12,118 research outputs found

    Fermionic Dark Matter in Radiative Inverse Seesaw Model with U(1)_{B-L}

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    We construct a radiative inverse seesaw model with local B-L symmetry, and investigate the flavor structure of the lepton sector and the fermionic Dark Matter. Neutrino masses are radiatively generated through a kind of inverse seesaw framework. The PMNS matrix is derived from each mixing matrix of the neutrino and charged lepton sector with large Dirac CP phase. We show that the annihilation processes via the interactions with Higgses which are independent on the lepton flavor violation, have to be dominant in order to satisfy the observed relic abundance by WMAP. The new interactions with Higgses allow us to be consistent with the direct detection result reported by XENON100, and it is possible to verify the model by the exposure of XENON100 (2012).Comment: 15 pages, 1 table, 5 figures; version accepted for publication in Physical Review

    Determination of Boundary Scattering, Intermagnon Scattering, and the Haldane Gap in Heisenberg Chains

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    Low-lying magnon dispersion in a S=1 Heisenberg antiferromagnetic (AF) chain is analyzed using the non-Abelian DMRG method. The scattering length aba_{\rm b} of the boundary coupling and the inter-magnon scattering length aa are determined. The scattering length aba_{\rm b} is found to exhibit a characteristic diverging behavior at the crossover point. In contrast, the Haldane gap Δ\Delta, the magnon velocity vv, and aa remain constant at the crossover. Our method allowed estimation of the gap of the S=2 AF chain to be Δ=0.0891623(9)\Delta = 0.0891623(9) using a chain length longer than the correlation length ξ\xi.Comment: 6 pages, 3 figures, 1 table, accepted in Phys. Rev.

    Shape transformations of a model of self-avoiding triangulated surfaces of sphere topology

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    We study a surface model with a self-avoiding (SA) interaction using the canonical Monte Carlo simulation technique on fixed-connectivity (FC) triangulated lattices of sphere topology. The model is defined by an area energy, a deficit angle energy, and the SA potential. A pressure term is also included in the Hamiltonian. The volume enclosed by the surface is well defined because of the self-avoidance. We focus on whether or not the interaction influences the phase structure of the FC model under two different conditions of pressure Δp{\it \Delta} p; zero and small negative. The results are compared with the previous results of the self-intersecting model, which has a rich variety of phases; the smooth spherical phase, the tubular phase, the linear phase, and the collapsed phase. We find that the influence of the SA interaction on the multitude of phases is almost negligible except for the evidence that no crumpled surface appears under {\it \Delta} p\=\0 at least even in the limit of zero bending rigidity \alpha\to \0. The Hausdorff dimension is obtained in the limit of \alpha\to \0 and compared with previous results of SA models, which are different from the one in this paper.Comment: 9 figure
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