強交互作用粒子

強交互作用粒子(Strongly interacting massive particles,縮寫 SIMPs),是一種彼此間以強力作用的假設粒子。在碰撞星系阿貝爾 3827,它們似乎是被散射而看起來落後於普通物質的暗物質。儘管與普通物質有微弱的作用,它們還是被推斷可能是暗物質[1]。然而,自那發現之後,根據對群集的進一步觀測,就不在模型中給予考慮[2][3]

強相互作用例子被提出作為解決超高能宇宙射線的問題[4][5],以及沒有冷卻流的星系星團[6][7]

從1990年開始,各種實驗和觀測都對SIMP要成為暗物質產生了限制[8][9][10][11][12][13]

SIMP的湮滅會產生巨大的熱量。DAMA實驗受限於使用的Nal(TI)晶體[11]

測量天王星的能量過剩排除SIMP在150MeV至104 GeV的可能[14]。地球的熱流極大地限制了任何截面[15]

相關條目

參考資料

  1. Wandelt, Benjamin D; Dave, Romeel; Farrar, Glennys R; McGuire, Patrick C; Spergel, David N; Steinhardt, Paul J, , 2000, arXiv:astro-ph/0006344
  2. Massey, Richard; 等, , 2017, arXiv:1708.04245 [astro-ph.CO]
  3. Grossman, Lisa. . ScienceNews. April 5, 2018 [2018-04-05]. (原始内容存档于2018-04-06).
  4. Chung, Daniel J. H; Farrar, Glennys R; Kolb, Edward W, , Physical Review D, 1997, 57 (8): 4606, Bibcode:1998PhRvD..57.4606C, arXiv:astro-ph/9707036, doi:10.1103/PhysRevD.57.4606
  5. Albuquerque, Ivone F. M; Farrar, Glennys R; Kolb, Edward W, , Physical Review D, 1998, 59 (1): 015021, Bibcode:1999PhRvD..59a5021A, arXiv:hep-ph/9805288, doi:10.1103/PhysRevD.59.015021
  6. Qin, Bo; Wu, Xiang-Ping, , Physical Review Letters, 2001, 87 (6): 061301, Bibcode:2001PhRvL..87f1301Q, arXiv:astro-ph/0106458, doi:10.1103/PhysRevLett.87.061301
  7. Chuzhoy, Leonid; Nusser, Adi, , The Astrophysical Journal, 2004, 645 (2): 950–954, Bibcode:2006ApJ...645..950C, arXiv:astro-ph/0408184, doi:10.1086/504505
  8. Starkman, Glenn D; Gould, Andrew; Esmailzadeh, Rahim; Dimopoulos, Savas, , Physical Review D, 1990, 41 (12): 3594, Bibcode:1990PhRvD..41.3594S, doi:10.1103/PhysRevD.41.3594
  9. Cyburt, Richard H; Fields, Brian D; Pavlidou, Vasiliki; Wandelt, Benjamin D, , Physical Review D, 2002, 65 (12): 123503, Bibcode:2002PhRvD..65l3503C, arXiv:astro-ph/0203240, doi:10.1103/PhysRevD.65.123503.
  10. Zaharijas, Gabrijela; Farrar, Glennys R, , Physical Review D, 2004, 72 (8): 083502, Bibcode:2005PhRvD..72h3502Z, arXiv:astro-ph/0406531, doi:10.1103/PhysRevD.72.083502
  11. Bacci, C.; 等, , Astroparticle Physics, 1996, 4 (3): 195–198, Bibcode:1996APh.....4..195B, doi:10.1016/0927-6505(95)00032-1
  12. McGuire, Patrick C; Steinhardt, Paul J, , , Hamburg, Germany, 2001: 1566, Bibcode:2001ICRC....4.1566M, arXiv:astro-ph/0105567
  13. Javorsek II, D; Fischbach, E; Teplitz, V, , The Astrophysical Journal, 2002, 568: 1, Bibcode:2002ApJ...568....1J, doi:10.1086/338796
  14. Mitra, Saibal, , Physical Review D, 2004, 70 (10): 103517, Bibcode:2004PhRvD..70j3517M, arXiv:astro-ph/0408341, doi:10.1103/PhysRevD.70.103517
  15. Mack, Gregory D; Beacom, John F; Bertone, Gianfranco, , Physical Review D, 2007, 76 (4): 043523, Bibcode:2007PhRvD..76d3523M, arXiv:0705.4298, doi:10.1103/PhysRevD.76.043523

進階讀物

  • Bertone, Gianfranco. . Cambridge University Press. 2010: 762. ISBN 978-0-521-76368-4.
  • Sharpe, Dan. . 2017 [2018-06-16]. ISBN 1520306318. (原始内容存档于2018-01-22).
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