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相关论文: Vector SIMP dark matter

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We consider a fermionic dark matter candidate interacting via a scalar mediator coupled with the Standard Model through a Higgs portal. We consider general setting including both scalar and pseudoscalar interactions between the scalar and…

高能物理 - 唯象学 · 物理学 2017-04-12 Kimmo Kainulainen , Kimmo Tuominen , Ville Vaskonen

Self-interacting dark matter (SIDM) is a simple and well-motivated scenario that could explain long-standing puzzles in structure formation on small scales. If the required self-interaction arises through a light mediator (with mass $\sim…

高能物理 - 唯象学 · 物理学 2015-11-04 Eugenio Del Nobile , Manoj Kaplinghat , Hai-Bo Yu

I present a class of hidden sector dark matter (DM) models with local dark gauge symmetries, where DM is stable due to unbroken local dark gauge symmetry, or due topology, or it is long-lived because of some accidental symme- tries, and the…

高能物理 - 唯象学 · 物理学 2015-03-19 P. Ko

We comprehensively study experimental constraints and prospects for a class of minimal hidden sector dark matter (DM) models, highlighting how the cosmological history of these models informs the experimental signals. We study simple…

高能物理 - 唯象学 · 物理学 2018-04-04 Jared A. Evans , Stefania Gori , Jessie Shelton

Based on observational constraints on large scale structure and halo structure, dark matter is generally taken to be cold and essentially collisionless. On the other hand, given the large number of particles and forces in the visible world,…

宇宙学与河外天体物理 · 物理学 2013-12-09 JiJi Fan , Andrey Katz , Lisa Randall , Matthew Reece

Large classes of non-supersymmetric string models equipped with standard-model features have been constructed, but very little of their phenomenology is known. Interestingly, their spectra exhibit scalar fields whose only couplings to…

高能物理 - 唯象学 · 物理学 2023-06-21 Esau Cervantes , Omar Perez-Figueroa , Ricardo Perez-Martinez , Saul Ramos-Sanchez

The Atomiki anomaly can be interpreted as a new light vector boson. If such a new particle exists, it could be a mediator between the Standard Model sector and the dark sector including the dark matter. We discussed some simple effective…

高能物理 - 唯象学 · 物理学 2018-01-24 Yasuhiro Yamamoto

We explore a two component dark matter model with a fermion and a scalar. In this scenario the Standard Model (SM) is extended by a fermion, a scalar and an additional pseudo scalar. The fermionic component is assumed to have a global ${\rm…

高能物理 - 唯象学 · 物理学 2017-10-25 Amit Dutta Banik , Madhurima Pandey , Debasish Majumdar , Anirban Biswas

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 laboratory experiments that can detect stable, neutral strongly interacting massive particles (SIMPs). We explore the SIMP annihilation cross section from its minimum value (restricted by cosmological bounds) to the barn range,…

高能物理 - 唯象学 · 物理学 2007-05-23 Vigdor L. Teplitz , Rabindra N. Mohapatra , Fred Olness , Ryszard Stroynowski

We consider laboratory experiments that can detect stable, neutral strongly interacting massive particles (SIMPs). We explore the SIMP annihilation cross section from its minimum value (restricted by cosmological bounds) to the barn range,…

高能物理 - 唯象学 · 物理学 2016-09-06 Vigdor L. Teplitz , Rabindra N. Mohapatra , Fred Olness , Ryszard Stroynowski

The Standard Model Effective Field Theory (SMEFT) and the Low Energy Effective Field Theory (LEFT) can be extended by adding additional spin 0, 1/2 and 1 dark matter particles which are singlets under the Standard Model (SM) gauge group. We…

高能物理 - 唯象学 · 物理学 2022-10-13 Jason Aebischer , Wolfgang Altmannshofer , Elizabeth E. Jenkins , Aneesh V. Manohar

More than one dark sector particle transforming under the same symmetry provides one stable dark matter (DM) component which undergoes co-annihilation with the heavier particle(s) decaying to DM. Specific assumptions on the kinematics and…

高能物理 - 唯象学 · 物理学 2024-10-22 Subhaditya Bhattacharya , Lipika Kolay , Dipankar Pradhan

We investigate the role of an axion-like particle (ALP) as a portal between the dark and visible sectors. Unlike conventional studies, which typically assume fermionic dark matter (DM), we explore the phenomenological implications of scalar…

高能物理 - 唯象学 · 物理学 2025-07-08 Francesco D'Eramo , Tommaso Sassi

A weak photon interaction with the hidden sector of the Universe, introduced recently to realize a "photonic portal", (to such a hypothetic sector responsible for cold dark matter), is conjectured to be embedded in a more extended weak…

高能物理 - 唯象学 · 物理学 2010-05-28 Wojciech Krolikowski

We demonstrate that in a two component dark matter (DM) set up, when DM$_1$ is equilibrated with the thermal bath, the other DM$_2$, in spite of having feeble or negligible interaction with the SM particles, can be brought to equilibrium…

高能物理 - 唯象学 · 物理学 2023-12-05 Subhaditya Bhattacharya , Jayita Lahiri , Dipankar Pradhan

The scalar dark matter candidate in a prototypical theory space little Higgs model is investigated. We review all details of the model pertinent to dark matter. We perform a thermal relic density calculation including couplings to the gauge…

高能物理 - 唯象学 · 物理学 2014-11-17 Andreas Birkedal-Hansen , Jay G. Wacker

We show that hidden hot dark matter, hidden-sector dark matter with interactions that decouple when it is relativistic, is a viable dark matter candidate provided it has never been in thermal equilibrium with the particles of the standard…

宇宙学与河外天体物理 · 物理学 2009-12-15 Kris Sigurdson

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 consider here three dark matter models with the gauge symmetry of the standard model plus an additional local $U(1)_D$ factor. One model is truly secluded and the other two models begin flipped, but end up secluded. All of these models…

高能物理 - 唯象学 · 物理学 2018-02-28 E. C. F. S. Fortes , V. Pleitez , F. W. Stecker