原始ブラックホールの証拠が惑星や地球上の日常的な物体に潜んでいるかもしれない(Evidence of primordial black holes may be hiding in planets, or even everyday objects here on Earth)

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2024-12-02 バッファロー大学(UB)

原始ブラックホールの証拠が惑星や地球上の日常的な物体に潜んでいるかもしれない(Evidence of primordial black holes may be hiding in planets, or even everyday objects here on Earth)
An illustration of small primordial black holes. In reality, such tiny black holes would have a difficult time forming the accretion disks that make them visible here. Photo: NASA

ニューヨーク州立大学バッファロー校の研究者らは、初期宇宙で形成されたとされる原始ブラックホール(PBH)が、惑星内部や地球上の物質内に存在する可能性を理論的に示しました。PBHが大きな岩石天体内に閉じ込められると、その液体核を吸収し、内部が空洞化する可能性があります。また、PBHが高速で固体物質を通過すると、顕微鏡で観察可能な直線的なトンネルを残すとされています。これらの痕跡は、地球上の岩石、金属、ガラスなどの古い物質内に存在する可能性があり、PBHの存在を確認する新たな手がかりとなるかもしれません。研究者らは、これらの痕跡を探すことは大きな資源を必要とせず、PBHの初めての証拠を得る可能性があると指摘しています。

<関連情報>

惑星、小惑星、そして地球上の小さな原始ブラックホールを探す Searching for small primordial black holes in planets, asteroids and here on Earth

De-Chang Dai, Dejan Stojkovic
Physics of the Dark Universe  Available online: 19 September 2024
DOI:https://doi.org/10.1016/j.dark.2024.101662

Abstract

Small primordial black holes could be captured by rocky planets or asteroids, consume their liquid cores from inside and leave hollow structures. We calculate the surface density and surface tension of a hollow structure around a black hole and compare them with the density and compressive strength of various materials that appear in nature to find the allowed parameter space. For example, granite or iron can support a hollow asteroid/planetoid/moon of the size of up to 0.1R⊕. Along the same lines, future civilizations might build spherical structures around black holes to harvest their energy. Using the strongest material that we currently know how to make (multiwall carbon nanotube), to withstand gravity of one solar mass black hole, the shell must be constructed at distances larger than 104R⊙. Alternatively, a fast black hole can leave a narrow tunnel in a solid object while passing through it. For example, a 1022 g black hole should leave a tunnel with a radius of 0.1μm, which is large enough to be seen by an optical microscope. We could look for such micro-tunnels here on Earth in very old rocks, or even glass or other solid structures in very old buildings. While our estimate gives a very small probability of finding such tunnels, looking for them does not require expensive equipment and long preparation, and the payoff might be significant.

1701物理及び化学
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