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相关论文: Determining the mass for an ultralight gravitino a…

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Gauge mediated supersymmetry breaking scenarios with an ultra-light gravitino of mass m_{3/2}=1-10 eV are very interesting, since there is no cosmological gravitino problem. We propose a new experimental determination of the gravitino mass…

高能物理 - 唯象学 · 物理学 2008-11-26 K. Hamaguchi , S. Shirai , T. T. Yanagida

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

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

The low-scale gauge mediation scenario of supersymmetry breaking predicts very light gravitino, which makes the next lightest supersymmetric particle (NLSP) quasi stable. We study the LHC phenomenology of the case that the NLSP is the stau.…

高能物理 - 唯象学 · 物理学 2015-06-03 Masaki Asano , Takumi Ito , Shigeki Matsumoto , Takeo Moroi

We report a study on the measurement of the SUSY breaking scale sqrt(F) in the framework of gauge-mediated supersymmetry breaking (GMSB) models at the LHC. The work is focused on the GMSB scenario where a stau is the next-to-lightest SUSY…

高能物理 - 唯象学 · 物理学 2010-02-03 S. Ambrosanio , B. Mele , S. Petrarca , G. Polesello , A. Rimoldi

We consider supersymmetric (SUSY) models in which a very light gravitino is the lightest SUSY particle. Assuming that a neutralino is the next-to-lightest SUSY particle, we present a measurement of the neutralino mass at the LHC in two…

高能物理 - 唯象学 · 物理学 2010-05-12 Koichi Hamaguchi , Eita Nakamura , Satoshi Shirai

A generic feature of gauge-mediated supersymmetry breaking models is that the gravitino is the lightest supersymmetric particle (LSP). In order not to overclose the universe, the gravitino LSP should be light enough (~ 1 keV), or…

高能物理 - 唯象学 · 物理学 2009-11-10 Gi-Chol Cho , Yosuke Uehara

In supergravity where the gravitino is the lightest supersymmetric particle (LSP), the next-to-lightest supersymmetric particle (NLSP) decays to the gravitino with a naturally long lifetime (10^4 - 10^8). However, cosmological constraints…

高能物理 - 唯象学 · 物理学 2011-03-21 J. L. Pinfold , L. Sibley

In the realm of natural supersymmetric models, higgsinos are typically the lightest electroweakinos. In gauge-mediated supersymmetry breaking models, the lightest higgsino-dominated particles decay into a $Z$-boson or a Higgs boson ($h$),…

高能物理 - 唯象学 · 物理学 2024-08-15 Jian-Peng Dai , Song Li , Jin-Min Yang , Yang Zhang , Pengxuan Zhu , Rui Zhu

In gauge-mediated supersymmetry (SUSY) breaking (GMSB) models the lightest supersymmetric particle (LSP) is the gravitino and the phenomenology is driven by the nature of the next-to-lightest SUSY particle (NLSP) which is either the…

高能物理 - 实验 · 物理学 2019-08-20 Gabriele Benelli

We study general conditions for the gravitino to be the lightest supersymmetric particle (LSP) in models with gravity mediated supersymmetry breaking. We find that the decisive quantities are the Kaehler potential K and the gauge kinetic…

高能物理 - 唯象学 · 物理学 2010-05-28 Joern Kersten , Oleg Lebedev

We draw a possible scenario for the observation of massive long-lived charged particles at the LHC detector ATLAS. The required flexibility of the detector triggers and of the identification and reconstruction systems are discussed. As an…

高能物理 - 唯象学 · 物理学 2007-05-23 S. Ambrosanio , B. Mele , A. Nisati , S. Petrarca , G. Polesello , A. Rimoldi , G. Salvini

If supersymmetry is spontaneously at a low energy scale then the resulting gravitino would be very light. The interaction strength of the longitudinal components of such a light gravitino to electron-selectron pair then becomes comparable…

高能物理 - 唯象学 · 物理学 2009-10-31 Uma Mahanta

High-scale supersymmetry (SUSY) with a split spectrum has become increasingly interesting given the current experimental results. A SUSY scale above the weak scale could be naturally associated with a heavy unstable gravitino, whose decays…

高能物理 - 唯象学 · 物理学 2015-06-19 JiJi Fan , Bithika Jain , Ogan Ozsoy

We have examined the capability of the LHC, running at both 7 and 8 TeV, to explore the 19(20)-dimensional parameter space of the pMSSM with neutralino(gravitino) LSPs and soft masses up to 4 TeV employing the ATLAS SUSY analysis suite.…

高能物理 - 唯象学 · 物理学 2012-12-03 M. W. Cahill-Rowley , J. L. Hewett , A. Ismail , T. G. Rizzo

In split-supersymmetry (split-SUSY), gluino is a metastable particle and thus can freeze out in the early universe. The late decay of such a long-life gluino into the lightest supersymmetric particle (LSP) may provide much of the cosmic…

高能物理 - 唯象学 · 物理学 2009-11-11 Fei Wang , Wenyu Wang , Jin Min Yang

The axino and the gravitino are extremely weakly interacting candidates for the lightest supersymmetric particle (LSP). We demonstrate that either of them could provide the right amount of cold dark matter. Assuming that a charged slepton…

高能物理 - 唯象学 · 物理学 2007-05-23 Frank Daniel Steffen

Low-scale gauge-mediated supersymmetry(SUSY)-breaking (GMSB) models with gravitino mass m_{3/2}<16 eV are attractive, since there are no flavor and cosmological problems. In this paper, we thoroughly study the collider signal in the case…

高能物理 - 唯象学 · 物理学 2015-03-17 Eita Nakamura , Satoshi Shirai

The `$\mu$ from $\nu$' supersymmetric standard model ($\mu\nu$SSM) solves the $\mu$ problem of supersymmetric models and reproduces neutrino data, simply using couplings with the three families of right-handed neutrinos $\nu$'s. Novel…

高能物理 - 唯象学 · 物理学 2016-08-30 Carlos Muñoz

We investigate the LHC sensitivity to supersymmetric models with light higgsinos, small R-parity breaking and gravitino dark matter. The limits on decaying gravitino dark matter from gamma-ray searches with the Fermi-LAT put a lower bound…

高能物理 - 唯象学 · 物理学 2013-03-06 S. Bobrovskyi , J. Hajer , S. Rydbeck
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