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相关论文: Freeze-in through portals

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At the tail of its velocity distribution, cold dark matter (DM) can annihilate at finite temperature to states heavier than itself. We explore the possibility that DM freezeout is dictated by these "forbidden annihilations" at the…

高能物理 - 唯象学 · 物理学 2017-02-15 Antonio Delgado , Adam Martin , Nirmal Raj

We propose a self-interacting dark matter (DM) scenario with right handed neutrino (RHN) portal to the standard model (SM). The dark sector consists of a particle DM, assumed to be a Dirac fermion, and a light mediator in terms of a dark…

高能物理 - 唯象学 · 物理学 2022-01-19 Debasish Borah , Manoranjan Dutta , Satyabrata Mahapatra , Narendra Sahu

We consider a simple Higgs portal dark matter (DM) model, where the Standard Model is extended with a complex singlet scalar. The imaginary part of the scalar becomes a massive and stable pseudo-Nambu-Goldstone boson, serving as the DM…

高能物理 - 唯象学 · 物理学 2025-12-05 Nicolás Bernal , Giovanna Cottin , Bastián Díaz Sáez , Manuel López

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 present a new study on the Gravity-Mediated Dark Matter (GMDM) scenario, where interactions between dark matter (DM) and the Standard Model are mediated by spin-two particles. Expanding on this established framework, we explore a novel…

高能物理 - 唯象学 · 物理学 2024-12-12 Hyun Min Lee , Myeonghun Park , Veronica Sanz

We discuss the possibility of realising a two-component dark matter (DM) scenario where the two DM candidates differ from each other by virtue of their production mechanism in the early universe. One of the DM candidates is thermally…

高能物理 - 唯象学 · 物理学 2019-11-13 Debasish Borah , Arnab Dasgupta , Sin Kyu Kang

Lepton portal dark matter (DM) models are a class of models where the DM candidates solely couple to charged leptons through a mediator carrying a lepton number. These models are very interesting since they avoid constraints from direct…

高能物理 - 唯象学 · 物理学 2023-07-05 Adil Jueid , Salah Nasri

We study a scenario where a dark sector, described by a Conformal Field Theory (CFT), interacts with the Standard Model through the neutrino portal. In this setup, conformal invariance breaks below the electroweak scale, causing the theory…

高能物理 - 唯象学 · 物理学 2024-12-03 Sungwoo Hong , Maxim Perelstein , Taewook Youn

We introduce a new mechanism for the simultaneous generation of baryon and dark matter asymmetries through ultraviolet-dominated freeze-in scatterings. The mechanism relies on heavy Majorana neutrinos that connect the visible Standard Model…

高能物理 - 唯象学 · 物理学 2026-03-05 Pouya Asadi , Marianne Moore , David E. Morrissey , Michael Shamma

We consider a simple extension of the standard model with fermionic dark matter (DM) and a $Z'$ gauge boson acting as a mediator. We also assume a scenario where cosmic reheating occurs at low temperatures due to the decay of a massive…

高能物理 - 唯象学 · 物理学 2024-12-18 Geneviève Bélanger , Nicolás Bernal , Alexander Pukhov

It is challenging to resolve the small-scale problem for dark matter being a weakly-interacting massive particle. We attempt to address this issue by proposing a self-interacting freeze-in dark matter via dark photon. In this model, the…

高能物理 - 唯象学 · 物理学 2024-10-22 Xinyue Yin , Shuai Xu , Sibo Zheng

Within the context of $N=1$ supersymmetric heterotic $M$-theory, we present a "freeze-in" mechanism for producing dark matter via a "moduli portal" between the observable and hidden sectors. It is assumed that the observable sector consists…

高能物理 - 唯象学 · 物理学 2022-09-28 Sebastian Dumitru , Burt A. Ovrut

We consider dark matter (DM) with very weak couplings to the standard model (SM), such that its self-annihilation cross section is much smaller than the canonical one, $\langle\sigma v\rangle_{\chi\chi} \ll…

高能物理 - 唯象学 · 物理学 2019-04-18 Mathias Garny , Jan Heisig , Marco Hufnagel , Benedikt Lülf , Stefan Vogl

We generalize models invoking a spin-2 particle as a mediator between the dark sector and the Standard Model. We show that a massive spin-2 messenger can efficiently play the role of a portal between the two sectors. The dark matter is then…

高能物理 - 唯象学 · 物理学 2018-06-20 Nicolas Bernal , Maira Dutra , Yann Mambrini , Keith A. Olive , Marco Peloso , Mathias Pierre

We investigate freeze-in production of light dark matter through the quark flavor-changing operator $(\bar{s}\gamma_\mu d)(\bar{\chi}\gamma^\mu\chi)$ in a low-reheating cosmology. For reheating temperatures below the QCD crossover, kaon…

高能物理 - 唯象学 · 物理学 2026-05-08 Motoi Endo , Takumu Yamanaka

In this article, we show that in the usual type-I seesaw framework, augmented solely by a neutrino portal interaction, the dark matter (DM) relic density can be created through freeze-in in a manner fully determined by the seesaw…

高能物理 - 唯象学 · 物理学 2021-10-26 Rupert Coy , Aritra Gupta , Thomas Hambye

In this article we discuss a general effective-theory description of a multi-component dark sector with an unspecified non-trivial symmetry and its interactions with the Standard Model generated by the exchange of heavy mediators. We then…

高能物理 - 唯象学 · 物理学 2015-06-15 Vannia Gonzalez Macias , Jose Wudka

We study the thermal freeze-out of a dark photon dark matter in the so-called dark-axion portal - a triple coupling among a dark photon, an axion-like particle and the SM $\gamma$ or $Z$ boson. We analyze in detail the thermal production…

高能物理 - 唯象学 · 物理学 2025-02-18 Bastián Díaz Sáez

We present a class of dark matter models, in which the dark matter particle is a feebly interacting massive particle (FIMP) produced via the decay of an electrically charged and/or colored parent particle. Given the feeble interaction, dark…

高能物理 - 唯象学 · 物理学 2019-10-02 G. Bélanger , N. Desai , A. Goudelis , J. Harz , A. Lessa , J. M. No , A. Pukhov , S. Sekmen , D. Sengupta , B. Zaldivar , J. Zurita

When dark matter particles only feebly interact with plasma constituents in the early universe, they never reach thermal equilibrium. As opposed to the freeze-out mechanism, where the dark matter abundance is determined at $T \ll M$, the…

高能物理 - 唯象学 · 物理学 2021-03-26 Simone Biondini , Jacopo Ghiglieri