کد مقاله | کد نشریه | سال انتشار | مقاله انگلیسی | نسخه تمام متن |
---|---|---|---|---|
1853410 | 1034207 | 2010 | 8 صفحه PDF | دانلود رایگان |
عنوان انگلیسی مقاله ISI
Decaying LSP in SO(10) GUT and PAMELA's cosmic positron
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کلمات کلیدی
موضوعات مرتبط
مهندسی و علوم پایه
فیزیک و نجوم
فیزیک هسته ای و انرژی بالا
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چکیده انگلیسی
We suppose that the lightest supersymmetric particle (LSP) in the minimal supersymmetric standard model (MSSM) is the dark matter. The bino-like LSP can decay through the SO(10) gauge interactions, if one right-handed (RH) neutrino (ν1c) is lighter than the LSP and its superpartner (νË1c) develops a vacuum expectation value (VEV), raising extremely small R-parity violation naturally. The leptonic decay modes can be dominant, if the VEV scale of 16H is a few orders of magnitude lower than the VEV of 45H (â1016GeV), and if a slepton (eË1c) is relatively lighter than squarks. The desired decay rate of the LSP, ÎÏâ¼10â26sâ1 to explain PAMELA data can be naturally achieved, because the gaugino mediating the LSP decay is superheavy. From PAMELA data, the SU(3)cÃSU(2)LÃSU(2)RÃU(1)BâL breaking scale (or the 16H VEV scale) can be determined. A global symmetry is necessary to suppress the Yukawa couplings between one RH (s)neutrino and the MSSM fields. Even if one RH neutrino is quite light, the seesaw mechanism providing the extremely light three physical neutrinos and their oscillations is still at work.
ناشر
Database: Elsevier - ScienceDirect (ساینس دایرکت)
Journal: Physics Letters B - Volume 685, Issue 1, 22 February 2010, Pages 19-26
Journal: Physics Letters B - Volume 685, Issue 1, 22 February 2010, Pages 19-26
نویسندگان
Bumseok Kyae,