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We interpret the KARMEN time anomaly as being due to the production of a (dominantly bino) neutralino with mass 33.9 MeV, which is the lightest supersymmetric particle but decays into 3 leptons through the violation of R-parity. For…

高能物理 - 唯象学 · 物理学 2011-02-16 Debajyoti Choudhury , Herbi Dreiner , Peter Richardson , Subir Sarkar

We examine the parameter space of the purely phenomenological minimal super- symmetric standard model (MSSM), without assuming any supersymmetry breaking scheme. We find that a large region of the parameter space can indeed yield the…

高能物理 - 唯象学 · 物理学 2012-02-29 Nishita Desai , Biswarup Mukhopadhyaya , Saurabh Niyogi

We investigate supergravity models in which the lightest supersymmetric particle (LSP) is a stable gravitino. We assume that the next-lightest supersymmetric particle (NLSP) freezes out with its thermal relic density before decaying to the…

高能物理 - 唯象学 · 物理学 2008-11-26 Jonathan L. Feng , Shufang Su , Fumihiro Takayama

We analyze the conditions under which some supersymmetric generalizations of a class of models descending from string theory allow an axion in the physical spectrum, due to the presence of anomalous abelian gauge interactions. The gauge…

高能物理 - 唯象学 · 物理学 2009-02-02 Claudio Coriano , Marco Guzzi , Nikos Irges , Antonio Mariano

The radiative decay $\nu_H \to \nu_L + \gamma$ of massive neutrinos is analyzed in the framework of the standard model with lepton mixing for very strong magnetic fields $B\gg B_{cr} = m_e^2/e \sim 4.14 \times 10^{13}$G. The analysis is…

高能物理 - 唯象学 · 物理学 2016-09-06 M. Kachelriess , G. Wunner

We revisit the current LHC constraints on the electroweak-ino sector parameters in the minimal supersymmetric standard model (MSSM) that are relevant to explaining the $(g-2)_\mu$ anomaly via the dominant chargino and muon sneutrino loop.…

高能物理 - 唯象学 · 物理学 2018-04-04 Kaoru Hagiwara , Kai Ma , Satyanarayan Mukhopadhyay

In SUSY models with Gauge Mediated Supersymmetry Breaking (GMSB) a gravitino is the lightest SUSY particle (LSP), while a neutralino or a slepton is the next-to-lightest (NLSP). For the pair-production of SUSY particles at the LHC large…

高能物理 - 实验 · 物理学 2019-08-14 M. Terwort

We observe that in SUSY models with non-universal GUT scale gaugino mass parameters, raising the GUT scale SU(2) gaugino mass |M_2| from its unified value results in a smaller value of -m_{H_u}^2 at the weak scale. By the electroweak…

高能物理 - 唯象学 · 物理学 2008-11-26 Howard Baer , Azar Mustafayev , Heaya Summy , Xerxes Tata

We consider extensions of the standard model based on open strings ending on D-branes, in which gauge bosons and their associated gauginos exist as strings attached to stacks of D-branes, and chiral matter exists as strings stretching…

高能物理 - 唯象学 · 物理学 2010-05-12 Luis A. Anchordoqui , Haim Goldberg , Dan Hooper , Danny Marfatia , Tomasz R. Taylor

The supersymmetric decays of the top quark into charged Higgs plus bottom, $\thb$, and into the supersymmetric partner of the top (${\wti u}_1$) plus the lightest neutralino (${\wti \chi}_1^0$), $\tstopneu$, are discussed within the…

高能物理 - 唯象学 · 物理学 2009-09-25 F. M. Borzumati

We consider a class of $U(1)^\prime$-extended MSSM in which the $U(1)^{\prime}$ symmetry is broken by vacuum expectation values (VEVs) of four MSSM singlet fields. While one MSSM singlet field interacts with the MSSM Higgs fields, three of…

高能物理 - 唯象学 · 物理学 2022-04-08 Yaşar Hiçyılmaz , Levent Selbuz , Levent Solmaz , Cem Salih Ün

Motived by the neutrino oscillation data, we consider the lightest tau sneutrino $\tilde \nu_{\tau_1}$ (which is mostly the right tau sneutrino) to be the lightest supersymmetric particle (LSP) in the framework of the minimal supersymmetric…

高能物理 - 唯象学 · 物理学 2009-10-31 C. -L. Chou , H. -L. Lai , C. -P. Yuan

We present some R-parity conserving supersymmetric models which can accommodate the 3.5 keV X-ray line reported in recent spectral studies of the Perseus galaxy cluster and the Andromeda galaxy. Within the Minimal Supersymmetric Standard…

高能物理 - 唯象学 · 物理学 2015-06-22 Bhaskar Dutta , Ilia Gogoladze , Rizwan Khalid , Qaisar Shafi

We have considered a supersymmetric scenario in which the minimal supersymmetric standard model is augmented with a right-chiral neutrino superfield for each generation. Such a scenario can have a lightest supersymmetric particle (LSP)…

高能物理 - 唯象学 · 物理学 2010-11-11 Sanjoy Biswas

We study the light-element abundances in supersymmetric model where the right-handed sneutrino is the lightest superparticle (LSP), assuming that the neutrino masses are purely Dirac-type. In such a scenario, the lightest superparticle in…

高能物理 - 唯象学 · 物理学 2010-05-25 Koji Ishiwata , Masahiro Kawasaki , Kazunori Kohri , Takeo Moroi

Phenomenological issues of no-scale structure of K\"{a}hler potential are re-examined, which arises in various approaches to supersymmetry breaking. When no-scale boundary conditions are given at the Grand Unified scale and universal…

高能物理 - 唯象学 · 物理学 2011-01-27 Shinji Komine , Masahiro Yamaguchi

We evaluate two-body decay modes of charginos in the Minimal Supersymmetric Standard Model with complex parameters (cMSSM). Assuming heavy scalar quarks we take into account all decay channels involving charginos, neutralinos, (scalar)…

高能物理 - 唯象学 · 物理学 2012-10-20 S. Heinemeyer , F. von der Pahlen , C. Schappacher

Most of the phenomenological studies of supersymmetry have been carried out using the so-called minimal supergravity scenario, where one assumes a universal scalar mass, gaugino mass, and trilinear coupling at M_{GUT}. Even though this is a…

高能物理 - 唯象学 · 物理学 2009-09-29 Andre de Gouvea , Alexander Friedland , Hitoshi Murayama

The NMSSM provides an excellent dark matter candidate, usually, the lightest neutralino ($\tilde{\chi}^0_1$) being the lightest supersymmetric particle (LSP), in the universe. It is a mixture of the bino, the neutral wino, the neutral…

高能物理 - 唯象学 · 物理学 2022-04-15 M. M. Almarashi , F. Alhazmi , R. Abdulhafidh , S. Abdul Basir

Supersymmetric (SUSY) standard models in which the lightest SUSY particle (LSP) is an ultralight gravitino (m_{3/2}=O(1) eV) are very attractive, since they are free from the cosmological gravitino problems. If the neutralino is the next…

高能物理 - 唯象学 · 物理学 2009-10-06 Satoshi Shirai , T. T. Yanagida