Search Publications

On the estimation of the local dark matter density using the rotation curve of the Milky Way
DOI: 10.1088/1475-7516/2019/10/037 Bibcode: 2019JCAP...10..037D

de Salas, P. F.; Malhan, K.; Freese, K. +2 more

The rotation curve of the Milky Way is commonly used to estimate the local dark matter density ρDM,solar. However, the estimates are subject to the choice of the distribution of baryons needed in this type of studies. In this work we explore several Galactic mass models that differ in the distribution of baryons and dark matter, in order to determ…

2019 Journal of Cosmology and Astroparticle Physics
Gaia 104
Using Gaia DR2 to constrain local dark matter density and thin dark disk
DOI: 10.1088/1475-7516/2019/04/026 Bibcode: 2019JCAP...04..026B

Buch, Jatan; Leung, John Shing Chau; Fan, JiJi

We use stellar kinematics from the latest Gaia data release (DR2) to measure the local dark matter (DM) density ρDM in a heliocentric cylinder of radius R= 150 pc and half-height z= 200 pc. We also explore the prospect of using our analysis to estimate the DM density in local substructure by setting constraints on the surface density an…

2019 Journal of Cosmology and Astroparticle Physics
Gaia 93
Structure formation and exotic compact objects in a dissipative dark sector
DOI: 10.1088/1475-7516/2019/03/036 Bibcode: 2019JCAP...03..036C

Chang, Jae Hyeok; Egana-Ugrinovic, Daniel; Essig, Rouven +1 more

We present the complete history of structure formation in a simple dissipative dark-sector model. The model has only two particles: a dark electron, which is a subdominant component of dark matter, and a dark photon. Dark-electron perturbations grow from primordial overdensities, become non-linear, and form dense dark galaxies. Bremsstrahlung cool…

2019 Journal of Cosmology and Astroparticle Physics
Gaia 66
The local and distant Universe: stellar ages and H0
DOI: 10.1088/1475-7516/2019/03/043 Bibcode: 2019JCAP...03..043J

Verde, Licia; Jimenez, Raul; Cimatti, Andrea +2 more

The ages of the oldest stellar objects in our galaxy provide an independent test of the current cosmological model as they give a lower limit to the age of the Universe. Recent accurate parallaxes by the Gaia space mission, accurate measurements of the metallicity of stars, via individual elemental abundances, and advances in the modelling of stel…

2019 Journal of Cosmology and Astroparticle Physics
Gaia 55
Spectral and spatial analysis of the dark matter subhalo candidates among Fermi Large Area Telescope unidentified sources
DOI: 10.1088/1475-7516/2019/11/045 Bibcode: 2019JCAP...11..045C

Ciucă, Ioana; Kawata, Daisuke; Domínguez, Alberto +5 more

Fermi-LAT unidentified sources (unIDs) have proven to be compelling targets for performing indirect dark matter (DM) searches. In a previous work, we found that among the 1235 unIDs in Fermi-LAT's catalogs (3FGL, 2FHL and 3FHL) only 44 of those are DM subhalos candidates. We now implement a spectral analysis to test whether these remaining sources…

2019 Journal of Cosmology and Astroparticle Physics
Gaia 26
Uncertainties in direct dark matter detection in light of Gaia's escape velocity measurements
DOI: 10.1088/1475-7516/2019/10/034 Bibcode: 2019JCAP...10..034W

Valluri, Monica; Freese, Katherine; Wu, Youjia +2 more

Direct detection experiments have set increasingly stringent limits on the cross section for spin-independent dark matter-nucleon interactions. In obtaining such limits, experiments primarily assume the standard halo model (SHM) as the distribution of dark matter in our Milky Way. Three astrophysical parameters are required to define the SHM: the …

2019 Journal of Cosmology and Astroparticle Physics
Gaia 22
Detecting dark photon dark matter with Gaia-like astrometry observations
DOI: 10.1088/1475-7516/2019/05/015 Bibcode: 2019JCAP...05..015G

Yuan, Qiang; Zhao, Yue; Guo, Huai-Ke +3 more

A class of dark photon dark matter models with ultralight masses would lead to oscillation of a test body through a coupling with baryons or B-L charge. This periodical oscillation of an observer results in swing of a star's apparent position due to the effect of aberration of light, which could be probed with high-precision astrometry observation…

2019 Journal of Cosmology and Astroparticle Physics
Gaia 12
Impact of substructure on local dark matter searches
DOI: 10.1088/1475-7516/2019/12/013 Bibcode: 2019JCAP...12..013I

Ibarra, Alejandro; Kavanagh, Bradley J.; Rappelt, Andreas

Dark matter substructure can contribute significantly to local dark matter searches and may provide a large uncertainty in the interpretation of those experiments. For direct detection experiments, sub-halos give rise to an additional dark matter component on top of the smooth dark matter distribution of the host halo. In the case of dark matter c…

2019 Journal of Cosmology and Astroparticle Physics
Gaia 12
All-sky angular power spectra from cleaned WISE×SuperCOSMOS galaxy number counts
DOI: 10.1088/1475-7516/2019/08/037 Bibcode: 2019JCAP...08..037X

Balaguera-Antolínez, A.; Costa-Duarte, M. V.; Xavier, H. S. +1 more

Aiming to extract cosmological information from linear scales of the WISE×SuperCOSMOS photometric redshift catalog, we perform a characterization of the systematic effects associated with stellar content, evidencing the presence of contamination and obscuration. We create an integrated model for these effects (which together we call "usurper conta…

2019 Journal of Cosmology and Astroparticle Physics
Gaia 9
Resonant assisted annihilation
DOI: 10.1088/1475-7516/2019/11/033 Bibcode: 2019JCAP...11..033N

Nath Maity, Tarak; Sankar Ray, Tirtha

Assisted annihilation is a novel mechanism to generate viable sub-GeV thermal dark matter, where a pair of stable dark matter annihilates with an assister to Standard Model states. Typically such 3 → 2 annihilation topologies are flux suppressed compared to 2 → 2 processes. In this paper, we explore the possibility of a resonant 3 → 2 assisted ann…

2019 Journal of Cosmology and Astroparticle Physics
INTEGRAL 8