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相关论文: Determining the Mass for a Light Gravitino

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We discuss the gravitino problem in contest of the Exotic see-saw mechanism for neutrinos and Leptogenesis, UV completed by intersecting D-branes Pati-Salam models. In the Exotic see-saw model, supersymmetry is broken at high scales…

高能物理 - 唯象学 · 物理学 2016-08-10 Andrea Addazi , Maxim Khlopov

Anomaly mediated supersymmetry breaking (AMSB), when implemented in MSSM is known to suffer from the problem of negative slepton mass squared leading to breakdown of electric charge conservation. We show however that when MSSM is extended…

高能物理 - 唯象学 · 物理学 2008-11-26 R. N. Mohapatra , Nobuchika Okada , Hai-Bo Yu

We analyse the direct detection of neutralino dark matter in supergravity scenarios with non-universal soft scalar and gaugino masses. In particular, the neutralino-nucleon cross section is computed and compared with the sensitivity of…

高能物理 - 唯象学 · 物理学 2008-11-26 D. G. Cerdeno , C. Munoz

We consider a SUSY breaking scenario without the Polonyi problem. To solve the problem, the enhanced couplings of the Polonyi field to an inflaton, gauge kinetic functions and itself are assumed. As a result, a gaugino mediated SUSY…

高能物理 - 唯象学 · 物理学 2015-06-12 Takeo Moroi , Tsutomu T. Yanagida , Norimi Yokozaki

The mass of the axino is computed in realistic supersymmetric extensions of the standard model. It is found to be strongly model dependent and can be as small as a few keV but also as large as the gravitino mass. Estimates of this mass can…

高能物理 - 唯象学 · 物理学 2008-11-26 E. J. Chun , Jihn E. Kim , H. P. Nilles

Within the Minimal Supersymmetric Standard Model (MSSM) we systematically investigate the bounds on the mass of the lightest neutralino. We allow for non-universal gaugino masses and thus even consider massless neutralinos, while assuming…

高能物理 - 唯象学 · 物理学 2010-04-23 H. K. Dreiner , S. Heinemeyer , O. Kittel , U. Langenfeld , A. M. Weber , G. Weiglein

We discuss two cosmological issues in a generic gauge-mediated supersymmetry (SUSY)-breaking model, namely the Universe's baryon asymmetry and the gravitino dark-matter density. We show that both problems can be simultaneously solved if…

高能物理 - 唯象学 · 物理学 2009-11-07 Masaaki Fujii , T. Yanagida

We consider an MSSM extension with anomaly mediation as the source of supersymmetry-breaking, and a U(1) symmetry which solves the tachyonic slepton problem, and introduces both the see-saw mechanism for neutrino masses, and the Higgs…

高能物理 - 唯象学 · 物理学 2015-06-04 Mark Hindmarsh , D. R. Timothy Jones

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 employ both the minimal gravity- and the minimal gauge mediations of supersymmetry breaking at the grand unified theory (GUT) scale in a single supergravity framework, assuming the gaugino masses are generated dominantly by the minimal…

高能物理 - 唯象学 · 物理学 2015-06-02 Bumseok Kyae

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 consider the prospects for the direct detection of dark matter in pure gravity meditation (PGM) models of supersymmetry breaking. Minimal PGM models require only two parameters, the gravitino mass, $m_{3/2}$, which sets the UV mass for…

高能物理 - 唯象学 · 物理学 2022-10-05 Jason L. Evans , Keith A. Olive

We present a model of supersymmetry breaking which produces gaugino masses and negligible scalar masses at a high scale. The model is inspired by ``deconstructing'' or ``latticizing'' models in extra dimensions where supersymmetry breaking…

高能物理 - 唯象学 · 物理学 2014-11-17 H. -C. Cheng , D. E. Kaplan , M. Schmaltz , W. Skiba

Gravitino dark matter, together with thermal leptogenesis, implies an upper bound on the masses of superparticles. In the case of broken R-parity the constraints from primordial nucleosynthesis are naturally satisfied and decaying…

高能物理 - 唯象学 · 物理学 2015-05-14 Wilfried Buchmuller

The gravitino is a promising candidate for cold dark matter. We study cosmological constraints on scenarios in which the gravitino is the lightest supersymmetric particle and a charged slepton the next-to-lightest supersymmetric particle…

高能物理 - 唯象学 · 物理学 2011-05-05 Frank Daniel Steffen

We investigate the superWIMP scenario in the framework of supersymmetry, in which the lightest supersymmetric particle is a stable gravitino. We consider slepton, sneutrino or neutralino being the next-lightest supersymmetric particle, and…

高能物理 - 唯象学 · 物理学 2007-05-23 Jonathan L. Feng , Shufang Su , Fumihiro Takayama

Gauge mediation models have two drawbacks, that is, the so-called \mu-problem and a lack of predictability of the gravitino dark matter abundance. We show that conformal sequestering in the supersymmetry breaking sector offers attractive…

高能物理 - 唯象学 · 物理学 2008-11-26 Satoshi Shirai , Fuminobu Takahashi , T. T. Yanagida , Kazuya Yonekura

In models with gauge mediated supersymmetry breaking the gravitino is the lightest supersymmetric particle. If R-parity is violated the gravitino decays, but with a half-live far exceeding the age of the universe and thus is, in principle,…

高能物理 - 唯象学 · 物理学 2008-11-26 M. Hirsch , W. Porod , D. Restrepo

The physics of moduli fields is examined in the scenario where the gravitino is relatively heavy with mass of order 10 TeV, which is favored in view of the severe gravitino problem. The form of the moduli superpotential is shown to be…

高能物理 - 唯象学 · 物理学 2009-11-11 Motoi Endo , Masahiro Yamaguchi , Koichi Yoshioka

In some areas of supersymmetry parameter space, sneutrinos are lighter than the charginos and the next-to-lightest neutralino, and they decay into the invisible neutrino plus lightest-neutralino channel with probability one. In such a…

高能物理 - 唯象学 · 物理学 2008-11-26 A. Freitas , W. Porod , P. M. Zerwas
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