488 research outputs found

    An S4×SU(5)S_4 \times SU(5) SUSY GUT of flavour in 6d

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    We propose a 6d model with a SUSY SU(5)SU(5) gauge symmetry. After compactification, it explains the origin of the S4S_4 Family Symmetry with CSD3 vacuum alignment, as well as SU(5)SU(5) breaking with doublet-triplet splitting. The model naturally accounts for all quark and lepton (including neutrino) masses and mixings, incorporating the highly predictive Littlest Seesaw structure. It spontaneously breaks CP symmetry, resulting in successful CP violation in the quark and lepton sectors, while solving the Strong CP problem. It also explains the Baryon Asymmetry of the Universe (BAU) through leptogenesis, with the leptogenesis phase directly linked to the Dirac and Majorana phases.Comment: 23 pages, 6 figures. v3: Version published in JHE

    SO(10)×S4\mathbf{SO(10)}\times \mathbf{S_4} Grand Unified Theory of Flavour and Leptogenesis

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    We propose a Grand Unified Theory of Flavour, based on SO(10)SO(10) together with a non-Abelian discrete group S4S_4, under which the unified three quark and lepton 16-plets are unified into a single triplet 3′3'. The model involves a further discrete group Z4R×Z43 \mathbb{Z}_4^R\times \mathbb{Z}_4^3 which controls the Higgs and flavon symmetry breaking sectors. The CSD2 flavon vacuum alignment is discussed, along with the GUT breaking potential and the doublet-triplet splitting, and proton decay is shown to be under control. The Yukawa matrices are derived in detail, from renormalisable diagrams, and neutrino masses emerge from the type I seesaw mechanism. A full numerical fit is performed with 15 input parameters generating 19 presently constrained observables, taking into account supersymmetry threshold corrections. The model predicts a normal neutrino mass ordering with a CP oscillation phase of 260∘260^{\circ}, an atmospheric angle in the first octant and neutrinoless double beta decay with mββ=11m_{\beta \beta}= 11 meV. We discuss N2N_2 leptogenesis, which fixes the second right-handed neutrino mass to be M2≃2×1011M_2\simeq 2\times 10^{11} GeV, in the natural range predicted by the model.Comment: 26 pages, 10 figure

    Towards a complete A4×SU(5)A_4 \times SU(5) SUSY GUT

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    We propose a renormalisable model based on A4A_4 family symmetry with an SU(5)SU(5) grand unified theory (GUT) which leads to the minimal supersymmetric standard model (MSSM) with a two right-handed neutrino seesaw mechanism. Discrete Z9×Z6\mathbb{Z}_9\times \mathbb{Z}_6 symmetry provides the fermion mass hierarchy in both the quark and lepton sectors, while Z4R\mathbb{Z}_4^R symmetry is broken to Z2R\mathbb{Z}_2^R, identified as usual R-parity. Proton decay is highly suppressed by these symmetries. We discuss both the A4A_4 and SU(5)SU(5) symmetry breaking sectors, including doublet-triplet splitting, Higgs mixing and the origin of the μ\mu term. The model provides an excellent fit (better than one sigma) to all quark and lepton (including neutrino) masses and mixing with spontaneous CP violation. With the A4A_4 vacuum alignments, (0,1,1)(0,1,1) and (1,3,1)(1,3,1), the model predicts the entire PMNS mixing matrix with no free parameters, up to a relative phase, selected to be 2π/32\pi/3 from a choice of the nine complex roots of unity, providing a direct link between neutrino oscillations and leptogenesis.Comment: 30 pages, 17 figures, 7 tables; Minor changes, references added, version accepted in JHE

    Long-Lived Non-Equilibrium Interstitial-Solid-Solutions in Binary Mixtures

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    We perform particle resolved experimental studies on the heterogeneous crystallisation process of two compo- nent mixtures of hard spheres. The components have a size ratio of 0.39. We compared these with molecular dynamics simulations of homogenous nucleation. We find for both experiments and simulations that the final assemblies are interstitial solid solutions, where the large particles form crystalline close-packed lattices, whereas the small particles occupy random interstitial sites. This interstitial solution resembles that found at equilibrium when the size ratios are 0.3 [Filion et al., Phys. Rev. Lett. 107, 168302 (2011)] and 0.4 [Filion, PhD Thesis, Utrecht University (2011)]. However, unlike these previous studies, for our system sim- ulations showed that the small particles are trapped in the octahedral holes of the ordered structure formed by the large particles, leading to long-lived non-equilibrium structures in the time scales studied and not the equilibrium interstitial solutions found earlier. Interestingly, the percentage of small particles in the crystal formed by the large ones rapidly reaches a maximum of around 14% for most of the packing fractions tested, unlike previous predictions where the occupancy of the interstitial sites increases with the system concentration. Finally, no further hopping of the small particles was observed

    Leptogenesis in minimal predictive seesaw models

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    We estimate the Baryon Asymmetry of the Universe (BAU) arising from leptogenesis within a class of minimal predictive seesaw models involving two right-handed neutrinos and simple Yukawa structures with one texture zero. The two right-handed neutrinos are dominantly responsible for the "atmospheric" and "solar" neutrino masses with Yukawa couplings to (νe,νμ,ντ)(\nu_e, \nu_{\mu}, \nu_{\tau}) proportional to (0,1,1)(0,1,1) and (1,n,n−2)(1,n,n-2), respectively, where nn is a positive integer. The neutrino Yukawa matrix is therefore characterised by two proportionality constants with their relative phase providing a leptogenesis-PMNS link, enabling the lightest right-handed neutrino mass to be determined from neutrino data and the observed BAU. We discuss an SU(5)SU(5) SUSY GUT example, where A4A_4 vacuum alignment provides the required Yukawa structures with n=3n=3, while a Z9\mathbb{Z}_9 symmetry fixes the relatives phase to be a ninth root of unity.Comment: 16 pages, 2 tables. v2: minor changes, references added, version accepted in JHE
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