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Formacion de estructura con campos escalares: la ... - Cinvestav

Formacion de estructura con campos escalares: la ... - Cinvestav

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Bibliografía[1] M.J. Disney, et al. Ga<strong>la</strong>xies appear simpler than expected. Nature, 455:1082, October2008.[2] G. Gentile, B. G. Famaey, H. Zhao, and P. Salucci. Universality of ga<strong>la</strong>ctic surface<strong>de</strong>nsities within one dark halo scale-length. Nature, 461:627, 2009.[3] Chris A. Collins, et. al. Nature, 458:603, 2009.[4] Pieter G. van Dokkum, Mariska Kriek, and Marijn Franx. Nature, 460:717, 2009.[5] Francisco Guzmán and Tonatiuh Matos. Sca<strong>la</strong>r fields as dark matter in spiral ga<strong>la</strong>xies.C<strong>la</strong>ssical and Quantum Gravity, 17:L9–L16, 2000.[6] Francisco Siddartha Guzmán and Luis Arturo Ureña-López. Newtonian col<strong>la</strong>pse ofsca<strong>la</strong>r field dark matter. Phys. Rev. D, 68:024023, Jul 2003.[7] Tonatiuh Matos. Sca<strong>la</strong>r field dark matter quantum effects as dark energy. ArXiv,0909.3634, 2010.[8] Tonatiuh Matos and Luis Arturo Ureña-López. Further analysis of a cosmologicalmo<strong>de</strong>l with quintessence and sca<strong>la</strong>r dark matter. Phys. Rev. D, 63(6):063506, Feb2001.[9] Argelia Bernal and F. Siddhartha Guzman. Sca<strong>la</strong>r field dark matter: Non-sphericalcol<strong>la</strong>pse and <strong>la</strong>te time behavior. Phys. Rev., D74:063504, 2006.[10] F. Siddhartha Guzmán and L. Arturo Ureña López. Evolution of the Schrödinger-Newton system for a self-gravitating sca<strong>la</strong>r field. Phys. Rev. D, 69(12):124033, Jun2004.[11] E. Ma<strong>de</strong>lung. Physik, 40(322), 1926.59

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