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Related papers: Dark Matter through the Axion Portal

200 papers

Axion-like particles are a well-motivated dark matter candidate that can form a condensate with low momentum and high occupation number. In the presence of dark radiation, this condensate loses energy, naturally increasing the energy…

High Energy Physics - Phenomenology · Physics 2024-09-24 Daniel Aloni , Hengameh Bagherian , Rashmish K. Mishra

Annihilating dark matter (DM) models based on a scalar hidden sector with Higgs portal-like couplings to the Standard Model are considered as a possible explanation for recently observed cosmic ray excesses. Two versions of the model are…

High Energy Physics - Phenomenology · Physics 2015-05-13 Kazunori Kohri , John McDonald , Narendra Sahu

In this paper, we discuss dark matter candidates in a visible heavy QCD axion model. There, a mirror copied sector of the Standard Model with mass scales larger than the Standard Model is introduced. By larger mass scales of the mirrored…

High Energy Physics - Phenomenology · Physics 2017-05-24 Hajime Fukuda , Masahiro Ibe , Tsutomu T. Yanagida

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

All presently known stellar-dynamical constraints on the size and mass of the supermassive compact dark object at the Galactic center are consistent with a ball of self-gravitating, nearly non-interacting, degenerate fermions with mass…

Astrophysics · Physics 2007-05-23 Neven Bilic , Gary B. Tupper , Raoul D. Viollier

Recently, constraints on bosonic asymmetric dark matter have been imposed based on the existence of old neutron stars excluding the dark matter masses in the range from $\sim 2$ keV up to several GeV. The constraints are based on the star…

High Energy Astrophysical Phenomena · Physics 2013-08-09 Chris Kouvaris , Peter Tinyakov

The axion is arguably one of the best motivated candidates for dark matter. For a decay constant greater than about 10^9 GeV, axions are dominantly produced non-thermally in the early universe and hence are "cold", their velocity dispersion…

High Energy Physics - Phenomenology · Physics 2016-12-30 Andreas Ringwald

Axions and axion-like particles are ubiquitous in extensions of the Standard Model and offer a unifying framework for addressing open problems in cosmology. Depending on their mass and interactions, axions can act as dark matter, drive…

High Energy Physics - Phenomenology · Physics 2026-05-01 Luca Visinelli

We propose a simple testable model with mass generation mechanisms for dark matter and neutrino based on the gauged $U(1)_{B-L}$ symmetry and an exact $Z_2$ parity. The $U(1)_{B-L}$ symmetry is spontaneously broken at the TeV scale, by…

High Energy Physics - Phenomenology · Physics 2011-08-08 Shinya Kanemura , Osamu Seto , Takashi Shimomura

We consider a model of dark matter whose most prominent signature is a monochromatic flux of TeV neutrinos from the galactic center. As an example of a general scenario, we consider a specific model where the dark matter is a fermion in the…

High Energy Physics - Phenomenology · Physics 2009-08-14 Adam Falkowski , Jose Juknevich , Jessie Shelton

A Higgs portal dark matter model for explaining the gamma-ray excess from the galactic center can be realized with the extension of local $SU(2)_X$ gauge symmetry with one quadruplet. Due to the residual $Z_3$ discrete symmetry of…

High Energy Physics - Phenomenology · Physics 2016-06-17 Chuan-Hung Chen , Takaaki Nomura

For the experimental search of neutralino dark matter, it is important to know its allowed mass and scattering cross section with the nucleon. In order to figure out how light a neutralino dark matter can be predicted in low energy…

High Energy Physics - Phenomenology · Physics 2011-09-12 Junjie Cao , Ken-ichi Hikasa , Wenyu Wang , Jin Min Yang

A new scheme for lightest supersymmetric particle (LSP) dark matter is introduced and studied in theories of TeV supersymmetry with a QCD axion, $a$, and a high reheat temperature after inflation, $T_R$. A large overproduction of axinos…

High Energy Physics - Phenomenology · Physics 2017-03-20 Raymond T. Co , Francesco D'Eramo , Lawrence J. Hall

Axion as a coherently oscillating scalar field is known to behave as a cold dark matter in all cosmologically relevant scales. For conventional axion mass with 10^{-5} eV, the axion reveals a characteristic damping behavior in the evolution…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-05 Chan-Gyung Park , Jai-chan Hwang , Hyerim Noh

A TeV scale decaying dark matter chiral multiplet N is introduced in addition to the minimal supersymmetric standard model(MSSM). For a calculable abundance of N, we introduce heavy axino decaying to N and MSSM particles including the…

High Energy Physics - Phenomenology · Physics 2009-10-29 Ji-Haeng Huh , Jihn E. Kim

Asymmetric dark matter is a well-motivated approach to explain the apparent coincidence between the relic densities of visible and dark matter, $\Omega_D \simeq 5.4\Omega_b$. A complete explanation requires two components, a relation…

High Energy Physics - Phenomenology · Physics 2026-03-04 Peter Cox , Rafael E. Pérez , Raymond R. Volkas

In the context of Twin Higgs models, we study a simple mechanism that simultaneously generates asymmetries in the dark and visible sector through the out-of-equilibrium decay of a TeV scale particle charged under a combination of baryon and…

High Energy Physics - Phenomenology · Physics 2016-08-24 Marco Farina , Angelo Monteux , Chang Sub Shin

In split supersymmetry, gauginos and Higgsinos are the only supersymmetric particles which are possibly accessible at foreseeable colliders. While the direct experimental searches, such as LEP and Tevatron experiments, gave robust lower…

High Energy Physics - Phenomenology · Physics 2009-01-07 Fei Wang , Wenyu Wang , Jin Min Yang

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…

High Energy Physics - Phenomenology · Physics 2023-02-16 Luca Di Luzio , Belen Gavela , Pablo Quilez , Andreas Ringwald

In this paper, we propose a bubble filtering-out mechanism for an asymmetric dark matter scenario during the Peccei-Quinn (PQ) phase transition. Based on a QCD axion model, extended by extra chiral neutrinos, we show that the PQ phase…

High Energy Physics - Phenomenology · Physics 2021-10-19 M. Ahmadvand