A Large Majorana-Mass From Calabi-Yau Superstring Models
Naoyuki Haba, Chuichiro Hattori, Masahisa Matsuda, Takeo Matsuoka, Daizo Mochinaga
Abstract
In Calabi-Yau superstring models it is found that two large intermediate energy scales of symmetry breaking can be induced for special types of the nonrenormalizable interactions. In the models one set of SO(10)-singlet, right-handed neutrino and their mirror chiral superfields is needed. Through the study of the minimization of the scalarpotential, the conditions for the presence of two large intermediate scales are obtained. In this scheme a Majorana-mass possibly amounts to O(109 10). This large Majorana-mass solves the solar neutrino problem and also is compatible with the cosmological bound for stable light neutrinos.
Create a lesson
Related papers
Cross-Moment Consistency and the Fifth Adler Coefficient in Hadronic Tau Decays
Gauhar Abbas, Debabina Biswas, Pratham Dadhich et al.
Ground-State Heavy-Baryon Mass Spectrum in the Relativistic Independent Quark Model
Divyajyoti Pandey, Kalpalata Dash, Sanjay Kumar Swain
Born spreading with consistent shower starting scales in MC@NLO and FxFx merging
Rikkert Frederix, Paolo Torrielli
Earthquake Forecast via Neutrino Tomography at the DUNE Baseline
Bipin Singh Koranga, Samrat Vashisht, Vivek Kumar Nautiyal
Light (anti)nuclei production via coalescence in electron-proton collisions: from HERA to EIC
Niccolò Ciavarelli, Francesco Noferini, Francesca Bellini
Heavy quarkonium spin transport in a hot medium
Nora Brambilla, Shuo Fang, Tom Magorsch et al.