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Preferred axion models are minimal realizations of the Peccei-Quinn solution to the strong CP problem while providing a dark matter candidate. These models invoke new heavy quarks that interact strongly with the Standard Model bringing them…

高能物理 - 唯象学 · 物理学 2025-03-26 Andrew Cheek , Ui Min

Gravity-mediated SUSY breaking models with R-parity conservation give rise to dark matter in the universe. I review neutralino dark matter in the minimal supergravity model (mSUGRA), models with non-universal soft SUSY breaking terms…

高能物理 - 唯象学 · 物理学 2015-05-13 Howard Baer

We introduce a mechanism for multi-component dark matter (DM) that originates from axion mixing and present some of its defining properties. In this context, multi-component DM implies that the cold DM is composed of the QCD axion and many…

高能物理 - 唯象学 · 物理学 2025-12-30 Hai-Jun Li

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…

高能物理 - 唯象学 · 物理学 2016-07-27 Howard Baer

Although the standard {\Lambda}CDM model describes the cosmic microwave background radiation and the large scale structure of the Universe with great success, it has some tensions with observations in the effective number of neutrino…

高能物理 - 唯象学 · 物理学 2012-11-26 Kiwoon Choi , Ki-Young Choi , Chang Sub Shin

We study a specific SUGRA model with nonuniversal gaugino masses as an alternative to the minimal SUGRA model in the context of supersymmetric dark matter. The lightest supersymmetric particle in this model comes out to be a Higgsino…

高能物理 - 唯象学 · 物理学 2009-11-10 Utpal Chattopadhyay , D. P. Roy

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

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

Phenomenologically viable and interesting regions of parameter space in the minimal super-gravity (mSUGRA) model with small $m_0$ and small $m_{1/2}$ consistent with the WMAP data on dark matter relic density and the bound on the mass of…

高能物理 - 唯象学 · 物理学 2008-11-26 Utpal Chattopadhyay , Debottam Das , Amitava Datta , Sujoy Poddar

We examine mixed axion/neutralino cold dark matter production in the SUSY DFSZ axion model where an axion superfield couples to Higgs superfields. We calculate a wide array of axino and saxion decay modes along with their decay…

高能物理 - 唯象学 · 物理学 2015-06-17 Kyu Jung Bae , Howard Baer , Eung Jin Chun

Recent cosmological data allow to determine the universal Dark Matter (DM) density to a precision of about 10%, if a simple, well-motivated ansatz for the spectrum of primordial density perturbations is correct. Not surprisingly, a thermal…

高能物理 - 唯象学 · 物理学 2007-05-23 Manuel Drees

The requirement that the lightest neutralino $\tilde\chi_1^0$ has the right thermal relic density to explain all Dark Matter in the universe strongly constrains the parameter space of supersymmetric models in general, and of the mSUGRA…

高能物理 - 唯象学 · 物理学 2009-11-11 Abdelhak Djouadi , Manuel Drees , Jean-Loic Kneur

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…

高能物理 - 唯象学 · 物理学 2015-04-20 Kyu Jung Bae , Howard Baer , Eung Jin Chun , Chang Sub Shin

The recent observations imply that there is an extra relativistic degree of freedom coined dark radiation. We argue that the QCD axion is a plausible candidate for the dark radiation, not only because of its extremely small mass, but also…

高能物理 - 唯象学 · 物理学 2015-06-03 Kwang Sik Jeong , Fuminobu Takahashi

The properties of axions that constitute 100% of cold dark matter (CDM) depend on the tensor-to-scalar ratio $r$ at the end of inflation. If $r=0.20^{+0.07}_{-0.05}$ as reported by the BICEP2 collaboration, then "half" of the CDM axion…

高能物理 - 唯象学 · 物理学 2014-07-09 L. Visinelli , P. Gondolo

In minimal Supergravity (mSUGRA) models the lightest supersymmetric particle (assumed to be the lightest neutralino) provides an excellent cold dark matter (CDM) candidate. The supersymmetric parameter space is significantly reduced, if the…

高能物理 - 唯象学 · 物理学 2009-11-11 Luisa Sabrina Stark , Petra Hafliger , Adrian Biland , Felicitas Pauss

We present brief synopses of supersymmetric models where either the neutralino composition or its mass is adjusted so that thermal relic neutralinos from the Big Bang saturate the measured abundance of cold dark matter in the universe. We…

高能物理 - 唯象学 · 物理学 2009-01-06 Howard Baer , Azar Mustafayev , Eun-Kyung Park , Xerxes Tata

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 perform a Bayesian model selection analysis in the the R-parity conserving MSSM to compare two different assumptions: whether the lightest neutralinos make all or only part of the cold dark matter. This corresponds to either imposing…

高能物理 - 唯象学 · 物理学 2011-06-07 S. S. AbdusSalam , F. Quevedo

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