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相关论文: Mainly axion cold dark matter in the minimal super…

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Axion/axino dark matter (DM) is explored in the minimal supergravity (mSUGRA) and Yukawa-unified supersymmetric grand-unified theory (SUSY GUT) models with surprising results. For this type of scenario, relic DM abundance has three…

高能物理 - 唯象学 · 物理学 2015-05-14 Heaya Ann Summy

Over almost all of minimal supergravity (mSUGRA or CMSSM) model parameter space, there is a large overabundance of neutralino cold dark matter (CDM). We find that the allowed regions of mSUGRA parameter space which match the measured…

高能物理 - 唯象学 · 物理学 2014-11-20 Howard Baer , Andrew D. Box

We consider supersymmetric (SUSY) models wherein the strong CP problem is solved by the Peccei-Quinn (PQ) mechanism with a concommitant axion/axino supermultiplet. We examine R-parity conserving models where the neutralino is the lightest…

高能物理 - 唯象学 · 物理学 2015-05-27 Howard Baer , Andre Lessa , Shibi Rajagopalan , Warintorn Sreethawong

We calculate the relic abundance of thermally produced neutralino cold dark matter in the general 19 parameter supergravity (SUGRA-19) model. A scan over GUT scale parameters reveals that models with a bino-like neutralino typically give…

高能物理 - 唯象学 · 物理学 2014-11-21 Howard Baer , Andrew D. Box , Heaya Summy

We introduce four supersymmetric (SUSY) axion models in which the strong CP problem and the $\mu$ problem are solved with the help of the Peccei-Quinn mechanism and the Kim-Nilles mechanism, respectively. The axion physics enriches the SUSY…

高能物理 - 唯象学 · 物理学 2024-10-15 Zhong-Jun Yang , Tai-Fu Feng , Xing-Gang Wu

Extending the Standard Model with three right-handed neutrinos and a simple QCD axion sector can account for neutrino oscillations, dark matter and baryon asymmetry; at the same time, it solves the strong CP problem, stabilizes the…

高能物理 - 唯象学 · 物理学 2021-09-24 Alberto Salvio , Simone Scollo

We propose a simple extension of the minimal supersymmetric standard model by introducing a gauge singlet in addition to right-handed neutrinos. The model resolves the strong CP problem by Pecci-Quinn symmetry, explains the origin of…

高能物理 - 唯象学 · 物理学 2010-08-02 Wan-Il Park

Within the minimal supergravity model (mSUGRA) framework, the expectation for the relic density of neutralinos exceeds the WMAP determination unless neutralinos a) have a significant higgsino component, b) have a mass close to half that of…

高能物理 - 唯象学 · 物理学 2009-11-10 Howard Baer , Azar Mustafayev , Stefano Profumo , Alexander Belyaev , Xerxes Tata

We present an overview of supersymmetry searches, both at collider experiments and via searches for dark matter (DM). We focus on three DM possibilities in the SUSY context: the thermally produced neutralino, a mixture of axion and axino,…

高能物理 - 唯象学 · 物理学 2014-11-18 Howard Baer , Eun-Kyung Park , Xerxes Tata

The minimal supergravity (mSUGRA or CMSSM) model is an oft-used framework for exhibiting the properties of neutralino (WIMP) cold dark matter (CDM). However, the recent evidence from Atlas and CMS on a light Higgs scalar with mass m_h\simeq…

高能物理 - 唯象学 · 物理学 2015-06-04 Howard Baer , Vernon Barger , Azar Mustafayev

If one simultaneously invokes the SUSY solution to the gauge hierarchy problem and the PQ solution to the strong CP problem, then one might expect mixed axion/neutralino dark matter (DM), i.e. two dark matter particles. In this case, dark…

高能物理 - 唯象学 · 物理学 2013-06-18 Kyu Jung Bae , Howard Baer , Andre Lessa

The axino is a promising candidate for dark matter in the Universe. It is electrically and color neutral, very weakly interacting, and could be - as assumed in this study - the lightest supersymmetric particle, which is stable for unbroken…

高能物理 - 唯象学 · 物理学 2009-11-10 Arnd Brandenburg , Frank Daniel Steffen

We review the main proposals of particle physics for the composition of the cold dark matter in the universe. Strong axion contribution to cold dark matter is not favored if the Peccei-Quinn field emerges with non-zero value at the end of…

高能物理 - 唯象学 · 物理学 2011-01-27 George Lazarides

Slightly extending a right-handed neutrino version of the $3-3-1$ model, we show that it is not only possible to solve the strong CP problem but also to give the total dark matter abundance reported by the Planck collaboration.…

高能物理 - 唯象学 · 物理学 2018-04-13 J. C. Montero , Ana R. Romero Castellanos , B. L. Sánchez-Vega

Recent studies of the cosmic microwave background, large scale structure, and big bang nucleosynthesis (BBN) show trends towards extra radiation. Within the framework of supersymmetric hadronic axion models, we explore two…

高能物理 - 唯象学 · 物理学 2014-01-03 Peter Graf , Frank Daniel Steffen

By eschewing finetuning from the electroweak and QCD sectors of supersymmetry (natural supersymmetry or SUSY), and by invoking the Kim-Nilles solution to the SUSY mu problem, one is lead to models wherein the dark matter is comprised of a…

高能物理 - 唯象学 · 物理学 2015-03-02 Kyu Jung Bae , Howard Baer , Eung Jin Chun

Axions are likely to be the Dark Matter (DM) that cosmological data require. They arise in the Peccei Quinn solution of the strong CP problem. In a previous work we showed that their model has a simple and natural generalization which…

天体物理学 · 物理学 2009-11-10 Roberto Mainini , Loris P. L. Colombo , Silvio A. Bonometto

We calculate the relic abundance of mixed axion/neutralino cold dark matter which arises in R-parity conserving supersymmetric (SUSY) models wherein the strong CP problem is solved by the Peccei-Quinn (PQ) mechanism with a concommitant…

高能物理 - 唯象学 · 物理学 2015-05-30 Howard Baer , Andre Lessa , Warintorn Sreethawong

If the axino is the lightest superpartner and satisfies cosmological bounds, including a preferred range of the relic abundance of cold dark matter, then the usual stringent constraints on the parameter space of the CMSSM become greatly…

高能物理 - 唯象学 · 物理学 2009-11-10 Laura Covi , Leszek Roszkowski , Roberto Ruiz de Austri , Michael Small

The Peccei-Quinn mechanism presents a neat solution to the strong CP problem. As a by-product, it provides an ideal dark matter candidate, "the axion", albeit with a tiny mass. Axions therefore can act as dark radiation if excited with…

高能物理 - 唯象学 · 物理学 2016-09-28 Anupam Mazumdar , Saleh Qutub , Ken'ichi Saikawa
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