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If the scalar tau $\stau$ is the next lightest supersymmetric particle and decays into a gravitino ($\gravitino$) being the lightest supersymmetric particle, it will have generally a very long lifetime. In this paper, we investigate the…

高能物理 - 唯象学 · 物理学 2010-10-27 Koichi Hamaguchi , Mihoko M. Nojiri , Albert de Roeck

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

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

Supersymmetric scenarios with a very weakly interacting lightest superpartner (LSP) - like the gravitino or axino - naturally give rise to a long-lived next-to-LSP (NLSP). If the NLSP is a charged slepton it leaves a very distinct signature…

高能物理 - 唯象学 · 物理学 2013-07-16 Jan Heisig

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

Long-lived particles have emerged as a compelling signature of physics beyond the standard model, offering unique discovery opportunities at current and future colliders. We present an analysis of charged long-lived particles leading to…

高能物理 - 唯象学 · 物理学 2026-05-25 Soumyaa Vashishtha , Maximilian Emanuel Goblirsch-Kolb , Isabell Melzer-Pellmann

In supersymmetric theories where the lightest supersymmetric particle is the gravitino the next to lightest supersymmetric particle (NLSP) is typically a long lived charged slepton. These NLSPs can be produced by high energy neutrinos…

高能物理 - 唯象学 · 物理学 2007-05-23 Ivone F. M. Albuquerque

We investigate charged tracks signals of a supersymmetric scenario, where the lighter stop is the next-to-lightest supersymmetric particle (NLSP). It is found that such an NLSP is stable on the scale of the detector at the LHC if one has a…

高能物理 - 唯象学 · 物理学 2008-11-26 Debajyoti Choudhury , Sudhir Kumar Gupta , Biswarup Mukhopadhyaya

We consider supergravity with a gravitino lightest supersymmetric particle. The next-to-lightest supersymmetric particle (NLSP) decays to the gravitino with lifetime naturally in the range 10^4 - 10^8 s. However, cosmological constraints…

高能物理 - 唯象学 · 物理学 2014-11-18 Jonathan L. Feng , Bryan T. Smith

The lighter scalar tau lepton $\sti$ may be the lightest scalar lepton and therefore would be found earlier in future collider experiments. We point out the impact of the measurement of the mass and the mixing angle of $\st$ to discriminate…

高能物理 - 唯象学 · 物理学 2009-10-28 Keisuke Fujii , Mihoko M. Nojiri , Toshifumi Tsukamoto

We analyze the prospects of observing lepton flavour violation in future e-e- and e+e- linear colliders in scenarios where the gravitino is the lightest supersymmetric particle, and the stau is the next-to-lightest supersymmetric particle.…

高能物理 - 唯象学 · 物理学 2010-02-03 Alejandro Ibarra , Sourov Roy

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

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

A study of various SUSY scenarios is presented in which the lightest supersymmetric particle is the gravitino $\sG$ and the next-to-lightest supersymmetric particle is a scalar tau $\stau$ with lifetimes ranging from seconds to years.…

高能物理 - 唯象学 · 物理学 2009-01-07 H. -U. Martyn

We consider a scenario where light bino is the next-to-lightest supersymmetric particle (NLSP) and gravitino/axino is the lightest superysmmetric particle (LSP). For a bino mass less than or around hundred GeV, it can be pair produced at…

高能物理 - 唯象学 · 物理学 2021-07-14 Junmou Chen , Chengcheng Han , Jin Min Yang , Mengchao Zhang

We analyze the scenario within the Next to Minimal Supersymmetric Standard Model (NMSSM), where the lightest supersymmetric particle (LSP) is singlino-like neutralino. By systematically considering various possible admixtures in the…

高能物理 - 唯象学 · 物理学 2023-08-22 Amit Adhikary , Rahool Kumar Barman , Biplob Bhattacherjee , Amandip De , Rohini M. Godbole , Suchita Kulkarni

Long-lived particles have significant enough lifetimes as to, when produced in collisions, leave a distinct signature in the detectors. Driven by increasingly higher energies, trigger and reconstruction algorithms at particle colliders are…

高能物理 - 实验 · 物理学 2021-09-14 Rebeca Gonzalez Suarez

We investigate the collider signatures of heavy, long-lived, neutral particles that decay to charged particles plus missing energy. Specifically, we focus on the case of a neutralino NLSP decaying to Z and gravitino within the context of…

高能物理 - 唯象学 · 物理学 2014-11-21 Patrick Meade , Matthew Reece , David Shih

In R-parity conserving supersymmetric (SUSY) models the lightest SUSY particle (LSP) is stable and a candidate for dark matter. Depending on the coupling and mass of this particle the life time of the next-to-lightest SUSY particle (NLSP)…

天体物理学 · 物理学 2008-11-26 Markus Ahlers

We consider supersymmetric theories where the gravitino is the lightest superparticle (LSP). Assuming that the long-lived next-to-lightest superparticle (NSP) is a charged slepton, we investigate two complementary ways to prove the…

高能物理 - 唯象学 · 物理学 2009-07-09 Wilfried Buchmuller , Koichi Hamaguchi , Michael Ratz , Tsutomu Yanagida
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