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The class of `Asymmetric Dark Matter' scenarios relies on the existence of a primordial particle/anti-particle asymmetry in the dark sector related to the baryon asymmetry as a way to address the observed similarity between the baryonic and…

高能物理 - 唯象学 · 物理学 2013-01-01 Gabrijela Zaharijas

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

A novel paradigm for thermal dark matter (DM), termed "bouncing dark matter", is presented. In canonical thermal DM scenarios, the DM abundance falls exponentially as the temperature drops below the mass of DM, until thermal freezeout…

高能物理 - 唯象学 · 物理学 2022-10-05 Bibhushan Shakya

We examine the vector-portal inelastic dark matter (DM) model with DM mass $m_\chi$ and dark photon mass $m_{A'}$, in the `forbidden dark matter' regime where $1 \lesssim m_{A'}/m_\chi \lesssim 2$, carefully tracking the dark sector…

高能物理 - 唯象学 · 物理学 2022-10-14 Patrick J. Fitzpatrick , Hongwan Liu , Tracy R. Slatyer , Yu-Dai Tsai

We study the constraints from direct detection and solar capture on dark matter scenarios with a subdominant dissipative component. This dissipative dark matter component in general has both a symmetric and asymmetric relic abundance.…

高能物理 - 唯象学 · 物理学 2015-06-18 JiJi Fan , Andrey Katz , Jessie Shelton

If dark matter was produced in the early Universe by the decoupling of its annihilations into known particles, there is a sharp experimental target for the size of its coupling. We show that if dark matter was produced by inelastic…

高能物理 - 唯象学 · 物理学 2020-04-22 Raffaele Tito D'Agnolo , Duccio Pappadopulo , Joshua T. Ruderman , Po-Jen Wang

The origin of dark matter as a thermal relic offers a compelling way in which the early universe was initially populated by dark matter. Alternative explanations typically appear exotic compared to the simplicity of thermal production.…

高能物理 - 理论 · 物理学 2016-12-21 Scott Watson

We show that the relic abundance of the minority component of asymmetric dark matter can be very sensitive to the expansion rate of the Universe and the temperature of transition between a non-standard pre-Big Bang Nucleosynthesis…

高能物理 - 唯象学 · 物理学 2015-06-15 Graciela B. Gelmini , Ji-Haeng Huh , Thomas Rehagen

We study thermal corrections to a model of real scalar dark matter (DM) interacting feebly with a SM fermion and a gauge-charged vector-like fermion mediator. We employ the Closed-Time-Path (CTP) formalism for our calculation and go beyond…

高能物理 - 唯象学 · 物理学 2025-07-09 Mathias Becker , Emanuele Copello , Julia Harz , Carlos Tamarit

Low energy antideuteron detection presents a unique channel for indirect detection, targeting dark matter that annihilates into hadrons in a relatively background-free way. Since the idea was first proposed, many WIMP-type models have…

高能物理 - 唯象学 · 物理学 2020-05-26 Lisa Randall , Weishuang Linda Xu

Thermal production of light dark matter with sub-GeV scale mass can be attributed to $3\rightarrow 2$ self-annihilation processes. We consider the thermal average for annihilation cross sections of dark matter at $3\rightarrow 2$ and…

高能物理 - 唯象学 · 物理学 2017-05-24 Soo-Min Choi , Hyun Min Lee , Min-Seok Seo

We fully explore the thermal freezeout histories of a vector-portal dark matter model, in the region of parameter space in which the ratio of masses of the dark photon $A^{\prime}$ and dark matter $\chi$ is in the range $1 \lesssim…

高能物理 - 唯象学 · 物理学 2022-11-09 Patrick J. Fitzpatrick , Hongwan Liu , Tracy R. Slatyer , Yu-Dai Tsai

The quest for the elusive dark matter (DM) that permeates the Universe (and in general the search for signatures of Physics beyond the Standard Model at astronomical scales) provides a unique opportunity and a tough challenge to the…

高能天体物理现象 · 物理学 2018-02-05 Daniele Gaggero , Mauro Valli

Any astrophysical object can, in principle, serve as a probe of the interaction between Dark Matter and regular, baryonic matter. This method is based on the potential observable consequences annihilations of captured Dark Matter has on the…

宇宙学与河外天体物理 · 物理学 2024-02-13 Cosmin Ilie

We suggest that an interplay between microscopic and macroscopic physics can give rise to dark matter (DM) whose interactions with the visible sector fundamentally undulate in time, independent of celestial dynamics. A concrete example is…

高能物理 - 唯象学 · 物理学 2020-12-30 Joe Davighi , Matthew McCullough , Joseph Tooby-Smith

In light of recent DAMIC-M results, we present the status of thermal-relic dark matter $\chi$ coupled to a kinetically-mixed dark photon $A^\prime$. In the predictive "direct annihilation" regime, $m_{A'} > m_\chi$, the relic abundance…

高能物理 - 唯象学 · 物理学 2025-05-08 Gordan Krnjaic

Light thermal dark matter has emerged as an attractive theoretical possibility and a promising target for discovery at experiments in the near future. Such scenarios generically invoke mediators with very small couplings to the Standard…

高能物理 - 唯象学 · 物理学 2025-02-24 Gopolang Mohlabeng , Adreja Mondol , Tim M. P. Tait

The particle nature of dark matter (DM) remains one of the most significant enigmas in modern cosmology. Axion-like particles (ALPs), as well-motivated candidates for cold dark matter, can undergo radiative decay into photon pairs, a…

宇宙学与河外天体物理 · 物理学 2026-05-08 Wen-Qing Guo

The relic density of a cold dark matter (CDM) candidate is calculated in the context of three non-standard cosmological scenaria and its value is compared with the one obtained in the standard regime. In particular, we consider the…

高能物理 - 唯象学 · 物理学 2016-11-09 C. Pallis

We study the thermodynamic history of composite Dark Matter models. We start with classifying the models by means of the symmetries partially protecting the composite Dark Matter decays and constrain their lifetimes. For each model, we…

高能物理 - 唯象学 · 物理学 2020-05-21 Nicola Andrea Dondi , Francesco Sannino , Juri Smirnov