ダークマターは予想より高温で誕生した可能性(Dark matter may have begun much hotter than scientists thought)

2026-01-13 ミネソタ大学

ミネソタ大学の研究チームが、暗黒物質(ダークマター)の起源に関する従来の理解を見直す新たな理論研究を発表した。一般に暗黒物質は、宇宙初期に「冷たい」状態で生成されたと考えられてきたが、本研究では、暗黒物質が誕生当初ははるかに高温だった可能性が示された。研究者らは初期宇宙の物理過程を理論モデルで再検討し、暗黒物質が高エネルギー状態で生成され、その後急速に冷却したシナリオでも、現在観測されている宇宙構造を説明できることを明らかにした。この「より高温な起源」を想定すると、暗黒物質の性質や相互作用に関する制約条件が変わり、将来の観測や実験で検証可能な新たな予測が得られるという。本研究は、暗黒物質探索の理論的枠組みを拡張し、宇宙の成り立ちを理解する上で重要な視点を提供している。

ダークマターは予想より高温で誕生した可能性(Dark matter may have begun much hotter than scientists thought)
New research suggests dark matter—one of the Universe’s greatest mysteries—may have started out moving nearly at the speed of light before cooling enough to help form galaxies.

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超相対論的フリーズアウト:WIMPからFIMPへの架け橋 Ultrarelativistic Freeze-Out: A Bridge from WIMPs to FIMPs

Stephen E. Henrich, Yann Mambrini, and Keith A. Olive
Physical Review Letters  Published: 24 November, 2025
DOI: https://doi.org/10.1103/zk9k-nbpj

Abstract

We reexamine the case for dark matter (DM) produced by ultrarelativistic freeze-out (UFO). UFO is the mechanism by which standard model neutrinos decouple from the radiation bath in the early Universe at a temperature ≈1  MeV. This corresponds to chemical freeze-out without Boltzmann suppression, such that the freeze-out (decoupling) temperature is much greater than and the neutrinos are therefore ultrarelativistic at freeze-out. While UFO has historically been rejected as a viable mechanism for DM production due to its association with hot DM and the accompanying incompatibility with Λ⁢CDM, we show that when the approximation of instantaneous reheating after inflation is lifted, UFO can produce cold DM and account for the entire observed relic density in large regions of parameter space. In fact, DM with masses ranging from sub-eV to PeV scales can undergo UFO and be cold before structure formation, given only a simple perturbative, postinflationary reheating period prior to radiation domination. For some interactions, such as a contact interaction between the Higgs and DM scalars, there is a seamless transition between the weakly interacting massive particle and feebly interacting massive particle regimes that excludes UFO. However, for many other interactions, such as standard model fermions producing fermionic DM via a heavy scalar or vector mediator, the weakly interacting massive particle to feebly interacting massive particle transition occurs necessarily via a large intermediate regime corresponding to UFO. We characterize the general features of UFO in this Letter, while we supply a more detailed analysis in a companion paper. These results render the conventional mechanism for producing hot DM broadly compatible with cold DM.

1701物理及び化学
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