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We discuss prospects of studying supersymmetric model at future $pp$ circular collider (FCC) with its centre-of-mass energy of $\sim 100\ {\rm TeV}$. We pay particular attention to the model in which Wino is lighter than other…

高能物理 - 唯象学 · 物理学 2019-08-05 Shoji Asai , So Chigusa , Toshiaki Kaji , Takeo Moroi , Masahiko Saito , Ryu Sawada , Junichi Tanaka , Koji Terashi , Kenta Uno

The recent result of the higgs search at the LHC experiment has lead to more attention to the supersymmetric standard models with heavy sfermions. Among them, the models with the almost pure wino being the lightest supersymmetric particle…

高能物理 - 唯象学 · 物理学 2015-06-12 Masahiro Ibe , Shigeki Matsumoto , Ryosuke Sato

In supersymmetric models, Winos, partners of the SU(2) gauge bosons, may be the lightest supersymmetric particles (LSPs). For generic parameters, charged and neutral Winos are highly degenerate. Charged Winos travel macroscopic distances,…

高能物理 - 唯象学 · 物理学 2009-09-15 Jonathan L. Feng , Takeo Moroi , Lisa Randall , Matthew Strassler , Shufang Su

The Wino is an $\mathrm{SU}(2)_{L}$ triplet Majorana fermion and a well-motivated dark matter candidate. The mass difference between the charged and the neutral Winos is small thanks to the $\mathrm{SU}(2)_{L}$ symmetry. The small mass…

高能物理 - 唯象学 · 物理学 2023-01-25 Masahiro Ibe , Masataka Mishima , Yuhei Nakayama , Satoshi Shirai

In some supersymmetric models like split supersymmetry or models with non-universal gaugino mass, bino (LSP) and winos (NLSP) may have rather small mass splitting in order to provide the correct dark matter relic density through bino/wino…

高能物理 - 唯象学 · 物理学 2015-04-01 Chengcheng Han , Lei Wu , Jin Min Yang , Mengchao Zhang , Yang Zhang

Higgsinos and Winos in the supersymmetric Standard Model are prime candidates for dark matter due to their weakly interacting nature. The mass differences between their charged components (charginos) and neutral components (neutralinos)…

高能物理 - 唯象学 · 物理学 2024-03-29 Masahiro Ibe , Yuhei Nakayama , Satoshi Shirai

Within the theory of supersymmetry, the lightest neutralino is a dark matter candidate and is often assumed to be the lightest supersymmetric particle (LSP) as well. If the neutral wino or higgsino is dark matter, the upper limit of the LSP…

高能物理 - 唯象学 · 物理学 2019-06-18 Masahiko Saito , Ryu Sawada , Koji Terashi , Shoji Asai

Some extensions of the standard model contain additional leptons which are vectorlike under weak isospin. A class of models is considered in which these leptons do not appreciably mix with the known leptons. In such models, the heavy…

高能物理 - 唯象学 · 物理学 2009-10-28 Marc Sher

We describe a new code and approach using particle-level information to recast the recent CMS disappearing track searches including all run 2 data. Notably, the simulation relies on knowledge of the detector geometry, and we also include…

高能物理 - 唯象学 · 物理学 2022-04-13 Mark D. Goodsell , Lakshmi Priya

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

We study the prospect of determining the decay properties of the gluino in the supersymmetric (SUSY) standard model at a 100 TeV future hadron collider. We consider the case where the neutral Wino is the lightest superparticle. In this…

高能物理 - 唯象学 · 物理学 2021-06-02 So Chigusa , Koichi Hamaguchi , Takeo Moroi , Atsuya Niki , Kosaku Ono

We analyse the mass reach for electroweakinos at future hadron colliders and their interplay with direct detection experiments. Motivated by the LHC data, we focus on split supersymmetry models with different electroweakino spectra. We find…

高能物理 - 唯象学 · 物理学 2015-05-12 Giovanni Grilli di Cortona

In models where the gravitino is the lightest supersymmetric particle (LSP), the next-to-lightest supersymmetric particle (NLSP) is long-lived. We consider an important charged NLSP candidate, the scalar tau $\tilde{\tau}$. Slow charged…

高能物理 - 唯象学 · 物理学 2008-11-26 Koichi Hamaguchi , Yoshitaka Kuno , Tsuyoshi Nakaya , Mihoko M. Nojiri

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

A collider signal with a stable gravitino of ${\cal O}(10)$eV mass at the International Linear Collider (ILC) experiment is investigated. Such a light gravitino is generally predicted in the low-scale gauge mediation scenario of the…

高能物理 - 唯象学 · 物理学 2011-07-06 Shigeki Matsumoto , Takeo Moroi

A search is presented for charged, long-lived supersymmetric particles in final states with one or more disappearing tracks. The search is based on data from proton-proton collisions at a center-of-mass energy of 13 TeV collected with the…

高能物理 - 实验 · 物理学 2024-04-29 CMS Collaboration

The next-generation water Cherenkov Hyper-Kamiokande detector will be able to detect thousands of neutrino events from a galactic Supernova explosion via Inverse Beta Decay processes followed by neutron capture on Gadolinium. This superb…

高能物理 - 唯象学 · 物理学 2023-10-10 Federica Pompa , Olga Mena

We point out that there is a parameter region in supersymmetry with heavy scalars and higgsinos, in which the heavier of bino and wino becomes long-lived as a consequence of the heavy higgsinos. In this region these electroweak gaugino…

高能物理 - 唯象学 · 物理学 2016-01-20 Krzysztof Rolbiecki , Kazuki Sakurai

In some class of supersymmetric (SUSY) models, the neutral Wino becomes the lightest superparticle and the Bino decays into the Wino and standard-model particles. In such models, we show that the measurement of the Bino mass is possible if…

高能物理 - 唯象学 · 物理学 2009-11-19 Shoji Asai , Yuya Azuma , Osamu Jinnouchi , Takeo Moroi , Satoshi Shirai , T. T. Yanagida

We investigate the phenomenology of a wino LSP as obtained in AMSB and some string models. The WMAP constraint on the DM relic density implies a wino LSP mass of 2.0-2.3 TeV. We find a viable signature for such a heavy wino at CLIC,…

高能物理 - 唯象学 · 物理学 2008-11-26 Utpal Chattopadhyay , Debottam Das , Partha Konar , D. P. Roy
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