Wave dark matter
L Hui - Annual Review of Astronomy and Astrophysics, 2021 - annualreviews.org
We review the physics and phenomenology of wave dark matter: a bosonic dark matter
candidate lighter than about 30 eV. Such particles have a de Broglie wavelength exceeding …
candidate lighter than about 30 eV. Such particles have a de Broglie wavelength exceeding …
Black holes, gravitational waves and fundamental physics: a roadmap
L Barack, V Cardoso, S Nissanke… - … and quantum gravity, 2019 - iopscience.iop.org
70 AIM, UMR 7158, CEA/DRF, CNRS, Université Paris Diderot, Irfu/Service d'Astrophysique,
Centre de Saclay, FR-91191 Gif-sur-Yvette, France
Centre de Saclay, FR-91191 Gif-sur-Yvette, France
Cosmological implications of ultralight axionlike fields
Cosmological observations are used to test for imprints of an ultralight axionlike field (ULA),
with a range of potentials V (ϕ)∝[1-cos (ϕ/f)] n set by the axion-field value ϕ and decay …
with a range of potentials V (ϕ)∝[1-cos (ϕ/f)] n set by the axion-field value ϕ and decay …
Ultra-light axions and the S 8 tension: joint constraints from the cosmic microwave background and galaxy clustering
We search for ultra-light axions as dark matter (DM) and dark energy particle candidates, for
axion masses 10-32 eV≤ ma≤ 10-24 eV, by a joint analysis of cosmic microwave …
axion masses 10-32 eV≤ ma≤ 10-24 eV, by a joint analysis of cosmic microwave …
Large-misalignment mechanism for the formation of compact axion structures: Signatures from the QCD axion to fuzzy dark matter
Axions are some of the best motivated particles beyond the Standard Model. We show how
the attractive self-interactions of dark matter (DM) axions over a broad range of masses, from …
the attractive self-interactions of dark matter (DM) axions over a broad range of masses, from …
New horizons: Scalar and vector ultralight dark matter
The last decade has seen unprecedented effort in dark matter model building at all mass
scales coupled with the design of numerous new detection strategies. Transformative …
scales coupled with the design of numerous new detection strategies. Transformative …
Axion dark matter detection with CMB polarization
MA Fedderke, PW Graham, S Rajendran - Physical Review D, 2019 - APS
We point out two ways to search for low-mass axion dark matter using cosmic microwave
background (CMB) polarization measurements. These appear, in particular, to be some of …
background (CMB) polarization measurements. These appear, in particular, to be some of …
Cosmological structure formation and soliton phase transition in fuzzy dark matter with axion self-interactions
We investigate cosmological structure formation in fuzzy dark matter (FDM) with the
attractive self-interaction (SI) with numerical simulations. Such a SI would arise if the FDM …
attractive self-interaction (SI) with numerical simulations. Such a SI would arise if the FDM …
Alleviating cosmological tensions with a coupled scalar fields model
G Liu, Z Zhou, Y Mu, L Xu - Physical Review D, 2023 - APS
In this paper, we investigate the interaction between early dark energy (EDE) and scalar
field dark matter, proposing a coupled scalar fields model to address the Hubble tension and …
field dark matter, proposing a coupled scalar fields model to address the Hubble tension and …
Brief review on scalar field dark matter models
LA Ureña-López - Frontiers in Astronomy and Space Sciences, 2019 - frontiersin.org
The existence of dark matter in the universe has been solidly established in the last
decades, after the arrival of accurate cosmological and astrophysical observations, and …
decades, after the arrival of accurate cosmological and astrophysical observations, and …