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Emergent Ising$_h^2$ integrability is anticipated in a quantum Ising ladder composed of two weakly-coupled critical transverse field Ising chains. The system is remarkable for including eight types of massive relativistic particles, with…

强关联电子 · 物理学 2025-05-29 Yunjing Gao , Xiao Wang , Ning Xi , Yunfeng Jiang , Rong Yu , Jianda Wu

In this work we complete a model independent analysis of dark matter constraining its mass and interaction strengths with data from astro- and particle physics experiments. We use the effective field theory framework to describe…

高能物理 - 唯象学 · 物理学 2015-06-19 Csaba Balázs , Tong Li , Jayden L. Newstead

We consider a scenario where the dark sector includes two Feebly Interacting Massive Particles (FIMPs), with couplings to the Standard Model particles that allow their production in the Early Universe via thermal freeze-in. These couplings…

高能物理 - 唯象学 · 物理学 2020-03-18 Johannes Herms , Alejandro Ibarra

We propose that dark matter is composed of particles that naturally have the correct thermal relic density, but have neither weak-scale masses nor weak interactions. These WIMPless models emerge naturally from gauge-mediated supersymmetry…

高能物理 - 唯象学 · 物理学 2009-01-10 Jonathan L. Feng , Jason Kumar

We consider dark matter as Strongly Interacting Massive Particles (SIMPs) in a hidden sector, thermally decoupled from the Standard Model heat bath. Due to its strong interactions, the number-changing processes of the SIMP lead to its…

高能物理 - 唯象学 · 物理学 2018-06-06 Matti Heikinheimo , Kasper Langaeble , Kimmo Tuominen

One of the most popular classes of candidates for dark matter are Weakly Interacting Massive Particles (WIMPs), i.e. particles possessing masses and couplings falling roughly within the electroweak scale. Apart from offering a natural…

高能物理 - 唯象学 · 物理学 2011-06-21 Andreas Goudelis

The WIMP (weakly interacting massive particle) paradigm for dark matter is currently being probed via many different experiments. Direct detection, indirect detection and collider searches are all hoping to catch a glimpse of these elusive…

高能物理 - 唯象学 · 物理学 2013-04-24 Herbert Dreiner , Moritz Huck , Michael Krämer , Daniel Schmeier , Jamie Tattersall

So far all evidences of dark matter (DM) come from astrophysical and cosmological observations, due to gravitational interactions of the DM. It is possible that the true DM particle in the universe joins gravitational interactions only, but…

高能物理 - 唯象学 · 物理学 2015-03-30 Jing Ren , Hong-Jian He

We develop a quantum-optical framework demonstrating that thermal radiation can confine a significant portion of its energy in dark collective modes -- highly entangled photon states that, despite their photonic nature, remain decoupled…

量子物理 · 物理学 2025-05-23 Celso Jorge Villas-Boas , Ciro Micheletti Diniz

We address the question of whether the upcoming generation of dark matter search experiments and colliders will be able to discover if the dark matter in the Universe has two components of weakly interacting massive particles (WIMPs). We…

高能物理 - 唯象学 · 物理学 2009-12-23 Stefano Profumo , Kris Sigurdson , Lorenzo Ubaldi

We study an effective field theory which includes the Standard Model extended by a Dark Sector consisting of two fermionic $SU(2)_{L}$-doublets. A $Z_2$ parity guarantees that, after electroweak symmetry breaking, the lightest neutral…

高能物理 - 唯象学 · 物理学 2017-04-03 Dimitrios Karamitros

We study the possibility that a dark group, a gauge group with particles interacting with the standard model particles only via gravity, is responsible for containing the dark energy and dark matter required by present day observations. We…

天体物理学 · 物理学 2009-11-07 Axel de la Macorra

The problem of the dark matter in the universe is reviewed. A short history of the subject is given, and several of the most obvious particle candidates for dark matter are identified. Particular focus is given to weakly interacting,…

高能天体物理现象 · 物理学 2012-06-15 Lars Bergström

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

A strongly interacting massive particle (SIMP) is an interesting candidate for dark matter (DM) because its self-interaction cross section can be naturally strong enough to address the astrophysical problem of small-scale structure…

高能物理 - 唯象学 · 物理学 2020-10-14 Ayuki Kamada , Masaki Yamada , Tsutomu T. Yanagida

This write--up gives a rather elementary introduction into particle physics aspects of the cosmological Dark Matter puzzle. A fairly comprehensive list of possible candidates is given; in each case the production mechanism and possible ways…

高能物理 - 唯象学 · 物理学 2009-10-31 Manuel Drees

A generic weakly interacting massive particle (WIMP) is one of the most attractive candidates to account for the cold dark matter in our Universe, since it would be thermally produced with the correct abundance to account for the observed…

宇宙学与河外天体物理 · 物理学 2021-10-13 David G. Cerdeno , Anne M. Green

One of the most puzzling problems of modern physics is the identification of the nature a non-relativistic matter component present in the universe, contributing to more than 25$\%$ of the total energy budget, known as Dark Matter. Weakly…

高能物理 - 唯象学 · 物理学 2019-01-18 Mathias Pierre

A fraction of the dark matter may consist of a particle species that interacts much more strongly with the Standard Model than a typical weakly interacting massive particle (WIMP) of similar mass. Such a strongly interacting dark matter…

高能物理 - 唯象学 · 物理学 2022-08-12 David McKeen , Marianne Moore , David E. Morrissey , Maxim Pospelov , Harikrishnan Ramani

This paper explores the possibility that dark matter particles are objects with a set of excitable levels, as for a string or drum. A change in excitation is associated with the absorption or emission of a photon, and the probability of…

宇宙学与河外天体物理 · 物理学 2020-02-25 Andrew J. Wren
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