中文
相关论文

相关论文: FIMP Dark Matter in Clockwork/Linear Dilaton Extra…

200 篇论文

We propose an experiment to search for ultralight scalar dark matter (DM) with dilatonic interactions. Such couplings can arise for the dilaton as well as for moduli and axion-like particles in the presence of CP violation. Ultralight…

高能物理 - 唯象学 · 物理学 2015-02-03 Asimina Arvanitaki , Junwu Huang , Ken Van Tilburg

Although it is usually thought that a class of weakly interacting massive particle (WIMP) dark matters (DMs), which have the vector coupling with the $Z$ boson, is denied by null results of the direct DM searches, such WIMP DMs are still…

高能物理 - 唯象学 · 物理学 2021-08-10 Nobuchika Okada , Osamu Seto

A strongly interacting massive particle (SIMP) is an interesting candidate for dark matter (DM) because its self-interaction cross section can be naturally strong enough to address the astrophysical problem of small-scale structure…

高能物理 - 唯象学 · 物理学 2020-10-14 Ayuki Kamada , Masaki Yamada , Tsutomu T. Yanagida

The tightening of the constraints on the standard thermal WIMP scenario has forced physicists to propose alternative dark matter (DM) models. One of the most popular alternate explanations of the origin of DM is the non-thermal production…

高能物理 - 唯象学 · 物理学 2017-02-27 Anirban Biswas , Sandhya Choubey , Sarif Khan

The existence of Dark Matter (DM) has been well established from various cosmological and astrophysical evidences. However, the particle properties of DM are largely undetermined and attempts to probe its interactions with the Standard…

高能物理 - 唯象学 · 物理学 2018-12-26 Nicolás Bernal , Arindam Chatterjee , Arnab Paul

In this paper, we construct the first asymmetric strongly interacting massive particles (SIMP) dark matter (DM) model, where a new vector-like fermion and a new complex scalar both having nonzero chemical potentials can be asymmetric DM…

高能物理 - 唯象学 · 物理学 2022-10-31 Shu-Yu Ho

We investigate the phenomenology of a non-thermal dark matter (DM) candidate in the context of flavor models that explain the hierarchy in the masses and mixings of quarks and leptons via the Froggatt-Nielsen (FN) mechanism. A…

高能物理 - 唯象学 · 物理学 2023-08-02 K. S. Babu , Shreyashi Chakdar , Nandini Das , Dilip Kumar Ghosh , Purusottam Ghosh

We consider simplified dark matter models (DM) interacting gravitationally with the standard model (SM) particles in a Randall-Sundrum (RS) framework. In this framework, the DM particles interact through the exchange of spin-2 Kaluza-Klein…

高能物理 - 唯象学 · 物理学 2019-10-07 Ashok Goyal , Rashidul Islam , Mukesh Kumar

A feebly interacting massive particle (FIMP), contrasting with a weakly interacting massive particle (WIMP), is an intriguing dark matter (DM) candidate. Light (keV-scale) FIMP DM is of particular interest: its radiative decay leaves a line…

高能物理 - 唯象学 · 物理学 2020-01-31 Ayuki Kamada , Keisuke Yanagi

We study the spin-dependence of Dark Matter (DM) particles which interact gravitationally with the Standard Model (SM) in an extra-dimensional Randall-Sundrum scenario. We assume that both the Dark Matter and the Standard Model are confined…

高能物理 - 唯象学 · 物理学 2021-03-12 Miguel G. Folgado , Andrea Donini , Nuria Rius

One of the most puzzling problems of modern physics is the identification of the nature a non-relativistic matter component present in the universe, contributing to more than 25$\%$ of the total energy budget, known as Dark Matter. Weakly…

高能物理 - 唯象学 · 物理学 2019-01-18 Mathias Pierre

In this paper, we investigate the possibility of testing the weakly interacting massive particle (WIMP) dark matter (DM) models by applying the simplest phenomenological model which introduces an interaction term between dark energy (DE)…

宇宙学与河外天体物理 · 物理学 2021-09-15 Wei Cheng , Yuan He , Jin-Wang Diao , Yu Pan , Jun Zeng , Jia-Wei Zhang

Strongly interacting massive particle (SIMP) has become one of the promising dark matter (DM) candidates due to its capability of addressing the small-scale anomaly, where the final DM abundance is set via the freeze-out of $3\rightarrow 2$…

高能物理 - 唯象学 · 物理学 2024-10-08 Debtosh Chowdhury , Sudipta Show

In this paper, we construct for the first time a two-component strongly interacting massive particles (SIMP) dark matter (DM) model, where a complex scalar and a vector-like fermion play the role of the SIMP DM candidates. These two…

高能物理 - 唯象学 · 物理学 2022-03-04 Shu-Yu Ho , Pyungwon Ko , Chih-Ting Lu

Feebly Interacting Massive Particles (FIMPs) are dark matter candidates that never thermalize in the early universe and whose production takes place via decays and/or scatterings of thermal bath particles. If FIMPs interactions with the…

高能物理 - 唯象学 · 物理学 2021-10-15 Francesco D'Eramo , Alessandro Lenoci

In this paper, we construct a viable model for a GeV scale self-interacting dark matter (DM), where the DM was thermally produced in the early universe. Here, a new vector-like fermion with a dark charge under the $U(1)_{D}$ gauge symmetry…

高能物理 - 唯象学 · 物理学 2024-04-24 Shu-Yu Ho , Pyungwon Ko , Dibyendu Nanda

The dynamics and detection possibility of a pseudo-FIMP (pFIMP) dark matter (DM) in the presence of a thermal DM have been studied in different contexts. The pFIMP phenomenology largely depends on the WIMP-like partner DM, as pFIMP…

高能物理 - 唯象学 · 物理学 2025-08-07 Jayita Lahiri , Dipankar Pradhan , Abhik Sarkar

Pseudo-feebly Interacting Massive Particle (pFIMP) has been postulated in two component dark matter (DM) scenarios, where it has feeble interaction with the visible sector, but sizeable one with a thermal bath partner. In this work, we…

高能物理 - 唯象学 · 物理学 2024-11-25 Subhaditya Bhattacharya , Dipankar Pradhan , Jahaan Thakkar

If the dark matter (DM) consists of a weakly interacting massive particle (WIMP), it can be produced and studied at future collider experiments like those at the LHC. The production of collider-stable WIMPs is characterized by hard…

高能物理 - 唯象学 · 物理学 2009-07-15 Spencer Chang , Andre de Gouvea

In the context of a simplified leptophilic Dark Matter (DM) scenario where the mediator is a new charged fermion carrying leptonic quantum number and the DM candidate is either scalar or vector, the complementarity of different bounds is…

高能物理 - 唯象学 · 物理学 2018-04-11 D. Barducci , A. Deandrea , S. Moretti , L. Panizzi , H. Prager