2014
DOI: 10.3389/fphy.2013.00033
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Theories relating baryon asymmetry and dark matter

Abstract: The nature of dark matter and the origin of the baryon asymmetry are two of the deepest mysteries of modern particle physics. In the absence of hints regarding a possible solution to these mysteries, many approaches have been developed to tackle them simultaneously leading to very diverse and rich models. We give a short review where we describe the general features of some of these models and an overview on the general problem. We also propose a diagrammatic notation to label the different models.

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Cited by 28 publications
(38 citation statements)
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References 72 publications
(105 reference statements)
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“…9, various mechanisms for DM production in the ADM models (Table 1 of Ref. [246]) are illustrated. One obvious mechanism is to relate the visible (V) sector baryon asymmetry to the dark (D) sector asymmetry via a heavy particle decay both to V and D sectors.…”
Section: Asymmetric Dark Matter (Adm)mentioning
confidence: 99%
See 2 more Smart Citations
“…9, various mechanisms for DM production in the ADM models (Table 1 of Ref. [246]) are illustrated. One obvious mechanism is to relate the visible (V) sector baryon asymmetry to the dark (D) sector asymmetry via a heavy particle decay both to V and D sectors.…”
Section: Asymmetric Dark Matter (Adm)mentioning
confidence: 99%
“…The idea behind asymmetric dark matter (ADM) [246][247][248] is based on an asymmetry between DM particles and their antiparticles (''anti-DM''). In the early Universe, only the number density difference between the two (asymmetric component) remains after the annihilation of the symmetric components of DM and anti-DM.…”
Section: Asymmetric Dark Matter (Adm)mentioning
confidence: 99%
See 1 more Smart Citation
“…Above this mass, the accretion rate scales as 1/m 2 χ for kinematic reasons: it is less likely that DM particles lose enough energy to be captured in a single scatter. 2 In the following, we are referring to µ F , the averaged Fermi chemical potential of neutrons in DM-neutron collision. It is not a surprise that Pauli blocking affects the capture rate for m χ below 1 GeV.…”
Section: Resultsmentioning
confidence: 99%
“…However, for Asymmetric Dark Matter (ADM, see e.g. the reviews of [1][2][3][4]), this is very interesting because DM accumulating in the center could form a core which could further gravitationally collapse into a black hole. The requirement that such collapses do not occur gives constraints on the mass and interactions of particle DM.…”
Section: Introductionmentioning
confidence: 99%