Tham khảo Vật_chất_tối_vô

Tham khảo Vật_chất_tối_vô_hướng

↑ Jeremiah P. Ostriker and Paul Steinhardt New Light on Dark Matter
↑ 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.
↑ 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.
↑ 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.
↑ 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.
↑ 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. arXiv:astro-ph/0004332. Bibcode:2000CQGra..17L..75M. doi:10.1088/0264-9381/17/13/101.
↑ 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. arXiv:astro-ph/0006024. Bibcode:2001PhRvD..63f3506M. doi:10.1103/PhysRevD.63.063506.
↑ Sahni, Varun; Wang, Limin (2000). “New cosmological model of quintessence and dark matter”. Physical Review D. 62 (10): 103517. arXiv:astro-ph/9910097. Bibcode:2000PhRvD..62j3517S. doi:10.1103/PhysRevD.62.103517.
1 2 Lee, Jae-Weon; Koh, In-Gyu (1996). “Galactic halos as boson stars”. Physical Review D. 53 (4): 2236–2239. arXiv:hep-ph/9507385. Bibcode:1996PhRvD..53.2236L. doi:10.1103/PhysRevD.53.2236.
↑ 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. arXiv:hep-ph/9205208. Bibcode:1994PhRvD..50.3650S. doi:10.1103/PhysRevD.50.3650.
↑ 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. arXiv:gr-qc/0110102. Bibcode:2002CQGra..19.5017A. doi:10.1088/0264-9381/19/19/314.
↑ 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. arXiv:gr-qc/0404014. Bibcode:2004PhRvD..69l4033G. doi:10.1103/PhysRevD.69.124033.
↑ Guzmán, F. Siddhartha; Ureña-López, L. Arturo (2006). “Gravitational Cooling of Self-gravitating Bose Condensates”. The Astrophysical Journal. 645 (2): 814–819. arXiv:astro-ph/0603613. Bibcode:2006ApJ...645..814G. doi:10.1086/504508.
↑ Bernal, Argelia; Guzmán, F. Siddhartha (2006). “Scalar field dark matter: Nonspherical collapse and late-time behavior”. Physical Review D. 74 (6): 063504. arXiv:astro-ph/0608523. Bibcode:2006PhRvD..74f3504B. doi:10.1103/PhysRevD.74.063504.

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