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相关论文: Probing the supersymmetric parameter space by WIMP…

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Phenomenology of relic neutralinos is analyzed in an effective supersymmetric scheme at the electroweak scale. It is shown that current direct experiments for WIMPs, when interpreted in terms of relic neutralinos, are indeed probing regions…

高能物理 - 唯象学 · 物理学 2007-05-23 A. Bottino , N. Fornengo , S. Scopel

After a short introduction on particle candidates for dark matter within possible extensions of the standard model, we concentrate on Weakly Interacting Massive Particles, and on one of their most interesting physical realizations: the…

高能物理 - 唯象学 · 物理学 2007-05-23 A. Bottino , F. Donato , N. Fornengo , S. Scopel

After a short introduction on some general implications of recent cosmological observations, we discuss the properties of relic neutralinos in connection with present experimental strategies for detecting WIMPs.

高能物理 - 唯象学 · 物理学 2009-11-07 A. Bottino , F. Donato , N. Fornengo , S. Scopel

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…

高能物理 - 唯象学 · 物理学 2009-10-28 A. Bottino , G. Mignola , M. Olechowski , S. Scopel

We analyze the properties of neutralino under the hypothesis that some preliminary experimental results of the DAMA/NaI Collaboration may be indicative of a yearly modulation effect. We examine which supersymmetric configurations would be…

高能物理 - 唯象学 · 物理学 2008-11-26 A. Bottino , F. Donato , N. Fornengo , S. Scopel

We study supersymmetric dark matter in the general flavor diagonal MSSM by means of an extensive random scan of its parameter space. We find that, in contrast with the standard mSUGRA lore, the large majority of viable models features…

高能物理 - 唯象学 · 物理学 2008-11-26 Stefano Profumo , Carlos E. Yaguna

Where is the long--awaited one? A supersymmetric neutralino has been a favored candidate for the WIMP dark matter but, so far, it has not been found. One way to locate it is to identify where it can be hiding in the vast supersymmetric…

高能物理 - 唯象学 · 物理学 2007-05-23 Leszek Roszkowski

It is shown that the new data of the DAMA/NaI detector, combined with recent calculations of nuclear structure functions, provide the most stringent upper bounds on the WIMP-nucleon cross-section both for spin-dependent and for scalar…

高能物理 - 唯象学 · 物理学 2009-10-30 A. Bottino , F. Donato , G. Mignola , S. Scopel , P. Belli , A. Incicchitti

New upper bounds on direct detection rates have recently been presented by a number of experimental collaborations working on searches for WIMPs. In this paper we analyze how the constraints on relic neutralinos which can be derived from…

高能物理 - 唯象学 · 物理学 2015-06-25 A. Bottino , F. Donato , N. Fornengo , S. Scopel

In previous papers we showed that the data of the DAMA/NaI experiment for WIMP direct detection, which indicate a possible annual modulation effect, are widely compatible with an interpretation in terms of a relic neutralino as the major…

高能物理 - 唯象学 · 物理学 2011-05-23 A. Bottino , F. Donato , N. Fornengo , S. Scopel

Direct and indirect detection rates of relic neutralinos are reviewed in the framework of the Minimal Supersymmetric Standard Model. The theoretical estimates are compared with the most recent experimental limits from low-background…

天体物理学 · 物理学 2007-05-23 N. Fornengo

From the relic density measurement by WMAP the WIMP annihilation cross section can be determined in a model independent way. If the WIMPS are postulated to be the neutralinos of Supersymmetry, then only a limited region of the…

高能物理 - 唯象学 · 物理学 2011-09-13 W. de Boer , M. Herold , C. Sander , V. Zhukov

Neutrino telescopes of large area offer the possibility of searching for indirect signals of relic neutralinos in the galactic halo, due to annihilations in the Sun or the Earth. Here we investigate the sensitivity, using a supergravity…

高能物理 - 唯象学 · 物理学 2009-09-11 V. Berezinsky , A. Bottino , J. Ellis , N. Fornengo , G. Mignola , S. Scopel

We demonstrate that the further indication of a possible annual modulation effect, singled out by the DAMA/NaI experiment for WIMP direct detection, is widely compatible with an interpretation in terms of a relic neutralino as the major…

高能物理 - 唯象学 · 物理学 2008-11-26 A. Bottino , F. Donato , N. Fornengo , S. Scopel

Various methods of searching for supersymmetric dark matter are sensitive to WIMPs with different properties. One consequence of this is that the phenomenology of dark matter detection can vary dramatically in different supersymmetric…

高能物理 - 唯象学 · 物理学 2009-11-10 Dan Hooper , Lian-Tao Wang

There is almost universal agreement among astronomers that most of the mass in the Universe and most of the mass in the Galactic halo is dark. Many lines of reasoning suggest that the dark matter consists of some new, as yet undiscovered,…

高能物理 - 唯象学 · 物理学 2009-10-28 G. Jungman , M. Kamionkowski , K. Griest

The lightest neutralino in supersymmetric models with conserved R-parity is an attractive candidate for non-luminous matter in the universe. If relic neutralinos are indeed present as dark matter in our galaxy, they can be directly detected…

高能物理 - 唯象学 · 物理学 2007-05-23 Michal Brhlik

We examine updated prospects for detecting WIMPs in supersymmetric models via direct and indirect dark matter search experiments. We examine several historical and also still viable scenarios: projections for well-tempered neutralinos…

高能物理 - 唯象学 · 物理学 2016-12-28 Howard Baer , Vernon Barger , Hasan Serce

We investigate the production of neutralino dark matter in a cosmological scenario featuring an early matter dominated era ending at a relatively low reheating temperature. In such scenarios different production mechanisms of weakly…

高能物理 - 唯象学 · 物理学 2018-12-18 Manuel Drees , Fazlollah Hajkarim

Recently the DAMA/NaI Collaboration reported further indication of a possible modulation effect in WIMP direct detection. In this note we discuss the relevance of this result for supersymmetric theories where the neutralino is the dark…

高能物理 - 唯象学 · 物理学 2007-05-23 Nicolao Fornengo
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