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The supersymmetric custodial triplet model (SCTM), which is a fully-super\-symmetric generalization of the Georgi-Machacek (GM) model, is constructed by extending the Higgs sector of the minimal supersymmetric standard model by three…

高能物理 - 唯象学 · 物理学 2025-08-01 LiangLiang Shang , Yuanping Wang , Xiaokang Du , Bingfang Yang , Stefano Moretti

The strong interactions among nucleons have an approximate spin-isospin exchange symmetry that arises from the properties of quantum chromodynamics in the limit of many colors, $N_c$. However this large-$N_c$ symmetry is well hidden and…

We study the QCD--DM scenario by analyzing the imprint of energy injection from decaying dark-sector particles on the spectral distortions (SDs) of the Cosmic Microwave Background (CMB). We adopt a unified framework capable of describing…

宇宙学与河外天体物理 · 物理学 2025-11-12 Jorge Mastache , Raúl Henriquez-Ortiz

We update a previously-proposed set of supersymmetric benchmark scenarios, taking into account the precise constraints on the cold dark matter density obtained by combining WMAP and other cosmological data, as well as the LEP and b -> s…

高能物理 - 唯象学 · 物理学 2009-09-11 M. Battaglia , A. De Roeck , J. Ellis , F. Gianotti , K. A. Olive , L. Pape

The WIMP dark matter (DM) hypothesis now is in an awkward position, owing to the stronger and stronger exclusion from DM direct detection. In this article we design a mechanism to evade this constraint.The idea is simple. DM has a…

高能物理 - 唯象学 · 物理学 2022-01-12 Jun Guo , Zhaofeng Kang , Peng Zhang

Leptophilic sub-MeV spin-zero dark matter (DM) decays into photons via one-loop processes, a scenario that has been in part overlooked in current literature. In this work, we provide updated and comprehensive upper limits on scalar,…

高能物理 - 唯象学 · 物理学 2025-09-30 Gabriele Montefalcone , Gilly Elor , Kimberly K. Boddy , Nicola Bellomo

A light fermionic weakly interacting massive particle (WIMP) dark matter is investigated by studying its minimal renormalizable model, where it requires a scalar mediator to have an interaction between the WIMP and standard model particles.…

高能物理 - 唯象学 · 物理学 2019-09-04 Shigeki Matsumoto , Yue-Lin Sming Tsai , Po-Yan Tseng

Extension of particle symmetry implies new conserved charges and the lightest particles, possessing such charges, should be stable. Created in early Universe, stable charged heavy leptons and quarks can exist and, hidden in elusive atoms…

天体物理学 · 物理学 2007-05-23 Maxim Yu. Khlopov

We discuss within the framework of effective four-fermion scalar interaction the phenomenology of a Weakly Interacting Massive Particle (WIMP) Dirac Dark Matter candidate which is exothermic (i.e. is metastable and interacts with nuclear…

高能物理 - 唯象学 · 物理学 2015-02-03 Stefano Scopel , Jong-Hyun Yoon

We study two realisations of the Fake Split Supersymmetry Model (FSSM), the simplest model that can easily reproduce the experimental value of the Higgs mass for an arbitrarily high supersymmetry scale, as a consequence of swapping…

高能物理 - 唯象学 · 物理学 2016-01-20 Karim Benakli , Luc Darmé , Mark Goodsell

In this work, we investigate the physical aspects of the inflection-point inflation scenario and assess its observational viability in light of current Cosmic Microwave Background (CMB) data. The model we consider encapsulates the inflaton…

宇宙学与河外天体物理 · 物理学 2024-06-25 Jamerson G. Rodrigues , Vinícius Oliveira , Rodrigo von Marttens , Carlos A. de S. Pires , Jailson Alcaniz

Multi-Higgs-doublet models can accommodate a dark matter candidate. An underlying symmetry not only ensures the candidate's stability but also helps control the number of free parameters. We consider two scenarios. First, we explore dark…

高能物理 - 唯象学 · 物理学 2025-06-11 Anton Kunčinas

We present an overview of scenarios where the observed Dark Matter (DM) abundance consists of Feebly Interacting Massive Particles (FIMPs), produced non-thermally by the so-called freeze-in mechanism. In contrast to the usual freeze-out…

高能物理 - 唯象学 · 物理学 2017-11-22 Nicolás Bernal , Matti Heikinheimo , Tommi Tenkanen , Kimmo Tuominen , Ville Vaskonen

We present a method for calculating large numbers of power spectra C_l and P(k) that accelerates CMBfast by a factor around 10^3 without appreciable loss of accuracy, then apply it to constrain 11 cosmological parameters from current Cosmic…

天体物理学 · 物理学 2009-10-07 Max Tegmark , Matias Zaldarriaga , Andrew J. S. Hamilton

We propose a scalar-mediated Self-Interacting Dark Matter (SIDM) model to address small-scale structure anomalies such as the core-cusp and diversity problems. The model is composed by a leptophilic scalar mediator and a pseudo-Dirac dark…

高能物理 - 唯象学 · 物理学 2026-05-05 Zihan Wang

A hidden strongly-interacting sector is a possible candidate for dark matter. One scenario consistent with astrophysical constraints is a QCD-like theory with gauge group Sp(4) and two fundamental non-degenerate fermions. We report…

高能物理 - 格点 · 物理学 2022-03-29 Axel Maas , Fabian Zierler

Scenarios for secluded WIMP dark matter models have been extensively studied in simplified versions. This paper shows a complete UV realization of a secluded WIMP dark matter model with an extra Abelian gauge symmetry that includes…

高能物理 - 唯象学 · 物理学 2025-05-09 Kimy Agudelo , Diego Restrepo , Andrés Rivera , David Suarez

Weakly interacting massive particles (WIMPs) form a promising solution to the dark matter problem and many experiments are now searching for these particles. Using effective field theories to describe the interaction of the WIMP with the…

高能物理 - 唯象学 · 物理学 2013-08-22 Daniel Schmeier

A hidden sector that kinetically mixes with the Minimal Supersymmetric Standard Model provides simple and well-motivated dark matter candidates that possess many of the properties of a traditional weakly interacting massive particle (WIMP).…

高能物理 - 唯象学 · 物理学 2020-10-21 Patrick Barnes , Zachary Johnson , Aaron Pierce , Bibhushan Shakya

In this paper, we consider three phantom dark energy models, in the context of interaction between the dark components namely cold dark matter (CDM) and dark energy (DE). The first model, known as $w_{\textrm{d}}$CDM can induce a big rip…

宇宙学与河外天体物理 · 物理学 2021-11-05 Amine Bouali , Imanol Albarran , Mariam Bouhmadi-Lopez , Ahmed Errahmani , Taoufik Ouali