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We study a new physics scenario with two inert and one active scalar doublets, hence a 3-Higgs Doublet Model (3HDM). We impose a $Z_2 \times Z'_2$ symmetry onto such a 3HDM with one inert doublet odd under the $Z_2$ transformation and the…

高能物理 - 唯象学 · 物理学 2023-03-29 Jaime Hernandez-Sanchez , Venus Keus , Stefano Moretti , Dorota Sokolowska

The inert doublet model (IDM) is a minimal extension of the Standard Model (SM) that can account for the dark matter in the universe. Naturalness arguments motivate us to study whether the model can be embedded into a theory with…

高能物理 - 唯象学 · 物理学 2015-09-29 Alexis D. Plascencia

We study the inert triplet models, in which the standard model (SM) is extended to have a new SU(2)L triplet scalar (Y=0 or 2) with an Z2 symmetry. We show that the neutral component of the triplet can be a good dark matter candidate. In…

高能物理 - 唯象学 · 物理学 2011-05-10 Takeshi Araki , C. Q. Geng , Keiko I. Nagao

We propose a minimal extension of the Standard Model to accommodate two-component dark matter (DM) and light neutrino mass. The symmetry of the Standard Model is enhanced by an unbroken $\mathbb{Z}_2 \times \mathbb{Z}'_2$ such that being…

高能物理 - 唯象学 · 物理学 2019-09-25 Debasish Borah , Rishav Roshan , Arunansu Sil

Scalar field dynamics may give rise to a nonzero cosmological variation of fundamental constants. Within different scenarios based on the unification of gauge couplings, the various claimed observations and bounds may be combined in order…

高能物理 - 唯象学 · 物理学 2010-04-21 Thomas Dent , Steffen Stern , Christof Wetterich

We investigate a two-component dark matter scenario in the type-I two-Higgs-doublet model. The dark sector contains a real scalar $s$ and a Dirac fermion $\chi$, whose stability is ensured by a $Z_4$ symmetry together with kinematic…

高能物理 - 唯象学 · 物理学 2026-03-20 Patricio Escalona , Jacinto P. Neto , M. J. Neves , Camila Ramos , David Suarez

Coupled dark matter-dark energy systems can suffer from non-adiabatic instabilities at early times and large scales. In these proceedings, we consider two parameterizations of the dark sector interaction. In the first one the…

宇宙学与河外天体物理 · 物理学 2014-11-20 L. Lopez Honorez , 0. Mena

We construct a class of scalar field models coupled to matter that lead to the dependence of masses and coupling constants on the ambient matter density. Such models predict a deviation of couplings measured on the Earth from values…

高能物理 - 唯象学 · 物理学 2008-11-26 Keith A. Olive , Maxim Pospelov

We investigate the matter density perturbation $\delta_m$ and power spectrum $P(k)$ in the running vacuum model (RVM) with the cosmological constant being a function of the Hubble parameter, given by $\Lambda = \Lambda_0 + 6 \sigma H H_0+…

宇宙学与河外天体物理 · 物理学 2016-11-09 Chao-Qiang Geng , Chung-Chi Lee

We consider a self-interacting dark matter model in which the massive dark photon mediating the self-interaction decays to light dark fermions to avoid over-closing the universe. We find that if the model is constrained to explain the dark…

高能物理 - 唯象学 · 物理学 2019-07-05 Ran Huo , Manoj Kaplinghat , Zhen Pan , Hai-Bo Yu

We show that decoupled hidden sectors can have observational consequences. As a representative model example, we study dark matter production in the Higgs portal model with one real singlet scalar $s$ coupled to the Standard Model Higgs via…

宇宙学与河外天体物理 · 物理学 2016-11-16 Matti Heikinheimo , Tommi Tenkanen , Kimmo Tuominen , Ville Vaskonen

We study the fluctuations in the brightness temperature of 21-cm signal $\delta T_{21}$ at the dark ages ($z\sim100$) with a dark matter candidate in Inter Doublet Model (IDM). We then explore the effects of different fractions of IDM dark…

宇宙学与河外天体物理 · 物理学 2021-09-22 Rupa Basu , Madhurima Pandey , Debasish Majumdar , Shibaji Banerjee

Thermal freeze-out is a prominent example of dark matter (DM) production mechanism in the early Universe that can yield the correct relic density of stable weakly interacting massive particles (WIMPs). At the other end of the mass scale,…

高能物理 - 唯象学 · 物理学 2020-08-05 Sebastian Trojanowski , Philippe Brax , Carsten van de Bruck

In this work, we study two scalar field driven dark energy models characterized by the axion potential and the inverse power law potential, each coupled to dark matter through a momentum exchange interaction. By formulating the dynamics as…

宇宙学与河外天体物理 · 物理学 2025-06-27 Prasanta Sahoo , Nandan Roy , Himadri Shekhar Mondal

We study the minimally and non-minimally coupled scalar field models as possible alternatives for dark energy, the mysterious energy component that is driving the accelerated expansion of the universe. After discussing the dynamics at both…

广义相对论与量子宇宙学 · 物理学 2019-12-03 Zahra Davari , Valerio Marra , Mohammad Malekjani

In this work, we consider an extension of the Standard Model (SM) with an inert Higgs doublet and a real scalar singlet, in order to address problems around the origin of dark matter (DM). In this model, the lightest among the CP-odd and…

高能物理 - 唯象学 · 物理学 2022-11-17 Mohammed Omer Khojali , Ammar Abdalgabar , Amine Ahriche , Alan S. Cornell

We investigate a string-inspired dark energy scenario featuring a scalar field with a coupling to the Gauss-Bonnet invariant. Such coupling can trigger the onset of late dark energy domination after a scaling matter era. The universe may…

高能物理 - 理论 · 物理学 2008-11-26 Tomi Koivisto , David F. Mota

The Inert Doublet Model is an extension of the Standard Model including one extra ``Inert scalar doublet'' and an exact $Z_2$ symmetry. The ``Inert scalar'' provides a new candidate for dark matter. We present a systematic analysis of the…

高能物理 - 唯象学 · 物理学 2007-06-04 Laura Lopez Honorez

In this work we analyze the full linear behaviour of the constrained interacting dark energy (CIDER) model, which is a conformally coupled quintessence model tailored to mimic a $\Lambda$CDM expansion. We compute the matter and temperature…

宇宙学与河外天体物理 · 物理学 2023-01-18 Bruno J. Barros , Diogo Castelão , Vitor da Fonseca , Tiago Barreiro , Nelson J. Nunes , Ismael Tereno

The dynamics of expansion of the Universe and evolution of scalar perturbations are studied for the quintessential scalar fields $Q$ with the classical Lagrangian satisfying the additional condition $w=const$ or $c^2_a=0$. Both…

天体物理学 · 物理学 2009-08-10 B. Novosyadlyj , O. Sergijenko