Tham khảo Vật chất tối vô hướng

  1. ↑ Jeremiah P. Ostriker and Paul Steinhardt New Light on Dark Matter
  2. ↑ J. Val Blain biên tập (2005). Trends in Dark Matter Research. Contributors: Reginald T. Cahill, F. Siddhartha Guzman, N. Hiotelis, A.A. Kirillov, V.E. Kuzmichev, V.V. Kuzmichev, A. Miyazaki, Yu. A. Shchekinov, L. Arturo Urena-Lopez, E.I. Vorobyov. Nova Publishers. tr. 40. ISBN 978-1-59454-248-0. 
  3. ↑ Galaxies are not scattered about the universe in a random way, but rather form an intricate network of filaments, sheets, and clusters. How these large-scale structures formed is at the root of many key questions in cosmology.
  4. ↑ Baldeschi, M. R.; Gelmini, G. B.; Ruffini, R. (ngày 10 tháng 3 năm 1983). “On massive fermions and bosons in galactic halos”. Physics Letters B 122 (3): 221–224. Bibcode:1983PhLB..122..221B. doi:10.1016/0370-2693(83)90688-3. 
  5. ↑ Membrado, M.; Pacheco, A. F.; Sañudo, J. (ngày 1 tháng 4 năm 1989). “Hartree solutions for the self-Yukawian boson sphere”. Physical Review A 39 (8): 4207–4211. Bibcode:1989PhRvA..39.4207M. doi:10.1103/PhysRevA.39.4207. 
  6. ↑ Matos, Tonatiuh; Ureña-López, L. Arturo (2000). “LETTER TO THE EDITOR: Quintessence and scalar dark matter in the Universe”. Classical and Quantum Gravity 17 (13): L75. Bibcode:2000CQGra..17L..75M. arXiv:astro-ph/0004332. doi:10.1088/0264-9381/17/13/101. 
  7. ↑ Matos, Tonatiuh; Arturo Ureña-López, L. (2001). “Further analysis of a cosmological model with quintessence and scalar dark matter”. Physical Review D 63 (6): 063506. Bibcode:2001PhRvD..63f3506M. arXiv:astro-ph/0006024. doi:10.1103/PhysRevD.63.063506. 
  8. ↑ Sahni, Varun; Wang, Limin (2000). “New cosmological model of quintessence and dark matter”. Physical Review D 62 (10): 103517. Bibcode:2000PhRvD..62j3517S. arXiv:astro-ph/9910097. doi:10.1103/PhysRevD.62.103517. 
  9. 1 2 Lee, Jae-Weon; Koh, In-Gyu (1996). “Galactic halos as boson stars”. Physical Review D 53 (4): 2236–2239. Bibcode:1996PhRvD..53.2236L. arXiv:hep-ph/9507385. doi:10.1103/PhysRevD.53.2236. 
  10. ↑ Sin, Sang-Jin; Urena-Lopez, L. A. (1994). “Late-time phase transition and the galactic halo as a Bose liquid”. Physical Review D 50 (6): 3650–3654. Bibcode:1994PhRvD..50.3650S. arXiv:hep-ph/9205208. doi:10.1103/PhysRevD.50.3650. 
  11. ↑ Alcubierre, Miguel; Guzmán, F. Siddhartha; Matos, Tonatiuh; Núñez, Darío; Ureña-López, L. Arturo; Wiederhold, Petra (2002). “Galactic collapse of scalar field dark matter”. Classical and Quantum Gravity 19 (19): 5017–5024. Bibcode:2002CQGra..19.5017A. arXiv:gr-qc/0110102. doi:10.1088/0264-9381/19/19/314. 
  12. ↑ Guzmán, F. Siddhartha; Ureña-López, L. Arturo (2004). “Evolution of the Schrödinger-Newton system for a self-gravitating scalar field”. Physical Review D 69 (12): 124033. Bibcode:2004PhRvD..69l4033G. arXiv:gr-qc/0404014. doi:10.1103/PhysRevD.69.124033. 
  13. ↑ Guzmán, F. Siddhartha; Ureña-López, L. Arturo (2006). “Gravitational Cooling of Self-gravitating Bose Condensates”. The Astrophysical Journal 645 (2): 814–819. Bibcode:2006ApJ...645..814G. arXiv:astro-ph/0603613. doi:10.1086/504508. 
  14. ↑ Bernal, Argelia; Guzmán, F. Siddhartha (2006). “Scalar field dark matter: Nonspherical collapse and late-time behavior”. Physical Review D 74 (6): 063504. Bibcode:2006PhRvD..74f3504B. arXiv:astro-ph/0608523. doi:10.1103/PhysRevD.74.063504. 

Tài liệu tham khảo

WikiPedia: Vật chất tối vô hướng http://www.sciam.com/article.cfm?chanID=sa004&arti... http://adsabs.harvard.edu/abs/1983PhLB..122..221B http://adsabs.harvard.edu/abs/1989PhRvA..39.4207M http://adsabs.harvard.edu/abs/1994PhRvD..50.3650S http://adsabs.harvard.edu/abs/1996PhRvD..53.2236L http://adsabs.harvard.edu/abs/2000CQGra..17L..75M http://adsabs.harvard.edu/abs/2000PhRvD..62j3517S http://adsabs.harvard.edu/abs/2001PhRvD..63f3506M http://adsabs.harvard.edu/abs/2002CQGra..19.5017A http://adsabs.harvard.edu/abs/2004PhRvD..69l4033G