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相关论文: The Four Basic Ways of Creating Dark Matter Throug…

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We review scenarios in which the particles that account for the Dark Matter (DM) in the Universe interact only through their couplings with the Higgs sector of the theory, the so-called Higgs-portal models. In a first step, we use a general…

高能物理 - 唯象学 · 物理学 2020-02-26 Giorgio Arcadi , Abdelhak Djouadi , Martti Raidal

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

Thermal relic dark matter has been severely constrained in recent years by direct and indirect dark matter searches, as well as multi-messenger probes of dark sectors. At the current level of experimental precision, it has become difficult…

高能物理 - 唯象学 · 物理学 2026-05-20 Wan-Zhe Feng , Zi-Hui Zhang

One loop correction to the dark matter (DM) annihilation cross section is usually assumed to be sub-dominate in calculating the DM relic density. In this paper, we propose a scenario where DM freezes out mainly via loops in the neutrino…

高能物理 - 唯象学 · 物理学 2020-09-28 Wei Chao

We study warm Higgs portal dark matter (DM) in the framework of freeze-in at stronger coupling. This scenario assumes that the Standard Model thermal bath temperature has always been relatively low, which suppresses dark matter production.…

高能物理 - 唯象学 · 物理学 2026-05-05 Duarte Feiteira , Oleg Lebedev , Vinícius Oliveira

The non-detection of dark matter may be attributed to the dark matter residing in a darker hidden sector. We explore the possibility that a hidden sector produced through the freeze-in mechanism, can further generate an even more hidden…

高能物理 - 唯象学 · 物理学 2025-12-05 Wan-Zhe Feng , Zi-Hui Zhang

We perform an analysis of Higgs portal models of dark matter (DM), where DM is light enough to contribute to invisible Higgs decays. Using effective field theory we show that DM can be a thermal relic only if there are additional light…

高能物理 - 唯象学 · 物理学 2013-12-09 Admir Greljo , J. Julio , Jernej F. Kamenik , Christopher Smith , Jure Zupan

In this talk, we present a mechanism of Dark Matter production during first order phase transitions and happening via the collision of the bubble wall and plasma quanta. We will first study the possibility that the dark matter is produced…

高能物理 - 唯象学 · 物理学 2024-12-10 Miguel Vanvlasselaer

In this paper, we investigate the production of Majorana fermionic dark matter (DM) via the Higgs portal, considering both freeze-in and freeze-out mechanisms during and after the post-inflationary reheating phase. We assume that the…

高能物理 - 唯象学 · 物理学 2026-02-13 Rajesh Mondal , Sourav Mondal , Toshifumi Yamada

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

Dark Matter (DM) may belong to a hidden sector that is only feebly interacting with the Standard Model (SM) and may have never been in thermal equilibrium in the Early Universe. In this case, the observed abundance of dark matter particles…

高能物理 - 唯象学 · 物理学 2019-02-07 Thomas Hambye , Michel H. G. Tytgat , Jérôme Vandecasteele , Laurent Vanderheyden

We present a systematic cosmological study of a universe in which the visible sector is coupled, albeit very weakly, to a hidden sector comprised of its own set of particles and interactions. Assuming that dark matter (DM) resides in the…

高能物理 - 唯象学 · 物理学 2015-03-17 Clifford Cheung , Gilly Elor , Lawrence J. Hall , Piyush Kumar

There are many extensions of the Standard Model with a dark matter (DM) candidate obtained via the freeze-out mechanism. It can happen that after all experimental and theoretical constraints are taken into account, all parameter points have…

高能物理 - 唯象学 · 物理学 2024-07-09 Rodrigo Capucha , Karim Elyaouti , Margarete Mühlleitner , Johann Plotnikov , Rui Santos

It is known that single-field freeze-in dark matter barely leaves footprints in dark matter direct detection and collider experiments. This situation can be altered in two-field context. In this work we propose a two-field freeze-in dark…

高能物理 - 唯象学 · 物理学 2025-08-18 Xinyue Yin , Shuai Xu , Sibo Zheng

The suppression of cosmological structure at small scales is a key signature of dark matter (DM) produced via freeze-in in the low-mass regime. We present a comprehensive analysis of its impact, incorporating recent constraints from Milky…

高能物理 - 唯象学 · 物理学 2025-12-12 Francesco D'Eramo , Alessandro Lenoci , Ariane Dekker

We show that dark matter could be made of massive gauge bosons whose stability doesn't require to impose by hand any discrete or global symmetry. Stability of gauge bosons can be guaranteed by the custodial symmetry associated to the gauge…

高能物理 - 唯象学 · 物理学 2010-03-26 Thomas Hambye

We propose a two-component asymmetric FIMP (feebly interacting massive particle) dark matter (DM) model in which both DM candidates are real scalar fields. The model is an extension of the Standard Model (SM) by two scalar DM components and…

高能物理 - 唯象学 · 物理学 2026-05-26 S. Peyman Zakeri

The increasingly stringent bounds on the Higgs-portal coupling, arising from dark matter (DM) direct-detection searches, confront the minimal renormalizable complex scalar DM scenario with thermal production, where freeze-out occurs in the…

高能物理 - 唯象学 · 物理学 2025-12-30 Manimala Mitra , Dipankar Pradhan , Subham Saha

We propose a renormalizable dark matter model in which a fermionic dark matter (DM) candidate communicates with the standard model particles through two distinct portals: Higgs and vector portals. The dark sector is charged under a $U(1)'$…

高能物理 - 唯象学 · 物理学 2015-07-08 Karim Ghorbani , Hossein Ghorbani

We present a purely gravitational infra-red-calculable production mechanism for dark matter (DM). The source of both the DM relic abundance and the hot Standard Model (SM) plasma is a primordial density of micro black holes (BHs), which…

高能物理 - 唯象学 · 物理学 2018-04-18 Olivier Lennon , John March-Russell , Rudin Petrossian-Byrne , Hannah Tillim