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相关论文: Axino Dark Matter and the CMSSM

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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

Supersymmetric extensions of the Standard Model that incorporate the axion 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, the axino…

高能物理 - 唯象学 · 物理学 2010-02-03 Laura Covi , Hang Bae Kim , Jihn E. Kim , Leszek Roszkowski

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 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

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 possibility of the CDM axino is presented. From the early days of supersymmetry, axino has been considered as hot dark matter and warm dark matter. But the CDM axino has been considered quite recently. It is because the low reheating…

天体物理学 · 物理学 2007-05-23 Jihn E. Kim

We address the question how light the lightest MSSM neutralino can be as dark matter candidate in a scenario where all supersymmetric scalar particles are heavy. The hypothesis that the neutralino accounts for the observed dark matter…

高能物理 - 唯象学 · 物理学 2015-06-23 Lorenzo Calibbi , Jonas M. Lindert , Toshihiko Ota , Yasutaka Takanishi

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

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

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

The axino dark matter hypothesis in RSII brane model is studied. Within the framework of CMSSM we assume that the lightest neutralino or stau is the NLSP, and that the axino production has a single contribution from the NLSP decay. It is…

高能物理 - 唯象学 · 物理学 2012-08-16 Jin U Kang , Grigoris Panotopoulos

The constraints imposed on the Minimal Supersymmetric Standard Model (MSSM) parameter space by the Large Hadron Collider (LHC) Higgs mass limit and gluino mass lower bound are revisited. We also analyze the thermal relic abundance of…

高能物理 - 唯象学 · 物理学 2016-01-12 W. Abdallah , S. Khalil

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

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

In recent work, it has been argued that multi-TeV masses for scalar superpartners are not unnatural. Indeed, they appear to have significant phenomenological virtues. Here we explore the implications of such `focus point' supersymmetry for…

高能物理 - 唯象学 · 物理学 2009-09-25 Jonathan L. Feng , Konstantin T. Matchev , Frank Wilczek

The axino, the supersymmetric partner of axion, is a well-motivated warm/hot dark matter candidate, and provides a natural solution to the relic density problem for the bino-like neutralino if it is the lightest supersymmetric particle…

高能物理 - 唯象学 · 物理学 2023-04-04 Wenxing Zhang , Waqas Ahmed , Imtiaz Khan , Tianjun Li , Shabbar Raza

The viability of the lightest neutralino as a dark matter candidate in the Next-to-Minimal Supersymmetric Standard Model is analysed. We carry out a thorough analysis of the parameter space, taking into account accelerator constraints as…

高能物理 - 唯象学 · 物理学 2010-10-27 D. G. Cerdeno , E. Gabrielli , D. E. Lopez-Fogliani , C. Munoz , A. M. Teixeira

We consider supersymmetric scenarios, compatible with all cosmological and phenomenological requirements, where the lightest SUSY particles (LSPs) are the neutralino and a quasi degenerate gluino. We study the neutralino relic abundance,…

高能物理 - 唯象学 · 物理学 2007-05-23 S. Profumo , C. E. Yaguna
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