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相关论文: Models for SIMP dark matter and dark photon

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Dark $Z$/dark photon ($Z'$) is one candidate of dark force carrier, which helps to interpret the properties of dark matter (DM). Other than traditional studies of DM including direct detection, indirect detection and collider simulation, in…

高能物理 - 唯象学 · 物理学 2015-07-06 Fanrong Xu

We discuss a QCD-scale composite axion model arising from dark QCD coupled to QCD. The presently proposed scenario not only solves the strong CP problem, but also is compatible with the preheating setup for the QCD baryogenesis. The…

高能物理 - 唯象学 · 物理学 2024-09-26 Bin Wang , Shinya Matsuzaki , Hiroyuki Ishida

A $SU(2)_D \times U(1)_D$ gauge-Higgs sector, an exact dark copy of the Standard Model (SM) one, is proposed. It is demonstrated that the dark gauge bosons ${\cal W}^{(p,m)}$, in analogous to the SM $W^\pm$, can fulfill the role as a…

高能物理 - 唯象学 · 物理学 2023-12-19 Van Que Tran , Thong T. Q. Nguyen , Tzu-Chiang Yuan

Well known scaling laws among the structural properties of the dark and the luminous matter in disc systems are too complex to be arisen by two inert components that just share the same gravitational field. This brings us to critically…

星系天体物理 · 物理学 2020-03-10 Paolo Salucci , Nicola Turini

While the paradigm of a weakly interacting massive particle (WIMP) has guided our search strategies for dark matter in the past decades, their null-results have stimulated growing interest in alternative explanations pointing towards…

高能物理 - 唯象学 · 物理学 2018-05-22 Jan Heisig

Loops of portal matter (PM) fields carrying both dark and Standard Model (SM) quantum numbers can lead to the kinetic mixing (KM) of the SM photon and the analogous dark photon (DP) of a phenomenologically interesting magnitude. However, in…

高能物理 - 唯象学 · 物理学 2026-03-12 Thomas G. Rizzo

A hidden sector that kinetically mixes with the Minimal Supersymmetric Standard Model provides simple and well-motivated dark matter candidates that possess many of the properties of a traditional weakly interacting massive particle (WIMP).…

高能物理 - 唯象学 · 物理学 2020-10-21 Patrick Barnes , Zachary Johnson , Aaron Pierce , Bibhushan Shakya

We briefly review some recent Cold Dark Matter (CDM) models. Our main focus are charge symmetric models of WIMPs which are not the standard SUSY LSP's (Lightest Supersymmetric Partners). We indicate which experiments are most sensitive to…

高能物理 - 唯象学 · 物理学 2009-10-29 Shmuel Nussinov

Well known scaling laws among the structural properties of the dark and the luminous matter in disc systems are too complex to be arisen by two inert components that just share the same gravitational field. This brings us to critically…

宇宙学与河外天体物理 · 物理学 2020-08-28 Paolo Salucci , Nicola Turini , Chiara Di Paolo

The regime of dark matter (DM) freeze-in at stronger coupling interpolates between freeze-in and freeze-out. It relies on Boltzmann-suppressed dark matter production, implying that the Standard Model bath temperature never exceeds the dark…

高能物理 - 唯象学 · 物理学 2024-04-09 Niko Koivunen , Oleg Lebedev , Martti Raidal

We study a model of dark matter in which the hidden sector interacts with standard model particles via a hidden photonic portal. We investigate the effects of this new interaction on the hydrogen atom, including the Stark, Zeeman and…

高能物理 - 唯象学 · 物理学 2015-12-11 S. A. Alavi , F. S. Kazemian

We study production of self-interacting dark matter (DM) during an early matter-dominated phase. As a benchmark scenario, we consider a model where the DM consists of singlet scalar particles coupled to the visible Standard Model (SM)…

高能物理 - 唯象学 · 物理学 2019-02-20 Nicolás Bernal , Catarina Cosme , Tommi Tenkanen

In this talk, I describe a class of electroweak (EW) scale dark matter (DM) models where its stability or longevity are the results of underlying dark gauge symmetries: stable due to unbroken local dark gauge symmetry or topology, or…

高能物理 - 唯象学 · 物理学 2016-05-03 P. Ko

We study the scattering of two identical pNGBs (pseudo-Nambu-Goldstone Bosons) in Sp(4) gauge theory with two mass-degenerate Dirac fermions in the pseudo-real fundamental representation. This theory serves as a realization of a SIMP…

高能物理 - 格点 · 物理学 2025-01-31 Yannick Dengler , Axel Maas , Fabian Zierler

We study the imprints of secluded dark sectors with a mass gap and self-interactions on the matter power spectrum. When Dark Matter (DM) is sufficiently light, in the ballpark of a few KeV, and self-interacting we find qualitative…

高能物理 - 唯象学 · 物理学 2022-08-31 Raghuveer Garani , Michele Redi , Andrea Tesi

We consider the possibility that dark matter can communicate with the Standard Model fields via flavor interactions. We take the dark matter to belong to a "dark sector" which contains at least two types, or "flavors", of particles and then…

高能物理 - 唯象学 · 物理学 2011-09-15 Jennifer Kile , Amarjit Soni

A simple extension of the Standard Model (SM) that provides an explicit realization of the dark-matter (DM) neutrino-portal paradigm is presented. The leading interactions between the dark sector, containing scalars and relic fermions, and…

高能物理 - 唯象学 · 物理学 2016-11-23 Vannia González-Macías , José Illana , José Wudka

We present a realistic, simple and natural model of strongly-interacting dark matter based on the neutrino-portal paradigm. The strong interactions at small velocities are generated by the exchange of dark photons, and produce the observed…

高能物理 - 唯象学 · 物理学 2021-01-20 J. M. Lamprea , E. Peinado , S. Smolenski , J. Wudka

We propose a new mechanism where asymmetric dark matter (ADM) and the baryon asymmetry are both generated in the same decay chain of a metastable weakly interacting massive particle (WIMP) after its thermal freeze-out. Dark matter and…

高能物理 - 唯象学 · 物理学 2020-12-11 Yanou Cui , Michael Shamma

We investigate a model in which Dark Matter is stabilized by means of a Z2 parity that results from the same non-abelian discrete flavor symmetry which accounts for the observed pattern of neutrino mixing. In our A4 example the standard…

高能物理 - 唯象学 · 物理学 2015-03-17 M. S. Boucenna , M. Hirsch , S. Morisi , E. Peinado , M. Taoso , J. W. F. Valle