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相关论文: Effective Theory of Freeze-in Dark Matter

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Dark matter (DM) that interacts too weakly with the Standard Model (SM) to reach full thermodynamic equilibrium can be still be created in significant amounts by rare SM collisions. This mechanism, called freeze-in, can proceed through a…

高能物理 - 唯象学 · 物理学 2018-11-26 Lindsay Forestell , David E. Morrissey

We study sterile neutrino dark matter (DM) in a classically conformal U(1)' extension of the Standard Model with three right-handed neutrinos and a Majoron-like singlet scalar that generate the observed pattern of active neutrino masses and…

高能物理 - 唯象学 · 物理学 2026-02-13 João Gonçalves , Danny Marfatia , António P. Morais , Vinícius Oliveira , Roman Pasechnik

We study the possibility of light Dirac neutrino portal dark matter (DM) in an effective field theory setup. Dirac nature of light neutrino automatically includes its right chiral part $\nu_R$ which, in our setup, also acts like a portal…

高能物理 - 唯象学 · 物理学 2025-09-01 Debasish Borah , Satyabrata Mahapatra , Dibyendu Nanda , Sujit Kumar Sahoo , Narendra Sahu

The freeze-in mechanism for dark matter (DM) requires extremely feeble interactions with the Standard Model (SM), preventing thermal equilibrium in the early Universe and typically evading experimental detection. However, for sufficiently…

高能物理 - 唯象学 · 物理学 2026-05-26 Dilip Kumar Ghosh , Sourav Gope , Xiao-Gang He , Xuan Hong , Sk Jeesun

We develop a general effective field theory (EFT) framework for neutrino-dark matter (DM) interactions, and apply it to systematically find all possible gauge-invariant ultraviolet (UV) completions at a given EFT operator dimension. Our…

高能物理 - 唯象学 · 物理学 2026-01-01 K. S. Babu , P. S. Bhupal Dev , Anil Thapa

We consider a minimal model of fermionic dark matter, in which the Majorana fermion dark matter (DM) $\chi$ couples with the Standard Model (SM) Higgs field $H$ through a higher-dimensional term $-{\cal L}\supset H^\dagger H…

高能物理 - 唯象学 · 物理学 2023-08-23 Junpei Ikemoto , Naoyuki Haba , Shimizu Yasuhiro , Toshifumi Yamada

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 explore a new mechanism for reproducing the Dark Matter (DM) abundance: scatterings of one DM particle on light Standard Model particles. Strong bounds on its decays can be satisfied if DM undergoes freeze-in and has a mass around or…

Motivated by the dynamical reasons for the hierarchical structure of the Yukawa sector of the Standard Model (SM), we consider an extension of the SM with a complex scalar field, known as `flavon', based on the Froggatt-Nielsen mechanism.…

高能物理 - 唯象学 · 物理学 2023-11-20 Rusa Mandal , Tom Tong

We consider a general, anomaly free U$(1)^\prime$ extension of the Standard Model (SM) where the neutrino mass is generated at the tree level via the inverse seesaw mechanism. The model contains three right handed neutrinos, three…

高能物理 - 唯象学 · 物理学 2024-07-02 Arindam Das , Srubabati Goswami , Vishnudath K. N. , Tanmay Kumar Poddar

We study dark matter (DM) which is cosmologically long-lived because of standard model (SM) symmetries. In these models an approximate stabilizing symmetry emerges accidentally, in analogy with baryon and lepton number in the renormalizable…

高能物理 - 唯象学 · 物理学 2015-07-06 Clifford Cheung , David Sanford

The aim of this thesis is to determine possible interactions between the Standard Model with right-chiral neutrinos and a sector of dark matter composed of a real scalar, left- and right-chiral fermion and a vector particle, which are…

高能物理 - 理论 · 物理学 2014-10-17 Mateusz Duch

We consider effective operators describing Dark Matter (DM) interactions with Standard Model fermions. In the non-relativistic limit of the DM field, the operators can be organized according to their mass dimension and their velocity…

高能物理 - 唯象学 · 物理学 2013-02-27 Andrea De Simone , Alexander Monin , Andrea Thamm , Alfredo Urbano

Semi-annihilation is a generic feature of dark matter theories stabilised by symmetries larger than a $Z_2$. It contributes to thermal freeze out, but is irrelevant for direct and collider searches. This allows semi-annihilating dark matter…

高能物理 - 唯象学 · 物理学 2017-03-08 Yi Cai , Andrew Spray

The freeze-in mechanism of dark matter production provides a simple and intriguing alternative to the WIMP paradigm. In this paper, we analyze whether freeze-in can be used to account for the dark matter in the so-called singlet fermionic…

高能物理 - 唯象学 · 物理学 2015-06-17 Michael Klasen , Carlos E. Yaguna

In this talk, I explained how the observed dark matter (DM) relic abundance can be accounted for in models composed of three sectors (the DM, the Standard Model (SM) and a light mediator) connected to each other. This scenario is explored…

高能物理 - 唯象学 · 物理学 2021-05-18 Laurent Vanderheyden

We study ultra-violet completions for d = 6 four-fermion operators in the standard model effective field theory (SMEFT), focusing on models that contain cold dark matter candidates. Via a diagrammatic method, we generate systematically…

高能物理 - 唯象学 · 物理学 2023-09-11 Ricardo Cepedello , Fabian Esser , Martin Hirsch , Veronica Sanz

We investigate the freeze-in of MeV-scale fermionic dark matter (DM) that couples to the Standard Model via a new vector mediator to assess the potential that future direct detection experiments have to observe new physics in either the DM…

高能物理 - 唯象学 · 物理学 2026-04-28 David Cerdeño , Patrick Foldenauer , Rafael López Noé , Óscar Zapata

Within the framework of the extra-dimensional Randall-Sundrum set-up, we investigate the freeze-in production of Standard Model (SM) gauge-singlet scalar, fermionic, and massive vector dark matter (DM). Assuming that both the DM and SM…

高能物理 - 唯象学 · 物理学 2026-05-26 Basabendu Barman , Ashmita Das , Partha Kumar Paul , Narendra Sahu , Rakesh Kumar SivaKumar

We demonstrate that the scalaron, a scalar degree of freedom, emerging from the $f(R)$ theory of gravity, can account for the observed dark matter (DM) abundance if its mass is around the MeV scale, to ensure its cosmological stability.…

高能物理 - 唯象学 · 物理学 2026-01-07 Basabendu Barman , Ashmita Das , Rakesh Kumar SivaKumar , Rudra Pratap Udgata
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