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相关论文: Axinos as Dark Matter

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Supersymmetric extensions of the Standard Model when combined with the Peccei-Quinn solution to the strong CP problem necessarily contain also the axino, the fermionic partner of the axion. In contrast to the neutralino and the gravitino,…

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

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

The axino is the fermionic superpartner of the axion. Assuming the axino is the lightest supersymmetric particle and stable due to R-parity conservation, we compute the relic axino density from thermal reactions in the early Universe. From…

高能物理 - 唯象学 · 物理学 2007-05-23 Arnd Brandenburg , Frank Daniel Steffen

The identification of dark matter in our particle physics model is still a very open question. Here we will argue that axinos can be successful dark matter candidates in models with supersymmetry and the axion solution of the strong CP…

宇宙学与河外天体物理 · 物理学 2009-10-22 Laura Covi , Jihn E. Kim

The connection of Dark Matter to our particle physics model is still one of the open cosmological questions. In these proceedings I will argue that axinos can be successful Cold Dark Matter candidates in models with Supersymmetry and the…

高能物理 - 唯象学 · 物理学 2009-11-11 Laura Covi

We point out that the axino predicted as the supersymmetric partner of the axion is a good candidate for the recently proposed sterile neutrino cool dark matter. The axino mass falls into the right range in the context of gauge mediated…

高能物理 - 唯象学 · 物理学 2009-10-31 Eung Jin Chun , Hang Bae Kim

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 existence of dark matter provides strong evidence for physics beyond the Standard Model. Extending the Standard Model with the Peccei-Quinn symmetry and/or supersymmetry, compelling dark matter candidates appear. For the axion, the…

高能物理 - 唯象学 · 物理学 2009-02-18 Frank Daniel Steffen

Axino arises in supersymmetric versions of axion models and is a natural candidate for cold or warm dark matter. Here we revisit axino dark matter produced thermally and non-thermally in light of recent developments. First we discuss the…

高能物理 - 唯象学 · 物理学 2015-05-30 Ki-Young Choi , Laura Covi , Jihn E. Kim , Leszek Roszkowski

In supersymmetric extensions of the Standard Model, the lightest neutralino, the gravitino, and the axino can appear as the lightest supersymmetric particle and as such provide a compelling explanation of the non-baryonic dark matter in our…

高能物理 - 唯象学 · 物理学 2007-11-28 Frank Daniel Steffen

The axino, the fermionic superpartner of the axion, is a well-motivated candidate for cold dark matter if it is the lightest supersymmetric particle. Since the axino couples very weakly to the matter multiplets, the next-to-lightest…

高能物理 - 唯象学 · 物理学 2012-07-25 Ayres Freitas , Frank Daniel Steffen , Nurhana Tajuddin , Daniel Wyler

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

The baryonic and cold dark matter are reviewed in the context of cosmological models. The theoretical search for the particle candidates is limited by supersymmetric extension of the Standard Model. Generically in such models there are just…

天体物理学 · 物理学 2007-05-23 V. Berezinsky

We analyze the mass of the axino, the fermionic superpartner of the axion, in general supergravity models incorporating a Peccei--Quinn--symmetry and determine the cosmological constraints on this mass. In particular, we derive a simple…

高能物理 - 唯象学 · 物理学 2010-11-01 E. J. Chun , A. Lukas

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 investigate the detectability of axino-like particle, which is defined as a supersymmetric partner of axion-like particle and can be a good candidate for dark matter in our Universe. Especially, we consider the fixed target experiments…

高能物理 - 唯象学 · 物理学 2020-01-22 Ki-Young Choi , Takeo Inami , Kenji Kadota , Inwoo Park , Osamu Seto

We review the status of axino dark matter. Two hierarchy problems, the strong CP problem and the gauge hierarchy problem, have led to introducing into particle physics a spontaneously broken global Peccei-Quinn symmetry and a softly broken…

宇宙学与河外天体物理 · 物理学 2015-06-16 Ki-Young Choi , Jihn E. Kim , Leszek Roszkowski

Weak scale supersymmetry is a highly motivated extension of the Standard Model that has a strong degree of support from data. It provides several viable dark matter candidates: the lightest neutralino (a WIMP), the gravitino, and the…

高能物理 - 唯象学 · 物理学 2009-12-07 Howard Baer

We revisit the cosmology of the supersymmetric QCD axion, highlighting the existence of a serious cosmological axino problem that is fully analogous to the gravitino problem of overclosure via thermal production. A general analysis implies…

高能物理 - 唯象学 · 物理学 2015-05-27 Clifford Cheung , Gilly Elor , Lawrence J. Hall

Gravitinos and axinos produced in the late decays of other supersymmetric particles are well-motivated dark matter (DM) candidates, whose experimental evidences are very distinctive and different from other standard candidates, as thermal…

高能物理 - 唯象学 · 物理学 2008-11-26 J. A. R. Cembranos , Jonathan L. Feng , A. Rajaraman , F. Takayama
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