17,366 research outputs found

    Supersymmetric SO(10)SO(10)-inspired leptogenesis and a new N2N_2-dominated scenario

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    We study the supersymmetric extension of SO(10)SO(10)-inspired thermal leptogenesis showing the constraints on neutrino parameters and on the reheat temperature TRHT_{\rm RH} that derive from the condition of successful leptogenesis from next-to-lightest right handed (RH) neutrinos (N2N_2) decays and the more stringent ones when independence of the initial conditions (strong thermal leptogenesis) is superimposed. In the latter case, the increase of the lightest right-handed neutrino (N1N_1) decay parameters helps the wash-out of a pre-existing asymmetry and constraints relax compared to the non-supersymmetric case. We find significant changes especially in the case of large tan⁡β\tan\beta values (≳15)(\gtrsim 15). In particular, for normal ordering, the atmospheric mixing angle can now be also maximal. The lightest (ordinary) neutrino mass is still constrained within the range 10≲m1/meV≲3010 \lesssim m_1/{\rm meV} \lesssim 30 (corresponding to 75≲∑imi/meV≲12075\lesssim \sum_i m_i/{\rm meV} \lesssim 120). Inverted ordering is still disfavoured, but an allowed region satisfying strong thermal leptogenesis opens up at large tan⁡β\tan\beta values. We also study in detail the lower bound on TRHT_{\rm RH} finding TRH≳1×1010 GeVT_{\rm RH}\gtrsim 1 \times 10^{10}\,{\rm GeV} independently of the initial N2N_2 abundance. Finally, we propose a new N2N_2-dominated scenario where the N1N_1 mass is lower than the sphaleron freeze-out temperature. In this case there is no N1N_1 wash-out and we find TRH≳1×109 GeVT_{\rm RH} \gtrsim 1\times 10^{9}\,{\rm GeV}. These results indicate that SO(10)SO(10)-inspired thermal leptogenesis can be made compatible with the upper bound from the gravitino problem, an important result in light of the role often played by supersymmetry in the quest of a realistic model of fermion masses.Comment: 35 pages, 10 figures; v3: matches JCAP versio

    3D beam-column finite element under non-uniform shear stress distribution due to shear and torsion

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    The paper discusses the application of a 2-node, three-dimensional (3D) beam-column finite element with an enhanced fiber cross-section model to the inelastic response analysis of concrete members. The element accounts for the local distribution of strains and stresses under the coupling of axial, flexural, shear, and torsional effects with an enriched kinematic description that accounts for the out-of-plane deformations of the cross-section. To this end the warping displacements are interpolated with the addition of a variable number of local degrees of freedom. The material response is governed by a 3D nonlinear stress-strain relation with damage that describes the degrading mechanisms of typical engineering materials under the coupling of normal and shear stresses. The element formulation is validated by comparing the numerical results with measured data from the response of two prismatic concrete beams under torsional loading and with standard beam formulations

    Strong thermal leptogenesis and the absolute neutrino mass scale

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    We show that successful strong thermal leptogenesis, where the final asymmetry is independent of the initial conditions and in particular a large pre-existing asymmetry is efficiently washed-out, favours values of the lightest neutrino mass m1≳10 meVm_1 \gtrsim 10\,{\rm meV} for normal ordering (NO) and m1≳3 meVm_1 \gtrsim 3\,{\rm meV} for inverted ordering (IO) for models with orthogonal matrix entries respecting ∣Ωij2∣≲2|\Omega_{ij}^2| \lesssim 2. . We show analytically why lower values of m1m_1 require a high level of fine tuning in the seesaw formula and/or in the flavoured decay parameters (in the electronic for NO, in the muonic for IO). We also show how this constraint exists thanks to the measured values of the neutrino mixing angles and can be tighten by a future determination of the Dirac phase. Our analysis also allows to place more stringent constraint for a specific model or class of models, such as SO(10)SO(10)-inspired models, and shows that some models cannot realise strong thermal leptogenesis for any value of m1m_1. A scatter plot analysis fully supports the analytical results. We also briefly discuss the interplay with absolute neutrino mass scale experiments concluding that they will be able in the coming years to either corner strong thermal leptogenesis or find positive signals pointing to a non-vanishing m1m_1. Since the constraint is much stronger for NO than for IO, it is very important that new data from planned neutrino oscillation experiments will be able to solve the ambiguity.Comment: 22 pages; 7 figures; v2: matches JCAP versio
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