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Related papers: Axino - New Candidate for Cold Dark Matter

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Flaton models of Peccei-Quinn symmetry have good particle physics motivation, and are likely to cause thermal inflation leading to a well-defined cosmology. They can solve the $\mu$ problem, and generate viable neutrino masses. Canonical…

High Energy Physics - Phenomenology · Physics 2009-10-31 Eung Jin Chun , Denis Comelli , David H. Lyth

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…

High Energy Physics - Phenomenology · Physics 2009-09-25 Jonathan L. Feng , Konstantin T. Matchev , Frank Wilczek

We consider the thermal production of axino dark matter in high-scale supersymmetry where all the superpartners except the axino are heavier than the maximum and reheating temperatures. In this case, the axinos are produced dominantly in…

High Energy Physics - Phenomenology · Physics 2018-10-02 Ki-Young Choi , Hyun Min Lee

A brief review of supersymmetric models and their candidates for dark matter is carried out. The neutralino is a WIMP candidate in the MSSM where $R$-parity is conserved, but this model has the $\mu$ problem. There are natural solutions to…

High Energy Physics - Phenomenology · Physics 2017-04-05 Carlos Munoz

When the strong CP problem is solved by spontaneous breaking of an anomalous global symmetry in theories with gauge-mediated supersymmetry breaking, the pseudo Goldstone fermion (the axino) is a good candidate of a light sterile neutrino.…

High Energy Physics - Phenomenology · Physics 2009-10-31 Eung Jin Chun

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…

High Energy Physics - Phenomenology · Physics 2014-11-21 Howard Baer , Andrew D. Box , Heaya Summy

There exist several well-motivated candidates for non-baryonic cold dark matter, including neutralinos, axions, axinos, gravitinos, Wimpzillas. I review the dark matter properties of the neutralino and the current status of its detection. I…

High Energy Physics - Phenomenology · Physics 2007-05-23 Leszek Roszkowski

The lack of evidence for weak scale supersymmetry from LHC Run-I and Run-II results along with null results from direct/indirect dark matter detection experiment have caused a paradigm shift in expected phenomenology of SUSY models. The…

High Energy Physics - Phenomenology · Physics 2017-11-22 Hasan Serce

Neutralinos are natural candidates for cold dark matter in many realizations of supersymmetry. We briefly review our recent results in the evaluation of neutralino relic abundance and direct detection rates in a class of supergravity…

High Energy Physics - Phenomenology · Physics 2009-11-07 N. Fornengo

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…

High Energy Physics - Phenomenology · Physics 2013-06-18 Kyu Jung Bae , Howard Baer , Andre Lessa

In supersymmetric axion models, if the gravitino or axino is the lightest SUSY particle (LSP), the other is often the next-to-LSP (NLSP). We investigate the cosmology of such a scenario and point out that the lifetime of the NLSP naturally…

High Energy Physics - Phenomenology · Physics 2017-07-12 Koichi Hamaguchi , Kazunori Nakayama , Yong Tang

The Kim-Nilles mechanism relates the $\mu$ term with the axion scale $f_a$, leading to the axino-Higgsino-Higgs Yukawa coupling of order $\mu/f_a$. This can bring a dangerous thermal production of axinos. If the axino is stable, its mass…

High Energy Physics - Phenomenology · Physics 2011-09-08 Eung Jin Chun

Gravitinos with a mass in the keV range are an interesting candidate for warm dark matter. Recent measurements of the matter density of the universe and of cosmic structures at the dwarf galaxy scale rule out the simplest gravitino models…

Astrophysics · Physics 2009-11-07 Edward A. Baltz , Hitoshi Murayama

The axino and the gravitino are well-motivated candidates for the lightest supersymmetric particle (LSP) and also for cold dark matter in the Universe. Assuming that a charged slepton is the next-to-lightest supersymmetric particle (NLSP),…

High Energy Physics - Phenomenology · Physics 2008-11-26 A. Brandenburg , L. Covi , K. Hamaguchi , L. Roszkowski , F. D. Steffen

After reviewing the theoretical, phenomenological and experimental motivations for supersymmetric extensions of the Standard Model, we recall that supersymmetric relics from the Big Bang are expected in models that conserve R parity. We…

Cosmology and Nongalactic Astrophysics · Physics 2010-01-21 John Ellis , Keith A. Olive

We present a supersymmetric axion model in which the fermionic superpartner of axion, i.e. the axino, corresponds to a sterile neutrino which would accommodate the LSND data with atmospheric and solar neutrino oscillations.

High Energy Physics - Phenomenology · Physics 2007-05-23 Kiwoon Choi

We examine dark matter production rates in supersymmetric axion models typified by the mass hierarchy m_gravitino << m_neutralino << m_axino. In such models, one expects the dark matter to be composed of an axion/gravitino admixture. After…

High Energy Physics - Phenomenology · Physics 2015-04-20 Kyu Jung Bae , Howard Baer , Eung Jin Chun , Chang Sub Shin

Supersymmetric models based on anomaly-mediated SUSY breaking (AMSB) generally give rise to a neutral wino as a WIMP cold dark matter (CDM) candidate, whose thermal abundance is well below measured values. Here, we investigate four…

High Energy Physics - Phenomenology · Physics 2014-11-20 Howard Baer , Radovan Dermisek , Shibi Rajagopalan , Heaya Summy

The strong CP problem of QCD is at heart a problem of naturalness: why is the F\tilde{F} term highly suppressed in the QCD Lagrangian when it seems necessary to explain why there are three and not four light pions? The most elegant solution…

High Energy Physics - Phenomenology · Physics 2016-07-27 Howard Baer

We point out that 7 keV axino dark matter (DM) in the R-parity violating (RPV) supersymmetric (SUSY) Dine-Fischler-Srednicki-Zhitnitsky model can simultaneously reproduce the 3.5keV X-ray excess, and evade stringent constraints from the…

High Energy Physics - Phenomenology · Physics 2018-03-21 Kyu Jung Bae , Ayuki Kamada , Seng Pei Liew , Keisuke Yanagi