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Related papers: Comments on a Massless Neutralino

200 papers

Signatures of anomaly mediated supersymmetry breaking in linear colliders are briefly reviewed after presenting an outline of the theoretical framework. A unique and distinct feature of a large class of models of this type is a winolike…

High Energy Physics - Phenomenology · Physics 2009-11-10 Sourov Roy

The Spin Light of neutrino, the process that becomes possible in matter for a neutrino with nontrivial electromagnetic properties, is considered for the case of nonequal neutrino masses in the initial and final states.

High Energy Physics - Phenomenology · Physics 2010-12-15 A. Grigoriev , A. Lokhov , A. Studenikin , A. Ternov

We review bounds on neutrino properties, in particular on their masses, coming mostly from cosmology, and also from astrophysics.

High Energy Physics - Phenomenology · Physics 2007-05-23 G. Gelmini

We discuss associated neutralino production e^+ e^- --> \tilde{\chi}^0_1 \tilde{\chi}^0_2 with both beams polarized in the MSSM, NMSSM and an E_6 model. It is shown that neutralinos with a large singlino component can be produced at a high…

High Energy Physics - Phenomenology · Physics 2007-05-23 S. Hesselbach , F. Franke , H. Fraas

Cosmology is at present one of the most powerful probes of neutrino properties. The advent of precision data from the cosmic microwave background and large scale structure has allowed for a very strong bound on the neutrino mass. Here, I…

High Energy Physics - Phenomenology · Physics 2009-11-10 Steen Hannestad

Phenomenology of neutralino dark matter in the minimal supersymmetric model is discussed for a scenario where the lightest Higgs boson mass is lighter than 114.4 GeV. We show that the scenario is consistent not only with many collider…

High Energy Physics - Phenomenology · Physics 2008-11-26 Masaki Asano , Shigeki Matsumoto , Masato Senami , Hiroaki Sugiyama

In the light of the recent Super-Kamiokande experiments which demonstrate neutrino oscillation, and therefore a non zero mass, it is pointed out how such a mass has also been deduced theoretically.

High Energy Physics - Theory · Physics 2007-05-23 B. G. Sidharth

We briefly discuss the main effects of the presence of a Light Sterile Neutrino (LS$\nu$) in Cosmology and how its properties can be constrained by Cosmic Microwave Background (CMB) and other cosmological measurements.

Cosmology and Nongalactic Astrophysics · Physics 2016-01-08 Stefano Gariazzo

We review models for neutrino mass, with special emphasis in supersymmetric models where R-parity is broken either explicitly or spontaneously. The simplest unified extension of the MSSM with explicit bilinear R-parity violation provides a…

High Energy Physics - Phenomenology · Physics 2007-10-31 Jorge C. Romao

Recent advances in cosmic observations have brought us to the verge of discovery of the absolute scale of neutrino masses. Nonzero neutrino masses are known evidence of new physics beyond the Standard Model. Our understanding of the…

The lightest supersymmetric particle (LSP) is stable in an R-parity conserving theory. In this article the steps needed to calculate the present day mass density of such a particle are detailed. It is shown that there can be a…

High Energy Physics - Phenomenology · Physics 2007-05-23 James D. Wells

The experimental and astrophysical status of neutrino masses is reviewed with an emphasis on the cosmologically interesting regime.

High Energy Physics - Phenomenology · Physics 2007-05-23 Georg G. Raffelt

We evaluate the fluxes of up--going muons detectable in a neutrino telescope and due to the annihilation of relic neutralinos in the Earth and in the Sun, taking realistically into account the fact that neutralinos might provide only a…

High Energy Physics - Phenomenology · Physics 2011-05-23 A. Bottino , N. Fornengo , G. Mignola , L. Moscoso

The current status of neutrino cosmology is reviewed, from the question of neutrino decoupling and the presence of sterile neutrinos to the effects of neutrinos on the cosmic microwave background and large scale structure. Particular…

High Energy Physics - Phenomenology · Physics 2009-11-10 Steen Hannestad

Supersymmetric models with a small neutralino-chargino mass difference, and as a result metastable charginos, have been a popular topic of investigation in collider phenomenology, e.g. in anomaly-mediated models of supersymmetry breaking.…

High Energy Physics - Phenomenology · Physics 2015-06-17 N. -E. Bomark , A. Kvellestad , S. Lola , P. Osland , A. R. Raklev

We study the viability of the lightest neutralino as a dark matter candidate in the Next-to-Minimal Supersymmetric Standard Model. Taking into account accelerator constraints as well as bounds on low-energy observables, and imposing…

High Energy Physics - Phenomenology · Physics 2008-11-26 Ana M. Teixeira

We study the phenomenology of neutralino dark matter within generic supersymmetric scenarios where the Gaugino and Higgsino masses are much lighter than the scalar soft breaking masses (Split Supersymmetry). We consider a low-energy…

High Energy Physics - Phenomenology · Physics 2007-05-23 Antonio Masiero , Stefano Profumo , Piero Ullio

Applying Jarlskog's treatment of the CKM matrix, to the neutralino mass matrix in MSSM for real soft gaugino SUSY breaking and $\mu$-parameters, we construct explicit analytical expressions for the four projectors which acting on any…

High Energy Physics - Phenomenology · Physics 2016-08-16 G. J. Gounaris , C. Le Mouël , P. I. Porfyriadis

We compare the first results on searches for supersymmetry with the Large Hadron Collider (LHC) to the current and near-term performance of experiments sensitive to neutralino dark matter. We limit our study to the particular slices of…

High Energy Physics - Phenomenology · Physics 2011-08-08 Stefano Profumo

We examine the allowed mass range of the lightest neutralino within the Minimal Non--minimal Supersymmetric Standard Model. Being absolutely stable if R-parity is conserved this lightest neutralino is a candidate for the dark matter of the…

High Energy Physics - Phenomenology · Physics 2007-12-12 S. Hesselbach , D. J. Miller , G. Moortgat-Pick , R. Nevzorov , M. Trusov