Tracy R.

Recent measurements of the cosmic microwave background (CMB) anisotropies by Planck provide a sensitive probe of dark matter annihilation during the cosmic dark ages, and specifically constrain the annihilation parameter feff⟨σ v ⟩/mχ. Using new results (paper II) for the ionization produced by particles injected at arbitrary…

2016 Physical Review D
Planck 448
Dark energy at early times, the Hubble parameter, and the string axiverse
DOI: 10.1103/PhysRevD.94.103523 Bibcode: 2016PhRvD..94j3523K

Kamionkowski, Marc; Karwal, Tanvi

Precise measurements of the cosmic microwave background (CMB) power spectrum are in excellent agreement with the predictions of the standard Λ CDM cosmological model. However, there is some tension between the value of the Hubble parameter H0 inferred from the CMB and that inferred from observations of the Universe at lower redshifts, a…

2016 Physical Review D
Planck 338
Improvement of cosmological neutrino mass bounds
DOI: 10.1103/PhysRevD.94.083522 Bibcode: 2016PhRvD..94h3522G

Ho, Shirley; Mena, Olga; Gerbino, Martina +3 more

The most recent measurements of the temperature and low-multipole polarization anisotropies of the cosmic microwave background from the Planck satellite, when combined with galaxy clustering data from the Baryon Oscillation Spectroscopic Survey in the form of the full shape of the power spectrum, and with baryon acoustic oscillation measurements, …

2016 Physical Review D
Planck 168
Reconciling CMB and structure growth measurements with dark energy interactions
DOI: 10.1103/PhysRevD.94.043518 Bibcode: 2016PhRvD..94d3518P

Pourtsidou, Alkistis; Tram, Thomas

We study a coupled quintessence model with pure momentum exchange and present the effects of such an interaction on the cosmic microwave background (CMB) and matter power spectrum. For a wide range of negative values of the coupling parameter β structure growth is suppressed and the model can reconcile the tension between cosmic microwave backgrou…

2016 Physical Review D
Planck 160
New constraints on interacting dark energy from cosmic chronometers
DOI: 10.1103/PhysRevD.94.023508 Bibcode: 2016PhRvD..94b3508N

Nunes, Rafael C.; Pan, Supriya; Saridakis, Emmanuel N.

We use the latest compilation of observational Hubble parameter measurements estimated with the differential evolution of cosmic chronometers, in combination with the local value of the Hubble constant recently measured with 2.4% precision, to constrain the cosmological scenario where dark energy interacts directly with the dark matter sector. To …

2016 Physical Review D
Planck 135
Eliminating the optical depth nuisance from the CMB with 21 cm cosmology
DOI: 10.1103/PhysRevD.93.043013 Bibcode: 2016PhRvD..93d3013L

Sherwin, Blake D.; Liu, Adrian; Pritchard, Jonathan R. +3 more

Amongst standard model parameters that are constrained by cosmic microwave background (CMB) observations, the optical depth τ stands out as a nuisance parameter. While τ provides some crude limits on reionization, it also degrades constraints on other cosmological parameters. Here we explore how 21 cm cosmology—as a direct probe of reionization—ca…

2016 Physical Review D
Planck 118
CMB constraints on cosmic strings and superstrings
DOI: 10.1103/PhysRevD.93.123503 Bibcode: 2016PhRvD..93l3503C

Moss, Adam; Charnock, Tom; Avgoustidis, Anastasios +1 more

We present the first complete Markov chain Monte Carlo analysis of cosmological models with evolving cosmic (super)string networks, using the unconnected segment model in the unequal-time correlator formalism. For ordinary cosmic string networks, we derive joint constraints on Λ cold dark matter (CDM) and string network parameters, namely the stri…

2016 Physical Review D
Planck 115
Kinematic Sunyaev-Zel'dovich effect with projected fields. II. Prospects, challenges, and comparison with simulations
DOI: 10.1103/PhysRevD.94.123526 Bibcode: 2016PhRvD..94l3526F

Spergel, David N.; Ferraro, Simone; Hill, J. Colin +2 more

The kinematic Sunyaev-Zel'dovich (kSZ) signal is a powerful probe of the cosmic baryon distribution. The kSZ signal is proportional to the integrated free electron momentum rather than the electron pressure (which sources the thermal SZ signal). Since velocities should be unbiased on large scales, the kSZ signal is an unbiased tracer of the large-…

2016 Physical Review D
Planck 85
Cosmological hints of modified gravity?
DOI: 10.1103/PhysRevD.93.023513 Bibcode: 2016PhRvD..93b3513D

Di Valentino, Eleonora; Melchiorri, Alessandro; Silk, Joseph

The recent measurements of cosmic microwave background (CMB) temperature and polarization anisotropies made by the Planck satellite have provided impressive confirmation of the Λ CDM cosmological model. However interesting hints of slight deviations from Λ CDM have been found, including a 95% C.L. preference for a "modified gravity" (MG) structure…

2016 Physical Review D
Planck 77
Cosmological limits on neutrino unknowns versus low redshift priors
DOI: 10.1103/PhysRevD.93.083527 Bibcode: 2016PhRvD..93h3527D

Di Valentino, Eleonora; Melchiorri, Alessandro; Mena, Olga +2 more

Recent cosmic microwave background (CMB) temperature and polarization anisotropy measurements from the Planck mission have significantly improved previous constraints on the neutrino masses as well as the bounds on extended models with massless or massive sterile neutrino states. However, due to parameter degeneracies, additional low redshift prio…

2016 Physical Review D
Planck 71