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Oct 14, 2013 ... Probing interactions within the dark matter sector via extra radiation contributions @ DSU, Trieste. 2. Motivation. Can we estimate how large is ...
Probing interactions within the dark matter sector via extra radiation contributions Roberto A. Lineros R. IFIC-CSIC/U. Valencia and MULTIDARK fellow

In collaboration with U. França, J. Palacio and S. Pastor Based on Phys. Rev. D 87, 123521 (2013), 1303.1776 and work in progress

Motivation

Can we estimate how large is the dark (matter) sector?

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Probing interactions within the dark matter sector via extra radiation contributions @ DSU, Trieste

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Outline

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Introduction



Relativistic species in the Early Universe



WIMP dark matter



A connexion between WIMP and Neff



Conclusions

Probing interactions within the dark matter sector via extra radiation contributions @ DSU, Trieste

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The history of the Universe

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Relativistic species in the Early Universe

Candidates for Dark Radiation SM neutrino contribution

● ● ●

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Sterile neutrinos Lepton asymmetries Neutrino reheating

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Relativistic species in the Early Universe Planck 2013 results Arxiv: 1303.5076

SM neutrino contribution

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Dark Matter

Observations supporting the Dark Matter hypothesis ● ● ● ●

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Dynamics of clusters and galaxies Structure formation CMB anisotropies Baryon Acoustic Oscillation

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WIMP dark matter ●

Big Bang thermal relic



Correct relic abundance for ~ 1 pb · c

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Mass in GeV-TeV range



Many searches strategies

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WIMP dark matter Relic abundance Indirect detection SM

DM

SM

Direct detection

DM

“production” at colliders 14/10/2013

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WIMP dark matter Relic abundance Indirect detection SM +DS

Direct detection

DM

Interaction with the Dark Sector

DM

SM +DS

“production” at colliders 14/10/2013

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WIMPs and Dark Radiation Nothing forbids that WIMPs can have interactions with the Dark Sector

Dark Sector Visible Sector

very light states WIMP

SM particles heavy states

Both sectors are in thermal equilibrium only if WIMPs do

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WIMPs and Dark Radiation Indeed, temperatures for WIMP freeze-out and the DS decoupling are related:

allowing us to explore the contribution of relativistic dof from the Dark Sector in the Early Universe:

N dark gauge bosons 14/10/2013

+3 dark fermions

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N dark gauge bosons ~3 TeV

~100 GeV – 2 TeV

~10 GeV

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+3 dark fermions ~100 GeV – 2 TeV

~10 GeV

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A prototype particle model A possible realization of the idea is:

Scalar DM with a SU(N) symmetry

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Scalar DM + U(1)

Indirect detection cross section

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Direct detection cross section

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Scalar DM + SU(N)

Indirect detection cross section

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Direct detection cross section

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Fermion DM + U(1)

It also works for fermion DM (+ scalar singlet) + SU(N) Indirect detection cross section 14/10/2013

Direct detection cross section

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Conclusions ●

The interactions present only in the Dark Sector can be observed



The latest results on Neff allow a maximum of 20 dark gauge bosons for TeV WIMPs and 13 for ~100 GeV WIMPs



WIMP annihilations in DS reduce the signal on indirect and direct searches allowing to surpass current exclusion zone

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Thanks for you attention

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Backup slides

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Relativistic dof of the SM PDG. Big-Bang Cosmology

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