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強交互作用粒子

十月 23, 2023

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（英语：Cooling flow）[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][來源請求]。

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 编辑

參考資料 编辑

  1. ^ Wandelt, Benjamin D; Dave, Romeel; Farrar, Glennys R; McGuire, Patrick C; Spergel, David N; Steinhardt, Paul J, Self-Interacting Dark Matter, 2000, arXiv:astro-ph/0006344   
  2. ^ Massey, Richard; et al, Dark matter dynamics in Abell 3827: new data consistent with standard Cold Dark Matter, 2017, arXiv:1708.04245   [astro-ph.CO] 
  3. ^ Grossman, Lisa. Dark matter isn’t interacting with itself after all. ScienceNews. April 5, 2018 [2018-04-05]. （原始内容于2018-04-06）. 
  4. ^ Chung, Daniel J. H; Farrar, Glennys R; Kolb, Edward W, Are ultrahigh energy cosmic rays signals of supersymmetry?, 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, Exotic massive hadrons and ultra-high energy cosmic rays, 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, Constraints on the Interaction between Dark Matter and Baryons from Cooling Flow Clusters, 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, Consequences of short range interactions between dark matter and protons in galaxy clusters, 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, Opening the window on strongly interacting dark matter, 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, Constraining Strong Baryon-Dark Matter Interactions with Primordial Nucleosynthesis and Cosmic Rays, 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, A Window in the Dark Matter Exclusion Limits, Physical Review D, 2004, 72 (8): 083502, Bibcode:2005PhRvD..72h3502Z, arXiv:astro-ph/0406531  , doi:10.1103/PhysRevD.72.083502 
  11. ^ 11.0 11.1 Bacci, C.; et al, Improved limits on strongly interacting massive particles with NaI(Tl) scintillators, 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, Cracking Open the Window for Strongly Interacting Massive Particles as the Halo Dark Matter, Proceedings of the International Cosmic Ray Conference, Hamburg, Germany, 2001: 1566, Bibcode:2001ICRC....4.1566M, arXiv:astro-ph/0105567   
  13. ^ Javorsek II, D; Fischbach, E; Teplitz, V, New Experimental Bounds on the Contributions to the Cosmological Density Parameter Ω from Strongly Interacting Massive Particles, The Astrophysical Journal, 2002, 568: 1, Bibcode:2002ApJ...568....1J, doi:10.1086/338796 
  14. ^ Mitra, Saibal, Uranus's anomalously low excess heat constrains strongly interacting dark matter, 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, Towards Closing the Window on Strongly Interacting Dark Matter: Far-Reaching Constraints from Earth's Heat Flow, Physical Review D, 2007, 76 (4): 043523, Bibcode:2007PhRvD..76d3523M, arXiv:0705.4298  , doi:10.1103/PhysRevD.76.043523 

