2011/06/30 by Mansi Dhuria, Aalok Misra
Mathematics · Physics and Astronomy · #Black Holes and Theoretical Physics #Cosmology and Gravitation Theories #Dimension (graph theory) #Divisor (algebraic geometry) #Geometry #Mathematics #Neutrino #Neutrino Physics Research #Particle physics #Physics #Pure mathematics #Ricci curvature #Supersymmetry #Thermodynamics #Volume (thermodynamics) #hep-ph #hep-th
paper · pdf · doi:10.1016/j.nuclphysb.2011.10.006
published as Nucl.Phys. B855 (2012) 439-507 · v3: an error in the Higgsino content of the neutralino and the consequent estimates of tree-level 3-body and 1-loop 2-body gluino decay (involving the neutralino) widths and lifetimes, corrected; conclusions, qualitatively, unchanged. arXiv admin note: text overlap with arXiv:1105.0365 by other author
openalex publication_date 2011/10/24 · arxiv created 2012/02/20 · arxiv updated 2015/05/28 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
We show that it is possible to realize a "mu-split SUSY" scenario [1] in the context of large volume limit of type IIB compactifications on Swiss-Cheese Calabi-Yau's in the presence of a mobile space-time filling D3-brane and a (stack of) D7-brane(s) wrapping the "big" divisor SigmaB. For this, we investigate the possibility of getting one Higgs to be light while other to be heavy in addition to a heavy Higgsino mass parameter. Further, we examine the existence of long lived gluino that manifests one of the major consequences of mu-split SUSY scenario, by computing its decay width as well as lifetime corresponding to the 3-body decays of the gluino into a quark, a squark and a neutralino or Goldstino, as well as 2-body decays of the gluino into either a neutralino or a Goldstino and a gluon. Guided by the geometric Kaehler potential for SigmaB obtained in [2] based on GLSM techniques, and the Donaldson's algorithm [3] for obtaining numerically a Ricci-flat metric, we give details of our calculation in [4] pertaining to our proposed metric for the full Swiss-Cheese Calabi-Yau, but for simplicity of calculation, close to SigmaB, which is Ricci-flat in the large volume limit. Also, as an application of the one-loop RG flow solution for the Higgsino mass parameter, we show that the contribution to the neutrino masses at the EW scale from dimension-six operators arising from the Kaehler potential, is suppressed relative to the Weinberg-type dimension-five operators.