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Related papers: Axino Cold Dark Matter Revisited

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Dark matter could be a thermal relic comprised of strongly interacting massive particles (SIMPs), where $3 \rightarrow 2$ interactions set the relic abundance. Such interactions generically arise in theories of chiral symmetry breaking via…

High Energy Physics - Phenomenology · Physics 2019-01-08 Yonit Hochberg , Eric Kuflik , Robert McGehee , Hitoshi Murayama , Katelin Schutz

We investigate the neutralino dark matter in the focus point gaugino mediation model with the O(100) GeV gravitino. The thermal relic abundance of the neutralino with a sizable Higgsino fraction can explain the dark matter density at the…

High Energy Physics - Phenomenology · Physics 2015-06-16 Tsutomu T. Yanagida , Norimi Yokozaki

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 a scenario with heavy supersymmetric sfermions and decoupled supersymmetric Higgs sector, a well tempered neutralino is the remaining candidate for thermal single-component sub-TeV dark matter. Well tempered neutralinos are studied in…

High Energy Physics - Phenomenology · Physics 2014-03-26 Archana Anandakrishnan , Kuver Sinha

Dark matter axions form a rethermalizing Bose-Einstein condensate. This provides an opportunity to distinguish axions from other forms of dark matter on observational grounds. I show that if the dark matter is axions, tidal torque theory…

Astrophysics of Galaxies · Physics 2015-05-18 Pierre Sikivie

I summarize some recent work on supersymmetric neutralinos as candidates for cold Dark Matter in the Universe. This includes a new scan of mSUGRA parameter space, with special emphasis on neutralinos annihilating predominantly through…

High Energy Physics - Phenomenology · Physics 2009-11-11 Manuel Drees

Compact stellar objects like supernovae and neutron stars cool by the emission of light particles like neutrinos and axions from their very dense interiors. In this article, we study in detail the photo-production of axions and neutrinos.…

High Energy Physics - Phenomenology · Physics 2024-09-24 Miguel Vanvlasselaer

In the axionic solution of the strong CP problem, fermions which transform under quantum chromodynamics (QCD) are required. In supersymmetry, by equating U(1)_{PQ} with U(1)_R, the natural candidates are the gluinos, as pointed out some…

High Energy Physics - Phenomenology · Physics 2008-11-26 Ernest Ma

In the supersymmetric (SUSY) standard model, the lightest neutralino may be the lightest SUSY particle (LSP), and it is is a candidate of the dark matter in the universe. The LSP dark matter might be produced by the non-thermal process such…

High Energy Physics - Phenomenology · Physics 2009-10-31 J. Hisano , K. Kohri , M. M. Nojiri

Supersymmetric grand unified theories based on the gauge group SO(10) are highly motivated. In the simplest models, one expects t-b-\tau Yukawa coupling unification, in addition to gauge, matter and Higgs unification. Yukawa unification…

High Energy Physics - Phenomenology · Physics 2015-05-18 Howard Baer

We examine the question to what extent prospective detection of dark matter by direct and indirect- detection experiments could shed light on what fraction of dark matter was generated thermally via the freeze-out process in the early…

High Energy Physics - Phenomenology · Physics 2017-10-18 Leszek Roszkowski , Sebastian Trojanowski , Krzysztof Turzynski

Dark matter has been recognized as an essential part of matter for over 70 years now, and many suggestions have been made, what it could be. Most of these ideas have centered on Cold Dark Matter, particles that are predicted in extensions…

Astrophysics · Physics 2016-11-15 Peter L. Biermann , Faustin Munyaneza

Axino as the superpartner of axion that solves the strong CP problem can be a good candidate of dark matter. Inspired by the 3.5 keV X-ray line signal found to be originated from galaxy clusters and Andromeda galaxy, we study axino models…

High Energy Physics - Phenomenology · Physics 2014-06-02 Seng Pei Liew

Both the naturalness of the electroweak symmetry breaking and the resolution of the strong CP problem may require a small Higgsino mass $\mu$ generated by a realization of the DFSZ axion model. Assuming the axino is the lightest…

High Energy Physics - Phenomenology · Physics 2014-10-07 Gabriela Barenboim , Eung Jin Chun , Sunghoon Jung , Wan Il Park

Scenarios with axion-like particles of variable masses, from the milli-eV range to ultralight, can be generated in a natural way in the context of effective field theory models with anomalous $U(1)$ gauge symmetries. They include…

High Energy Physics - Phenomenology · Physics 2020-05-06 Claudio Corianò , Matteo Maria Maglio , Alessandro Tatullo , Dimosthenis Theofilopoulos

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…

High Energy Physics - Phenomenology · Physics 2011-07-18 T. Asaka , T. Yanagida

In supersymmetric theories, the presence of axions usually implies the existence of a non-compact, (pseudo)moduli space. In gauge mediated models, the axion would seem a particularly promising dark matter candidate. The cosmology of the…

High Energy Physics - Theory · Physics 2013-05-29 Linda M. Carpenter , Michael Dine , Guido Festuccia , Lorenzo Ubaldi

The far infrared physics is a fascinating topic for theoretical physics, since the foundation of quantum field theory and neutrinos seem to be strongly related with the far infrared physics of our Universe. In this work we shall explore the…

High Energy Physics - Phenomenology · Physics 2023-09-26 V. K. Oikonomou

Axions might play a crucial role for the solution of the strong CP-problem and explanation of cold dark matter in the universe. In addition they may find applications in the formulation of inflationary models for the early universe and can…

High Energy Physics - Phenomenology · Physics 2012-09-06 Athanasios Chatzistavrakidis , Encieh Erfani , Hans Peter Nilles , Ivonne Zavala

We show that the $\Omega_b - \Omega_{DM}$ coincidence can naturally be explained in a framework where axino cold dark matter is predominantly produced in non-thermal processes involving decays of Q-balls formed in Affleck-Dinebaryogenesis.…

High Energy Physics - Phenomenology · Physics 2008-11-26 Leszek Roszkowski , Osamu Seto