進階讀物 编辑

十月 23, 2023
強交互作用粒子, 此條目需要編修, 以確保文法, 用詞, 语气, 格式, 標點等使用恰当, 2018年6月16日, 請按照校對指引, 幫助编辑這個條目, 幫助, 討論, 此條目需要擴充, 2018年6月16日, 请協助改善这篇條目, 更進一步的信息可能會在討論頁或扩充请求中找到, 请在擴充條目後將此模板移除, 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. 此條目需要編修 以確保文法 用詞 语气 格式 標點等使用恰当 2018年6月16日 請按照校對指引 幫助编辑這個條目 幫助 討論 此條目需要擴充 2018年6月16日 请協助改善这篇條目 更進一步的信息可能會在討論頁或扩充请求中找到 请在擴充條目後將此模板移除 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 英语 Cooling flow 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 來源請求 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 编辑大質量弱相互作用粒子 自交互作用暗物質 英语 Self interacting dark matter 參考資料 编辑 Wandelt Benjamin D Dave Romeel Farrar Glennys R McGuire Patrick C Spergel David N Steinhardt Paul J Self Interacting Dark Matter 2000 arXiv astro ph 0006344 nbsp Massey Richard et al Dark matter dynamics in Abell 3827 new data consistent with standard Cold Dark Matter 2017 arXiv 1708 04245 nbsp astro ph CO Grossman Lisa Dark matter isn t interacting with itself after all ScienceNews April 5 2018 2018 04 05 原始内容存档于2018 04 06 Chung Daniel J H Farrar Glennys R Kolb Edward W Are ultrahigh energy cosmic rays signals of supersymmetry Physical Review D 1997 57 8 4606 Bibcode 1998PhRvD 57 4606C arXiv astro ph 9707036 nbsp doi 10 1103 PhysRevD 57 4606 Albuquerque Ivone F M Farrar Glennys R Kolb Edward W Exotic massive hadrons and ultra high energy cosmic rays Physical Review D 1998 59 1 015021 Bibcode 1999PhRvD 59a5021A arXiv hep ph 9805288 nbsp doi 10 1103 PhysRevD 59 015021 Qin Bo Wu Xiang Ping Constraints on the Interaction between Dark Matter and Baryons from Cooling Flow Clusters Physical Review Letters 2001 87 6 061301 Bibcode 2001PhRvL 87f1301Q arXiv astro ph 0106458 nbsp doi 10 1103 PhysRevLett 87 061301 Chuzhoy Leonid Nusser Adi Consequences of short range interactions between dark matter and protons in galaxy clusters The Astrophysical Journal 2004 645 2 950 954 Bibcode 2006ApJ 645 950C arXiv astro ph 0408184 nbsp doi 10 1086 504505 Starkman Glenn D Gould Andrew Esmailzadeh Rahim Dimopoulos Savas Opening the window on strongly interacting dark matter Physical Review D 1990 41 12 3594 Bibcode 1990PhRvD 41 3594S doi 10 1103 PhysRevD 41 3594 Cyburt Richard H Fields Brian D Pavlidou Vasiliki Wandelt Benjamin D Constraining Strong Baryon Dark Matter Interactions with Primordial Nucleosynthesis and Cosmic Rays Physical Review D 2002 65 12 123503 Bibcode 2002PhRvD 65l3503C arXiv astro ph 0203240 nbsp doi 10 1103 PhysRevD 65 123503 Zaharijas Gabrijela Farrar Glennys R A Window in the Dark Matter Exclusion Limits Physical Review D 2004 72 8 083502 Bibcode 2005PhRvD 72h3502Z arXiv astro ph 0406531 nbsp doi 10 1103 PhysRevD 72 083502 11 0 11 1 Bacci C et al Improved limits on strongly interacting massive particles with NaI Tl scintillators Astroparticle Physics 1996 4 3 195 198 Bibcode 1996APh 4 195B doi 10 1016 0927 6505 95 00032 1 McGuire Patrick C Steinhardt Paul J Cracking Open the Window for Strongly Interacting Massive Particles as the Halo Dark Matter Proceedings of the International Cosmic Ray Conference Hamburg Germany 2001 1566 Bibcode 2001ICRC 4 1566M arXiv astro ph 0105567 nbsp Javorsek II D Fischbach E Teplitz V New Experimental Bounds on the Contributions to the Cosmological Density Parameter W from Strongly Interacting Massive Particles The Astrophysical Journal 2002 568 1 Bibcode 2002ApJ 568 1J doi 10 1086 338796 Mitra Saibal Uranus s anomalously low excess heat constrains strongly interacting dark matter Physical Review D 2004 70 10 103517 Bibcode 2004PhRvD 70j3517M arXiv astro ph 0408341 nbsp doi 10 1103 PhysRevD 70 103517 Mack Gregory D Beacom John F Bertone Gianfranco Towards Closing the Window on Strongly Interacting Dark Matter Far Reaching Constraints from Earth s Heat Flow Physical Review D 2007 76 4 043523 Bibcode 2007PhRvD 76d3523M arXiv 0705 4298 nbsp doi 10 1103 PhysRevD 76 043523 進階讀物 编辑Bertone Gianfranco Particle Dark Matter Observations Models and Searches Cambridge University Press 2010 762 ISBN 978 0 521 76368 4 Sharpe Dan Exploring Composite Dark Matter with SIDM and CDM 2017 2018 06 16 ISBN 1520306318 原始内容存档于2018 01 22 取自 https zh wikipedia org w index php title 強交互作用粒子 amp oldid 62290124, 维基百科，wiki，书籍，书籍，图书馆，

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