Dark matter induced nucleon decay: model and signatures

被引:0
作者
Junwu Huang
Yue Zhao
机构
[1] Stanford University,Stanford Institute of Theoretical Physics, Physics Department
[2] SLAC National Accelerator Laboratory,undefined
来源
Journal of High Energy Physics | / 2014卷
关键词
Beyond Standard Model; Rare Decays;
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摘要
If dark matter (DM) carries anti-baryon number, a DM particle may annihilate with a nucleon by flipping to anti-DM. Inspired by Hylogenesis models, we introduce a single component DM model where DM is asymmetric and carries B and L as -1/2. It can annihilate with a nucleon to an anti-lepton and an anti-DM at leading order or with an additional meson at sub-leading order. Such signals may be observed in proton decay experiments. If DM is captured in the Sun, the DM induced nucleon decay can generate a large flux of anti-neutrinos, which could be observed in neutrino experiments. Furthermore, the anti-DM particle in the final state obtains a relatively large momentum (few hundred MeV), and escapes the Sun. These fast-moving anti-DM particles could also induce interesting signals in various underground experiments.
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[1]  
Petraki K(2013)Review of asymmetric dark matter Int. J. Mod. Phys. A 28 1330028-undefined
[2]  
Volkas RR(1979)A cosmological upper limit on the mass of heavy neutrinos Phys. Lett. B 87 144-undefined
[3]  
Hut P(1985)Technocosmology: could a technibaryon excess provide a ‘natural’ missing mass candidate? Phys. Lett. B 165 55-undefined
[4]  
Olive KA(1990)Baryogenesis in a Baryon Symmetric Universe Phys. Rev. D 42 326-undefined
[5]  
Nussinov S(1987)What Is the Cosmion? Nucl. Phys. B 281 726-undefined
[6]  
Dodelson S(1990)Electroweak Fermion Number Violation and the Production of Stable Particles in the Early Universe Phys. Lett. B 241 387-undefined
[7]  
Widrow LM(1991)Baryogenesis, sphalerons and the cogeneration of dark matter Phys. Rev. D 44 3062-undefined
[8]  
Gelmini G(1992)A Single explanation for both the baryon and dark matter densities Phys. Rev. Lett. 68 741-undefined
[9]  
Hall LJ(1998)A Simultaneous solution to baryogenesis and dark matter problems Phys. Part. Nucl. 29 257-undefined
[10]  
Lin M(2005)Asymmetric sneutrino dark matter and the Ω Phys. Lett. B 605 228-undefined