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Several models of dark matter motivate the concept of hidden sectors consisting of SU(3)_C x SU(2)_L x U(1)_Y singlet fields. The interaction between our and hidden matter could be transmitted by new abelian U'(1) gauge bosons A' mixing…

高能物理 - 唯象学 · 物理学 2012-06-22 S. N. Gninenko

We study a lepton portal dark matter model, motivated by the deviation of the $W$ boson mass reported by the CDF collaboration. We introduce vector-like leptons and a scalar dark matter (DM) which exclusively couples to the extra leptons…

高能物理 - 唯象学 · 物理学 2022-07-20 Junichiro Kawamura , Shohei Okawa , Yuji Omura

SO(10) grand unified theories can ensure the stability of new particles in terms of the gauge group structure itself, and in this respect are well suited to accommodate dark matter (DM) candidates in the form of new stable massive…

高能物理 - 唯象学 · 物理学 2016-03-23 Sofiane M. Boucenna , Martin B. Krauss , Enrico Nardi

We revisit the Higgs portal vector dark matter model including a hidden sector Higgs field that generates the mass of the vector dark matter. The model becomes renormalizable and has two scalar bosons, the mixtures of the standard model…

高能物理 - 唯象学 · 物理学 2015-06-12 Seungwon Baek , P. Ko , Wan-Il Park , Eibun Senaha

In this analysis we demonstrate the freeze-in realization of a non-abelian vector boson dark matter (DM). We choose to elaborate an existing $SU(2)_N$ extension ($N$ stands for neutral) of the Standard Model (SM) with an additional…

高能物理 - 唯象学 · 物理学 2020-03-04 Basabendu Barman , Subhaditya Bhattacharya , Mohammadreza Zakeri

Light vector fields during inflation obtain a superhorizon perturbation spectrum when their conformal invariance is appropriately broken. Such perturbations, by means of some suitable mechanism (e.g. the vector curvaton mechanism), can…

高能物理 - 唯象学 · 物理学 2015-06-16 Juan C. Bueno Sanchez , Konstantinos Dimopoulos

We provide a simple model of vector dark matter (DM) which can realize the recently proposed freeze-out mechanism with catalyzed annihilation. In our setup, a vector DM field $X_\mu$ and a catalyst field $C_\mu$ is unified by an SU(2)$_D$…

高能物理 - 唯象学 · 物理学 2022-01-24 Chengfeng Cai , Hong-Hao Zhang

We consider a dark sector scenario with two dark matter species with opposite dark $U(1)$ charges and an asymmetric population comprising some fraction of the dark matter abundance. A new mechanism for boosting dark matter is introduced,…

高能物理 - 唯象学 · 物理学 2023-05-02 Michael Geller , Zamir Heller-Algazi

We propose a minimal setup that realises dynamical inflection point inflation, and, using the same field content, generates neutrino masses, a baryon asymmetry of the universe, and dark matter. A dark $SU(2)_D$ gauge sector with a dark…

高能物理 - 唯象学 · 物理学 2024-02-15 Debasish Borah , Arnab Dasgupta , Daniel Stolarski

Current techniques cannot detect axion dark matter over much of its parameter space, particularly in the theoretically well-motivated region where the axion decay constant f_a lies near the GUT and Planck scales. We suggest a novel…

高能物理 - 唯象学 · 物理学 2011-10-03 Peter W. Graham , Surjeet Rajendran

Superheavy dark matter has been attractive as a candidate of particle dark matter. We propose a ``natural" particle model, in which the dark matter serves as the inflaton in natural inflation, while decaying to high-energy particles at…

高能物理 - 唯象学 · 物理学 2025-12-03 Kohta Murase , Yuma Narita , Wen Yin

The origin of non-baryonic Dark Matter remains elusive despite ongoing sensitive searches for heavy, thermally produced dark matter particles. Recently, it has been shown, that non-thermally produced vector bosons (sometimes called hidden…

高能物理 - 实验 · 物理学 2019-10-09 Le Hoang Nguyen , Andrei Lobanov , Dieter Horns

We propose a new mechanism to produce axion dark matter from inflationary fluctuations. Quantum fluctuations during inflation are strengthened by a coupling of the axion kinetic term to the inflaton, which we parametrize as an effective…

高能物理 - 唯象学 · 物理学 2024-03-18 Ameen Ismail , Seung J. Lee , Bingrong Yu

Dark matter with mass below about a GeV is essentially unobservable in conventional direct detection experiments. However, newly proposed technology will allow the detection of single electron events in semiconductor materials with…

高能物理 - 唯象学 · 物理学 2012-11-13 Peter W. Graham , David E. Kaplan , Surjeet Rajendran , Matthew T. Walters

We propose a vector dark matter model with an exotic dark SU(2) gauge group. Two Higgs triplets are introduced to spontaneously break the symmetry. All of the dark gauge bosons become massive, and the lightest one is a viable vector DM…

高能物理 - 唯象学 · 物理学 2021-07-28 Zexi Hu , Chengfeng Cai , Yi-Lei Tang , Zhao-Huan Yu , Hong-Hao Zhang

If cosmic inflation was driven by an electrically neutral scalar field stable on cosmological time scales, the field necessarily constitutes all or part of dark matter (DM). We study this possibility in a scenario where the inflaton field…

高能物理 - 唯象学 · 物理学 2019-03-13 Juan P. Beltrán Almeida , Nicolás Bernal , Javier Rubio , Tommi Tenkanen

A light hidden photon or axion-like particle is a good dark matter candidate and they are often associated with the spontaneous breaking of dark global or gauged U(1) symmetry. We consider the dark Higgs dynamics around the phase transition…

高能物理 - 唯象学 · 物理学 2021-10-27 Kazunori Nakayama , Wen Yin

Vector boson fusion (VBF) processes at the Large Hadron Collider (LHC) provide a unique opportunity to search for new physics with electroweak couplings. Two studies are presented: (i) A search of supersymmetric dark matter in the final…

Bosonic superweakly interacting massive particles (super-WIMPs) are a candidate for warm dark matter. With the absorption of such a boson by a xenon atom these dark matter candidates would deposit an energy equivalent to their rest mass in…

A natural possibility for dark matter is that it is composed of the stable pions of a QCD-like hidden sector. Existing literature largely assumes that pion self-interactions alone control the early universe cosmology. We point out that…

高能物理 - 唯象学 · 物理学 2018-04-19 Asher Berlin , Nikita Blinov , Stefania Gori , Philip Schuster , Natalia Toro