Noble dark matter: Surprising elusiveness of dark baryons

IF 5 2区 物理与天体物理 Q1 Physics and Astronomy
Pouya Asadi, Austin Batz, Graham D. Kribs
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引用次数: 0

Abstract

Dark matter could be a baryonic composite of stronglyc upled constituents transforming under SU(2)L. We classify the SU(2)L representations of baryons in a class of simple confining dark sectors and find that the lightest state can be a pure singlet or a singlet that mixes with other neutral components of SU(2)L representations, which strongly suppresses the dark matter candidate’s interactions with the Standard Model. We focus on models with a confining SU(Nc) and heavy dark quarks constituting vectorlike Nf-plet of SU(2)L. For benchmark Nc and Nf, we calculate baryon mass spectra, incorporating electroweak gauge boson exchange in the nonrelativistic quark model, and demonstrate that above TeV mass scales, dark matter is dominantly a singlet state. The combination of this singlet nature with the recently discovered H-parity results in an inert state analogous to noble gases, hence we coin the term noble dark matter. Our results can be understood in the nonrelativistic effective theory that treats the dark baryons as elementary states, where we find singlets accompanying triplets, 5-plets, or more exotic representations. This generalization of WIMP-like theories is more difficult to find or rule out than dark matter models that include only a single SU(2)L multiplet (such as a wino), motivating new searches in colliders and a reanalysis of direct and indirect detection prospects in astrophysical observations. Published by the American Physical Society 2025
高贵的暗物质:令人惊讶的难以捉摸的黑暗重子
暗物质可能是在SU(2)L作用下转变的强耦合组分的重子复合物。我们将重子的SU(2)L表示分类为一类简单受限的暗扇区,并发现最轻的状态可以是纯单重态,也可以是与SU(2)L表示的其他中性组分混合的单重态,这强烈抑制了暗物质候选物质与标准模型的相互作用。我们关注的是具有受限SU(Nc)和重暗夸克构成SU(2)L的类矢量nf -夸克的模型。对于基准Nc和Nf,我们计算了重子质量谱,在非相对论夸克模型中结合电弱规范玻色子交换,并证明在TeV质量尺度以上,暗物质主要是单线态。这种单线态性质与最近发现的h宇称相结合,产生了一种类似于惰性气体的惰性状态,因此我们创造了“惰性暗物质”这个术语。我们的结果可以在非相对论有效理论中理解,该理论将暗重子视为基本态,其中我们发现单重态伴随着三重态、五重态或更奇特的表示。与只包含单个SU(2)L多星(如wino)的暗物质模型相比,这种类wimp理论的推广更难以发现或排除,这促使人们在对撞机中进行新的搜索,并重新分析天体物理观测中直接和间接探测的前景。2025年由美国物理学会出版
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来源期刊
Physical Review D
Physical Review D 物理-天文与天体物理
CiteScore
9.20
自引率
36.00%
发文量
0
审稿时长
2 months
期刊介绍: Physical Review D (PRD) is a leading journal in elementary particle physics, field theory, gravitation, and cosmology and is one of the top-cited journals in high-energy physics. PRD covers experimental and theoretical results in all aspects of particle physics, field theory, gravitation and cosmology, including: Particle physics experiments, Electroweak interactions, Strong interactions, Lattice field theories, lattice QCD, Beyond the standard model physics, Phenomenological aspects of field theory, general methods, Gravity, cosmology, cosmic rays, Astrophysics and astroparticle physics, General relativity, Formal aspects of field theory, field theory in curved space, String theory, quantum gravity, gauge/gravity duality.
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