頂夸克
參考來源

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↑  Ellis, Espinosa, Giudice, Hoecker, & Riotto, J.; Espinosa, J.R.; Giudice, G.F.; Hoecker, A.; Riotto, A. . Phys. Lett. B. 2009, 679 (4): 369–375. Bibcode:2009PhLB..679..369E. arXiv:0906.0954 . doi:10.1016/j.physletb.2009.07.054.
↑  Masina, Isabella. . Phys. Rev. D. 2013-02-12, 87 (5): 53001. Bibcode:2013PhRvD..87e3001M. arXiv:1209.0393 . doi:10.1103/PhysRevD.87.053001. （原始内容存档于2013-04-14）.
↑  Irene Klotz (editing by David Adams and Todd Eastham). . Huffington Post. Reuters. 2013-02-18  [21 February 2013]. （原始内容存档于2017-09-07）. Earth will likely be long gone before any Higgs boson particles set off an apocalyptic assault on the universe
↑   For example, Huffington Post/Reuters
↑  Boyle, Alan. . NBC News' Cosmic log. 2013-02-19  [21 February 2013]. （原始内容存档于2013-02-21）. [T]he bad news is that its mass suggests the universe will end in a fast-spreading bubble of doom. The good news? It'll probably be tens of billions of years . The article quotes Fermilab's Joseph Lykken: "[T]he parameters for our universe, including the Higgs [and top quark's masses] suggest that we're just at the edge of stability, in a "metastable" state. Physicists have been contemplating such a possibility for more than 30 years. Back in 1982, physicists Michael Turner and Frank Wilczek wrote in Nature that "without warning, a bubble of true vacuum could nucleate somewhere in the universe and move outwards..."
↑  Peralta, Eyder. . npr – two way. 2013-02-19  [21 February 2013]. （原始内容存档于2015-05-04）.  Article cites Fermilab's Joseph Lykken: "The bubble forms through an unlikely quantum fluctuation, at a random time and place,"
繪圖顯示，宇宙是否穩定，還是只是長壽泡沫，這要依希格斯玻色子與頂夸克的質量而定。直至2012年為止，從兆電子伏特加速器與大型強子對撞機實驗數據得到的2σ橢圓，仍舊允許這兩種可能結局。