Asymmtric Dark Matter and an Anti-ν signal
Hajime Fukuda (Kavli IPMU)
in collaboration with Shigeki Matsumoto (Kavli IPMU), Satyanarayan Mukhopadhyay (U. Pittsburgh)
arXiv:1411.4014, Phys. Rev. D 92, 013008
Asymmtric Dark Matter and an Anti- signal Hajime Fukuda ( Kavli - - PowerPoint PPT Presentation
Asymmtric Dark Matter and an Anti- signal Hajime Fukuda ( Kavli IPMU) in collaboration with Shigeki Matsumoto (Kavli IPMU), Satyanarayan Mukhopadhyay (U. Pittsburgh) arXiv:1411.4014, Phys. Rev. D 92 , 013008 A Rigid New Physics Dark
Hajime Fukuda (Kavli IPMU)
in collaboration with Shigeki Matsumoto (Kavli IPMU), Satyanarayan Mukhopadhyay (U. Pittsburgh)
arXiv:1411.4014, Phys. Rev. D 92, 013008
Dark energy Dark matter Baryon
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Can we use any symmetry? DM with
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…Not constraining at all
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WIMP ADM Mass EWSB (1-10) GeV Relic abundance WIMP miracle B-L asymmetry Interaction SU(2)L, etc. B-L share Annihilation Detection Collider DD ID model dependent
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WIMP ADM Mass EWSB (1-10) GeV Relic abundance WIMP miracle B-L asymmetry Interaction SU(2)L, etc. B-L share Annihilation Detection Collider DD ID model dependent
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share B-L
nB~nDM w/o tuning
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B-L sharing interaction Y neutral B-L charged 8/14
lead (anti)neutrino signal! e p ν B-L
1
QEM
1 QEM=0 and B-L≠0 ⇒ only ν
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= Balancing
Particle densities
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with a DM-only hidden sector (B-L)ADM is positive
Ibe, Matsumoto and Yanagida 2012
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μcharge ncharge μparticle nparticle
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Indirect detection is possible
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Anti-ν signal is important Hyper-K, INO, …etc.
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