MSLED, Neutrino Oscillations and the Cosmological Constant
J. Matias, C. P. Burgess
Abstract
We explore the implications for neutrino masses and mixings within the minimal version of the supersymmetric large-extra-dimensions scenario (MSLED). This model was proposed in hep-ph/0404135 to extract the phenomenological implications of the promising recent attempt (in hep-th/0304256) to address the cosmological constant problem. Remarkably, we find that the simplest couplings between brane and bulk fermions within this approach can lead to a phenomenologically-viable pattern of neutrino masses and mixings that is also consistent with the supernova bounds which are usually the bane of extra-dimensional neutrino models. Under certain circumstances the MSLED scenario can lead to a lepton mixing (PMNS) matrix close to the so-called bi-maximal or the tri-bimaximal forms (which are known to provide a good description of the neutrino oscillation data). We discuss the implications of MSLED models for neutrino phenomenology.
Create a lesson
Related papers
Can cosmic neutrinos induce a cosmic birefringence signal?
Mario Reig
Power corrections to heavy-quark spin correlations in small-x deep-inelastic scattering
Meisen Gao
Scale-Invariant Three-Component Dark Matter and Gravitational Wave Signals
Mojtaba Hosseini, Rouzbeh Rouzbehi
Optimal-Transport Contrastive Learning for Centrality Determination in Heavy-Ion Collisions
Shu-Yun Yang, Yu Zhang
Enhancing Gravitational Waves from Global Strings via a First-Order Phase Transition
Yongtao Jia, Ligong Bian, Huai-Ke Guo
Natural Dark Matter in Generalized No-scale F-SU(5) at the HL-LHC and LUX-ZEPLIN Experiment
Tianjun Li, James A. Maxin, Dimitri V. Nanopoulos