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Forecasts for warm dark matter from photometric galaxy surveys
(2018-11-01)
We present a Fisher matrix forecast for the sensitivity on the mass of a thermal warm dark matter (WDM) particle from current (DES-like) and future (LSST-like) photometric galaxy surveys using the galaxy angular power ...
A Data Driven Solution to the Dark Matter ProblemA Data Driven Solution to the Dark Matter Problem
(USFQ PRESS, departamento editorial de la Universidad San Francisco de Quito USFQ, 2023)
DM particles: how warm they can be?
(Iop Publishing Ltd, 2009-02-01)
One of important questions concerning particles which compose the Dark Matter (DM) is their average speed. We consider the model of relativistic weakly interacting massive particles and try to impose an upper bound on their ...
Self Interactions in Warm Dark Matter: A View from Cosmological Perturbation Theory
(SP MAIK Nauka/Interperiodica, 2021-10)
We provide a short overview into Self Interacting Warm Dark Matter (SI-WDM) models from the context of Cosmological Perturbation Theory (CPT). The aim is to generalize conventional Cold DM models, by proposing a more general ...
Interacting warm dark matter
(IOP PUBLISHING LTD, 2013)
Boltzmann hierarchies for self-interacting warm dark matter scenarios
(IOP Publishing, 2020-09)
We provide a general framework for self-interacting warm dark matter (WDM) in cosmological perturbations, by deriving from first principles a Boltzmann hierarchy which retains certain independence from a particular interaction ...
DM particles: how warm they can be?
(Iop Publishing Ltd, 2009-02-01)
One of important questions concerning particles which compose the Dark Matter (DM) is their average speed. We consider the model of relativistic weakly interacting massive particles and try to impose an upper bound on their ...
DM particles: how warm they can be?
(Iop Publishing Ltd, 2014)