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相关论文: A Test for Light Gravitino Scenario at the LHC

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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 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

High energy electron-photon colliders provide unique opportunities for probing physics beyond the standard model. We have studied the experimental signatures for two supersymmetric scenarios, with the lightest supersymmetric particle (LSP)…

高能物理 - 唯象学 · 物理学 2009-10-28 Ken Kiers , John N. Ng , Guohong Wu

We address the question how light the lightest MSSM neutralino can be as dark matter candidate in a scenario where all supersymmetric scalar particles are heavy. The hypothesis that the neutralino accounts for the observed dark matter…

高能物理 - 唯象学 · 物理学 2015-06-23 Lorenzo Calibbi , Jonas M. Lindert , Toshihiko Ota , Yasutaka Takanishi

Supersymmetric scenarios where the lightest superparticle (LSP) is the gravitino are an attractive alternative to the widely studied case of a neutralino LSP. A strong motivation for a gravitino LSP arises from the possibility of achieving…

高能物理 - 唯象学 · 物理学 2014-04-24 Jan Heisig

In supersymmetric (SUSY) models with the gravitino being the lightest SUSY particle (LSP), the SUSY breaking scale (i.e., the gravitino mass) could be determined by measuring the lifetime of the next-to-lightest SUSY particle (NLSP).…

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

The axino and the gravitino are well-motivated candidates for the lightest supersymmetric particle (LSP) and also for cold dark matter in the Universe. Assuming that a charged slepton is the next-to-lightest supersymmetric particle (NLSP),…

高能物理 - 唯象学 · 物理学 2008-11-26 A. Brandenburg , L. Covi , K. Hamaguchi , L. Roszkowski , F. D. Steffen

In a large class of supersymmetric (SUSY) axion model the mass of axino $\axino$ (a fermionic superpartner of the axion) is predicted as $m_{\axino} \lesssim {\cal O}(1)$ keV. Thus, the axino is the lightest SUSY particle (LSP). We pointed…

高能物理 - 唯象学 · 物理学 2011-07-18 T. Asaka , T. Yanagida

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

Various supersymmetric (SUSY) scenarios predict a sub-GeV neutralino decaying into a single photon and an invisible state. This signature has recently been studied in a number of intensity frontier experiments, finding constraints…

高能物理 - 唯象学 · 物理学 2023-06-02 Krzysztof Jodłowski

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

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

We consider the possibility that the gravitino might be the lightest supersymmetric particle (LSP) in the constrained minimal extension of the Standard Model (CMSSM). In this case, the next-to-lightest supersymmetric particle (NSP) would be…

高能物理 - 唯象学 · 物理学 2008-11-26 John Ellis , Keith A. Olive , Yudi Santoso , Vassilis Spanos

We discuss the prospects for detecting supersymmetric particles in variants of the minimal supersymmetric extension of the Standard Model (MSSM), in light of laboratory and cosmological constraints. We first assume that the lightest…

高能物理 - 唯象学 · 物理学 2009-09-11 John Ellis , Keith A. Olive , Yudi Santoso , Vassilis C. Spanos

In this paper we study the experimental consequences of a theory which naturally has a heavy, stable (or almost stable) gluino. We define the boundary conditions at a messenger scale $M \sim 10^{14}$ GeV which lead to this alternative…

高能物理 - 唯象学 · 物理学 2009-10-31 Stuart Raby , Kazuhiro Tobe

We consider theories with spontaneously broken global or local supersymmetry where the pseudo-goldstino or the gravitino is the lightest superparticle (LSP). Assuming that the long-lived next-to-lightest superparticle (NSP) is a charged…

高能物理 - 唯象学 · 物理学 2007-05-23 Wilfried Buchmuller , Koichi Hamaguchi , Michael Ratz , Tsutomu Yanagida

Using the latest LHC data, we analyse and compare the lower limits on the masses of gluinos and the lightest stop in two natural supersymmetric motivated scenarios: one with a neutralino being the lightest supersymmetric particle (LSP) and…

高能物理 - 唯象学 · 物理学 2019-10-02 Jong Soo Kim , Stefan Pokorski , Krzysztof Rolbiecki , Kazuki Sakurai

We have explored the possibilities of scenarios with heavy gluinos and light stops in supersymmetric (SUSY) standard models with extra vector-like multiplets. If we assume the hierarchical structure for soft masses of the minimal…

高能物理 - 唯象学 · 物理学 2017-04-06 Junji Hisano , Wataru Kuramoto , Takumi Kuwahara

In supersymmetric axion models, if the gravitino or axino is the lightest SUSY particle (LSP), the other is often the next-to-LSP (NLSP). We investigate the cosmology of such a scenario and point out that the lifetime of the NLSP naturally…

高能物理 - 唯象学 · 物理学 2017-07-12 Koichi Hamaguchi , Kazunori Nakayama , Yong Tang

Supersymmetric scenarios with a very weakly interacting lightest superparticle (LSP) - like the gravitino or axino - naturally give rise to a long-lived next-to-LSP (NLSP). In the case of a stau NLSP, the scenario shows up in a very…

高能物理 - 唯象学 · 物理学 2012-07-13 Jan Heisig
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