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相关论文: Mainly axion cold dark matter in the minimal super…

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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…

高能物理 - 唯象学 · 物理学 2014-11-20 Howard Baer , Radovan Dermisek , Shibi Rajagopalan , Heaya Summy

SUSY/SUGRA models with naturalness defined via small $\mu$ are constrained due to experiment on the relic density and the experimental limits on the WIMP-proton cross-section and WIMP annihilation cross-section from indirect detection…

高能物理 - 唯象学 · 物理学 2020-05-20 Amin Aboubrahim , Wan-Zhe Feng , Pran Nath

Recent analyses of WMAP9 data show that dark radiation-- parametrized by the apparent number of additional neutrinos \Delta N_{eff} contributing to the cosmic expansion-- is consistent with the Standard Model and bounded from above by about…

高能物理 - 唯象学 · 物理学 2015-06-12 Kyu Jung Bae , Howard Baer , Andre Lessa

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

We compute the dark matter relic densities of neutralinos and axions in a supersymmetric model with a gauged anomalous U(1) symmetry, kinetically mixed with $U(1)_Y$ of hypercharge. The model is a variant of the USSM (the U(1) extended…

高能物理 - 唯象学 · 物理学 2015-05-20 Claudio Coriano , Marco Guzzi , Antonio Mariano

I give a short overview on some of the favorite particle Cold Dark Matter candidates today, focusing on those having detectable interactions: the axion, the KK-photon in Universal Extra Dimensions, the heavy photon in Little Higgs and the…

高能物理 - 唯象学 · 物理学 2008-11-26 Stefano Scopel

We study the experimental constraints on a model of a two-component dark matter, consisting of the QCD axion, and a scalar particle, both contributing to the dark matter relic abundance of the Universe. The global Peccei-Quinn symmetry of…

高能物理 - 唯象学 · 物理学 2020-02-28 Suman Chatterjee , Anirban Das , Tousik Samui , Manibrata Sen

A detailed analysis of dark matter event rates in minimal supergravity models (MSGM) is given. It is shown analytically that the lightest neutralino the ${{\tilde {Z}_{1}}}$ is the LSP over almost all of the parameter space, and hence the…

高能物理 - 唯象学 · 物理学 2008-11-26 R. Arnowitt , Pran Nath

We consider Higgsino-like dark matter (DM) in the Minimal Supersymmetric Standard Model (MSSM) with additional right-handed neutrino chiral superfields, and propose a new non-thermal way of generating the right amount of relic DM via…

高能物理 - 唯象学 · 物理学 2017-05-15 Anibal D. Medina

To elucidate the composition of dark matter (DM) is one of the most important open questions in particle and astroparticle phenomenology. Within the framework of minimal supersymmetric extensions of the standard model of fundamental…

高能物理 - 唯象学 · 物理学 2020-04-03 Andres D. Perez

We explore a KSVZ-like extension of the Standard Model with a Dirac fermion and three right-handed neutrinos. PQ symmetry allows the Dirac mass for neutrinos and prevents the Majorana mass. A $\mathcal{Z}_2$ symmetry guarantees the…

高能物理 - 唯象学 · 物理学 2025-07-16 Shivam Gola

We show that dark matter can be accounted for by an axion that solves the strong CP problem, but is much lighter than usual due to a $Z_\mathcal{N}$ symmetry. The whole mass range from the canonical QCD axion down to the ultra-light regime…

高能物理 - 唯象学 · 物理学 2023-02-16 Luca Di Luzio , Belen Gavela , Pablo Quilez , Andreas Ringwald

There appear to be three challenges that any theory of dark matter must face: (i) why is $\Omega_{DM}$ of the same order as $\Omega_{Baryons}$ ? (ii) what are the near solar mass objects ($\sim 0.5 M_{\odot}$) observed by the MACHO…

天体物理学 · 物理学 2016-11-03 R. N. Mohapatra , V. L. Teplitz

The combination of new cosmic microwave background data with cosmological priors has determined the physical cold dark matter (cdm) density to be $\Omega_{\rm cdm} h^2 = 0.13\pm0.01$. We find the corresponding regions of parameters in the…

高能物理 - 唯象学 · 物理学 2008-11-26 Vernon Barger , Chung Kao

We perform a study of the dark matter candidates of a constrained version of the minimal R-parity-conserving supersymmetric model with a gauged $U(1)_{B-L}$. It turns out that there are four additional candidates for dark matter in…

高能物理 - 唯象学 · 物理学 2015-06-05 Lorenzo Basso , Ben O'Leary , Werner Porod , Florian Staub

{\tenrm The possibility of detecting supersymmetric dark matter is examined within the framework of the minimal supergravity model (MSGM), where the $\tilde{Z}_{1}$ is the LSP for almost the entire parameter space. A brief discussion is…

高能物理 - 唯象学 · 物理学 2009-09-25 R. Arnowitt , Pran Nath

A major fraction of the mass content of the universe is composed of dark matter (DM), i.e. particles not interacting significantly with electromagnetic radiation, with ordinary matter or self-interacting (cold dark matter). The axion is…

高能物理 - 实验 · 物理学 2018-12-12 Woohyun Chung

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

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

The cosmological scenario where the Peccei-Quinn symmetry is broken after inflation is investigated. In this scenario, topological defects such as strings and domain walls produce a large number of axions, which contribute to the cold dark…

高能物理 - 唯象学 · 物理学 2015-08-12 Masahiro Kawasaki , Ken'ichi Saikawa , Toyokazu Sekiguchi