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archive.today
Buckley, Matthew R.; Difranzo, Anthony (1 February 2018). "Synopsis: A Way to Cool Dark Matter". Physical Review Letters. 120 (5): 051102. Archived from the original on 26 October 2020. 암흑 물질에 대해 널리 알려진 믿음 중 하나는 암흑 물질이 에너지를 방출하여 냉각될 수 없다는 것이다. 만약 가능하다면, 중입자 물질이 행성들, 항성들, 은하들을 형성하는 것과 같은 방식으로 뭉쳐서 고밀도의 천체들을 만들 수 있다. 지금까지의 관측에 따르면 암흑 물질은 그렇게 하지 않는다는 것을 암시한다. 그것은 확산 해일로에만 존재한다... 결과적으로, 완전히(또는 대부분) 암흑 물질로 만들어진 별들과 같은 매우 고밀도인 천체들이 있을 가능성은 극히 낮다.
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Garrett, Katherine; Dūda, Gintaras (2011). "Dark Matter: A Primer". Advances in Astronomy. 2011 (968283): 1–22. arXiv:1006.2483. MACHO들은 우리 은하의 비발광 질량의 아주 작은 비율만을 설명할 수 있으며, 이는 대부분의 암흑 물질이 강하게 집중될 수 없거나 중입자 천체 물리학 물체의 형태로 존재할 수 없다는 것을 보여준다. 마이크로 렌즈 조사가 우리 은하계 해일로에서 갈색 왜성, 블랙홀, 중성자별과 같은 중입자성 물체를 배제하지만, 다른 형태의 중입자성 물질이 대부분의 암흑 물질을 구성할 수 있을까? 놀랍게도 대답은 '아니오'이다..."
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Garrett, Katherine; Dūda, Gintaras (2011). "Dark Matter: A Primer". Advances in Astronomy. 2011 (968283): 1–22. arXiv:1006.2483. MACHO들은 우리 은하의 비발광 질량의 아주 작은 비율만을 설명할 수 있으며, 이는 대부분의 암흑 물질이 강하게 집중될 수 없거나 중입자 천체 물리학 물체의 형태로 존재할 수 없다는 것을 보여준다. 마이크로 렌즈 조사가 우리 은하계 해일로에서 갈색 왜성, 블랙홀, 중성자별과 같은 중입자성 물체를 배제하지만, 다른 형태의 중입자성 물질이 대부분의 암흑 물질을 구성할 수 있을까? 놀랍게도 대답은 '아니오'이다..."
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영향력 있는 논문은 1980년에 루빈과 포드의 결과를 발표했다.Rubin, V.; Thonnard, W.K. Jr.; Ford, N. (1980). "Rotational Properties of 21 Sc Galaxies with a Large Range of Luminosities and Radii from NGC 4605 (R = 4kpc) to UGC 2885 (R = 122kpc)". The Astrophysical Journal. 238: 471. Bibcode:1980ApJ...238..471R.
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jhu.edu
releases.jhu.edu
"Did gravitational wave detector find dark matter?". Johns Hopkins University. 15 June 2016. Retrieved 20 June 2015. 그들의 존재가 확실하게 확립되지는 않았지만 원시 블랙홀은 과거에 암흑 물질 신비에 대한 가능한 해결책으로 제안되었다. 그러나 그것들에 대한 증거가 너무 적기 때문에 원시 블랙홀-암흑 물질 가설은 과학자들 사이에서 큰 지지를 얻지 못했다. 그러나 LIGO의 발견은 특히 그 실험에서 감지된 물체가 암흑 물질에 대해 예측된 질량과 일치하기 때문에 가능성을 새롭게 제시한다. 과거에 과학자들이 만든 예측은 우주 탄생 당시의 조건을 유지하면서 우주에 거의 균일하게 분포되어 은하 주변의 해일로로 무리를 이루는 원시 블랙홀을 많이 생성할 것이다. 이 모든 것이 암흑 물질의 좋은 후보가 될 것이다.
kavlifoundation.org
"Blowing in the Wind"Archived 2020년 10월 7일 - 웨이백 머신. Kavli News. Sheffield: Kavli Foundation. Retrieved 7 January 2014. Scientists at Kavli MIT are working on ... a tool to track the movement of dark matter."
lbl.gov
pdg.lbl.gov
Drees, M.; Gerbier, G. (2015). "Dark Matter" (PDF). Chin. Phys. C. 38: 090001.
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Kuijken, Konrad; Heymans, Catherine; Hildebrandt, Hendrik; Nakajima, Reiko; Erben, Thomas; Jong, Jelte T. A.; Viola, Massimo; Choi, Ami; Hoekstra, Henk; Miller, Lance; van Uitert, Edo (10 October 2015). "Gravitational lensing analysis of the Kilo-Degree Survey". Monthly Notices of the Royal Astronomical Society. 454 (4): 3500–3532.
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Baumann, Daniel. "Cosmology: Part III" (PDF). Mathematical Tripos. Cambridge University. pp. 21–22. Archived from the original (PDF) on 2 February 2017.
"Blowing in the Wind"Archived 2020년 10월 7일 - 웨이백 머신. Kavli News. Sheffield: Kavli Foundation. Retrieved 7 January 2014. Scientists at Kavli MIT are working on ... a tool to track the movement of dark matter."
