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Related papers: Lightest Neutralino Mass in the MNSSM

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We study the scenario of gravitino DM with a general neutralino NLSP in a model independent way. We consider all neutralino decay channels and compare them with the most recent BBN constraints. We check how those bounds are relaxed for a…

High Energy Physics - Phenomenology · Physics 2009-11-13 Laura Covi , Jasper Hasenkamp , Stefan Pokorski , Jonathan Roberts

We examine the current state of neutralino dark matter and consider how the LEP constraints on the Minimal Supersymmetric Standard Model parameters are squeezing the available dark matter regions. We also show how cosmological constraints…

High Energy Physics - Phenomenology · Physics 2007-05-23 Toby Falk

We present the strongest current cosmological upper limit on the sum of neutrino masses of < 0.18 (95% confidence). It is obtained by adding observations of the large-scale matter power spectrum from the WiggleZ Dark Energy Survey to…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-16 Signe Riemer-Sørensen , David Parkinson , Tamara M. Davis

The relic abundance and the scalar cross-section off nucleon for light neutralinos (of mass below about 45 GeV) are evaluated in an effective MSSM model without GUT-inspired relations among gaugino masses. It is shown that these neutralinos…

High Energy Physics - Phenomenology · Physics 2008-11-26 A. Bottino , N. Fornengo , S. Scopel

We give an overview of our precise calculation of the relic density of the lightest neutralino, in which we included relativistic Boltzmann averaging, subthreshold and resonant annihilations, and coannihilation processes with charginos and…

High Energy Physics - Phenomenology · Physics 2015-06-25 Paolo Gondolo , Joakim Edsjo

We consider the problem of a proper definition of the mass of a heavy unstable boson. It is shown how various definitions are related by the renormalization-scheme independence of the full resummed amplitude. This is made explicit for the…

High Energy Physics - Phenomenology · Physics 2009-10-28 Wim Beenakker , Geert Jan van Oldenborgh , Jiri Hoogland , Ronald Kleiss

We examine the cross sections for the elastic scattering of neutralinos $\chi$ on nucleons $p,n$, as functions of $m_\chi$ in the constrained minimal supersymmetric standard model. We find narrow bands of possible values of the cross…

High Energy Physics - Phenomenology · Physics 2009-09-11 John Ellis , Andrew Ferstl , Keith A. Olive

The latest experimental results from the LHC and dark matter (DM) searches suggest that the parameter space allowed in supersymmetric theories is subject to strong reductions. These bounds are especially constraining for scenarios entailing…

High Energy Physics - Phenomenology · Physics 2017-05-04 M. Peiro , S. Robles

Promptly decaying lightest neutralinos and long-lived staus are searched for in the context of light gravitino scenarios. It is assumed that the stau is the next to lightest supersymmetric particle (NLSP) and that the lightest neutralino is…

High Energy Physics - Experiment · Physics 2010-04-08 DELPHI Collaboration , P. Abreu et al

We study the neutralino sector of the left-right supersymmetric model. In addition to the possibilities available in the minimal supersymmetric model, the neutralino states can be superpartners of the U(1)_{B-L} gauge boson, the neutral…

High Energy Physics - Phenomenology · Physics 2009-11-11 Durmus A. Demir , Mariana Frank , Ismail Turan

We revisit the case of a light neutralino LSP in the framework of the MSSM. We consider a model with eleven free parameters. We show that all scenarios where the annihilation of light neutralinos rely mainly on the exchange of a light…

High Energy Physics - Phenomenology · Physics 2013-05-29 Daniel Albornoz Vasquez , Genevieve Belanger , Celine Boehm

At present, the strongest upper limit on $\sum m_{\nu}$, the sum of neutrino masses, is from cosmological measurements. However, this bound assumes that the neutrinos are stable on cosmological timescales, and is not valid if the neutrino…

High Energy Physics - Phenomenology · Physics 2020-05-04 Zackaria Chacko , Abhish Dev , Peizhi Du , Vivian Poulin , Yuhsin Tsai

Light neutralino dark matter can be achieved in the Minimal Supersymmetric Standard Model if staus are rather light, with mass around 100 GeV. We perform a detailed analysis of the relevant supersymmetric parameter space, including also the…

High Energy Physics - Phenomenology · Physics 2013-11-07 Genevieve Belanger , Guillaume Drieu La Rochelle , Beranger Dumont , Rohini M. Godbole , Sabine Kraml , Suchita Kulkarni

The electroweak sector may play a crucial role in discovering supersymmetry. We systematically investigate the patterns of the MSSM-like electroweakinos, when the neutralino relic abundance $\Omega_\chi h^2\leq 0.12$, that is, also…

High Energy Physics - Phenomenology · Physics 2016-01-20 Marcin Badziak , Antonio Delgado , Marek Olechowski , Stefan Pokorski , Kazuki Sakurai

The case for small neutrino mass differences from atmospheric and solar neutrino oscillation experiments has become compelling, but leaves the overall neutrino mass scale m_nu undetermined. The most restrictive limit of m_nu < 0.8 eV arises…

Astrophysics · Physics 2009-11-07 G. G. Raffelt

Vacuum stability implies a lower limit on the mass of the higgs boson in the Standard Model (SM). In contrast, an upper limit on the lightest higgs mass can be calculated in supersymmetric (susy) models. The main uncertainty in each limit…

High Energy Physics - Phenomenology · Physics 2015-06-25 Marco A. Diaz , Tonnis A. ter Veldhuis , Thomas J. Weiler

Upper limits on neutrino masses from cosmology have been reported recently to reach the impressive sub-eV level, which is competitive with future terrestrial neutrino experiments. In this brief overview of the latest limits from cosmology I…

High Energy Physics - Phenomenology · Physics 2009-11-11 Oystein Elgaroy

BLMSSM is the extension of the minimal supersymmetric standard model(MSSM). Its local gauge group is $SU(3)_C \times SU(2)_L \times U(1)_Y \times U(1)_B \times U(1)_L$. Supposing the lightest scalar neutrino is dark matter candidate, we…

High Energy Physics - Phenomenology · Physics 2021-09-22 Ming-Jie Zhang , Shu-Min Zhao , Xing-Xing Dong , Zhong-Jun Yang , Tai-Fu Feng

We consider the phenomenological implications of a soft SUSY breaking term BN at the TeV scale (here B is the U(1)_Y gaugino and N is the right-handed neutrino field). In models with a massless (or nearly massless) neutralino, such a term…

High Energy Physics - Phenomenology · Physics 2016-09-06 I. Gogoladze , J. Lykken , C. Macesanu , S. Nandi

We examine the properties of relic neutralinos in the regions of the parameter space selected by recent fits to all the electroweak observables within the Minimal Supersymmetric Standard Model. We discuss the relic neutralino cosmic…

High Energy Physics - Phenomenology · Physics 2009-10-28 A. Bottino , G. Mignola , M. Olechowski , S. Scopel