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温暗物质

温暗物质（英语：Warm Dark Matter，简称WDM）是理论上性质介于热暗物质和冷暗物质之间的暗物质，经常以惰性中微子作为WDM的代表。

这个温暗物质模型，使得天文物理学家在宇宙各处搜寻能合于理论的物质。

参考资料

相关条目

暗物质
- 热暗物质（HDM）
- 冷暗物质（CDM）
Lambda-CDM model
修正牛顿力学

暗物质的形态

重子暗物质
冷暗物质
热暗物质
轻暗物质（英语：Light dark matter）
混合暗物质
温暗物质
自交互作用暗物质（英语：Self-interacting dark matter）
标量场暗物质（英语：Scalar field dark matter）
原初黑洞

假想的粒子

轴子
超轴子
变色龙粒子（英语：Chameleon particle）
暗光子（英语：Dark photon）
黑洞子（英语：Holeum）
LSP（英语：Lightest Supersymmetric Particle）
迷你电荷粒子（英语：Minicharged particle）
超中性子
惰性中微子
SIMP
WIMP

理论和物体

星系晕尖点问题
暗流体
暗星系
暗球状星团
暗物质晕
暗辐射（英语：Dark radiation）
暗星
矮星系问题
晕质量函数（英语：Halo mass function）
质量维度一费米子
晕族大质量致密天体
镜物质（英语：Mirror matter）
纳瓦罗–弗伦克–怀特分布（英语：Navarro–Frenk–White profile）
埃纳斯托轮廓

搜寻实验

直接侦测	轴子暗物质实验（英语：Axion Dark Matter Experiment） ANAIS ArDM 中国暗物质实验低温暗物质搜寻计划迷你惰气基低温低能量天文物理学（英语：Cryogenic Low-Energy Astrophysics with Neon） COUPP CRESST（英语：Cryogenic Rare Event Search with Superconducting Thermometers）罕见事件低温地下观测站（英语：CUORE） DAMA/LIBRA DAMA/NaI DarkSide DEAP DMTPC（英语：Dark Matter Time Projection Chamber） DRIFT EDELWEISS EURECA KIMS LUX（英语：Large Underground Xenon experiment） LZ 粒子和天体物理氙探测器 PICO PICASSO SIMPLE UKDMC WARP XENON ZEPLIN-III

间接侦测	AMS-02 ANTARES ATIC（英语：Advanced Thin Ionization Calorimeter） CALET（英语：Calorimetric Electron Telescope） CAST（英语：CERN Axion Solar Telescope）暗物质粒子探测卫星神奇伽马射线望远镜 HAWC（英语：High Altitude Water Cherenkov Experiment）高能立体视野望远镜冰立方 MOA OGLE PAMELA VERITAS（英语：VERITAS）

其它计划	MultiDark PVLAS SNOLAB

可能的暗星系

相关的

分类
维基共享

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