3-8 July 2016
The University of Melbourne
Australia/Melbourne timezone

Distinguishing between Warm Dark Matter and Late Kinetic Decoupling using CMB spectral distortions.

4 Jul 2016, 14:00
20m
Carillo Gantner Theatre ()

Carillo Gantner Theatre

Carrillo Gantner Theatre, Sidney Myer Asia Centre The University of Melbourne VIC 3010 Australia
Talk Dark Matter and Particle Astrophysics Dark Matter and Particle Astrophysics

Speaker

James Diacoumis (University of New South Wales)

Description

Recently a number of alternative dark matter models have been introduced as a means of explaining the physics of small-scale structure formation. These include, warm dark matter and dark matter with late kinetic decoupling both of which differ substantially from the canonical cold dark matter formalism. One interesting way of constraining the phenomenology in these models is to look at the characteristic imprint they leave on the photon spectrum left over from the Big Bang. These imprints are known as spectral distortions in the literature and arise due to spatial fluctuations in the photon temperature along the line of sight. As a result, the thermal history of the photon bath gives us a unique insight into the evolution of the early universe. In this talk I will show how this insight can be used to constrain the phenomenology of these dark matter models, in particular noting that the signatures can be used to distinguish between warm dark matter and late kinetic decoupling scenarios.

Primary author

James Diacoumis (University of New South Wales)

Co-authors

Jan Hamann Steen Hannestad (Aarhus University) Yvonne Wong (The University of New South Wales)

Presentation Materials