EDP Sciences Journals List
Advanced Search
Subscriber Authentication Point
Home All issues Volume 421/1 Article
Free access article

Issue A&A
Volume 421, Number 1, July I 2004
Page(s) 71 - 81
Section Cosmology (including clusters of galaxies)
DOI http://dx.doi.org/10.1051/0004-6361:20041090

Abstract (A&A 421 p.71)
References of  A&A 421 p. 71
  • Abramo, L. R. W., & Finelli, F. 2001, Phys. Rev. D, 64, 083513 [NASA ADS] [CrossRef]
  • Albrecht, A., & Skordis, K. 2000, Phys. Rev. Lett., 84, 2076 [NASA ADS] [CrossRef]
  • Alcubierre, A., Guzman, F., Matos, T., et al. 2002, Class. Quant. Grav., 19, 5017 [NASA ADS]
  • Amendola, L. 2000, Phys. Rev. D, 62, 043511 [NASA ADS] [CrossRef]
  • Amendola, L. 2003, Linear and Non-Linear Perturbations in Dark Energy Models [arXiv:astro-ph/0311175]
  • Arbey, A., Lesgourgues, J., & Salati, P. 2001, Phys. Rev. D, 64, 123528 [NASA ADS] [CrossRef]
  • Bagla, J., Jassal, H., & Padmanabhan, T. 2003, Phys. Rev. D, 67, 063504 [NASA ADS] [CrossRef]
  • Bartelmann, M., Perrotta, F., & Baccigalupi, C. 2002, A&A, 396, 21 [EDP Sciences] [NASA ADS]
  • Bartolo, N., Corasaniti, P., Liddle, A. R., & Marquarti, M. 2003, Perturbations in cosmologies with scalar field and a perfect fluid [arXiv:astro-ph/0311503]
  • Battye, R. A., & Weller, J. 2003, Phys. Rev. D, 68, 083506 [NASA ADS] [CrossRef]
  • Brax, P., & Martin, J. 1999, Phys. Lett. B, 468, 40 [NASA ADS] [CrossRef] [MathSciNet]
  • Barreiro, T., Copeland, E., & Nunes, N. J. 2000, Phys. Rev. D, 61 127301
  • Bean, R., & Magueijo, J. 2002, Phys. Rev. D, 66, 063505 [NASA ADS] [CrossRef] [MathSciNet]
  • Caldwell, R. R., Dave, R., & Steinhardt, P. 1998, Ap&SS, 261, 303 [NASA ADS]
  • Causse, M. 2003, A rolling tachyon field for both dark energy and dark halos of galaxies [arXiv:astro-ph/0312206]
  • Dolag, K., Bartelmann, M., Perrotta, F., et al. 2003, Numerical Study of Halo Concentrations in Dark-Energy Cosmologies [arXiv:astro-ph/0309771]
  • Doran, M., Mueller, C., Schaefer, G., & Wetterich, C. 2003, Phys. Rev. D, 68, 063505 [NASA ADS] [CrossRef]
  • Ferreira, P. G., & Joyce, M. 1997, Phys. Rev. Lett., 79, 4740 [NASA ADS] [CrossRef]
  • Giovi, F., Baccigalupi, C., & Perrotta, F. 2003, Weak lensing, structure formation and dark energy [arXiv:astro-ph/0309422]
  • Guzman, F., & Urena-Lopez, L. 2003, Phys. Rev. D, 68, 024023 [NASA ADS] [CrossRef]
  • Hwang, J. C., & Noh, H. 2001, Phys. Rev. D, 64, 103509 [NASA ADS] [CrossRef]
  • Lahav, O., Rees, M. J., Lilje, P. B., Primack, J. R., et al. 1991, MNRAS, 251, 128 [NASA ADS]
  • Landau, L., & Lifshitz, E. 1975, The Classical Theory of Fields, 4th. ed. (Oxford: Pergamon)
  • Linder, E. V., & Jenkins, A. 2003, MNRAS, 346, 573 [NASA ADS] [CrossRef]
  • Lokas, E., & Hoffman, Y. 2001, Nonlinear evolution of spherical perturbation in the universe with cosmological constant and quintessence [arXiv:astro-ph/0108283]
  • Ma, C., Caldwell, R. R., Bode, P., & Wang, L. 1999, ApJ, 521, L1 [NASA ADS] [CrossRef]
  • Maccio, A. V., Bonometto, S. A., Mainini, R., & Klypin, A. 2003a, Structure formation in dynamical dark energy models [arXiv:astro-ph/0309439]
  • Maccio, A. V., Quercellini, C., Mainini, R., Amendola, L., & Bonometto, S. A. 2003b, N-body simulations for coupled dark energy: Halo mass functions and density profiles [arXiv:astro-ph/0309671]
  • Mainini, R., Maccio, A. V., & Bonometto, S. A. 2003a, New Astron., 8, 173 [NASA ADS] [CrossRef]
  • Mainini, R., Maccio, A. V., Bonometto, S. A., & Klypin, A. 2003b, ApJ, 599, 24 [NASA ADS] [CrossRef]
  • Matarrese, S, Pietroni, M., & Schimd, C. 2003, JCAP, 0308, 005 [NASA ADS]
  • Mota, D. F., & Barrow, J. D. 2004a, MNRAS, 349, 281 [NASA ADS] [CrossRef]
  • Mota, D. F., & Barrow, J. D. 2004b, Phys. Lett. B, 581, 141 [NASA ADS] [CrossRef]
  • Padmanabhan, T. 1995, Structure formation in the universe (Cambridge University Press)
  • Padmanabhan, T., & Choudhury, T. 2002, Phys. Rev. D, 66, 081301 [NASA ADS] [CrossRef]
  • Padmanabhan, T. 2002, Phys. Rev. D, 66, 021301 [NASA ADS] [CrossRef]
  • Peacock, J. 1999, Cosmological Physics (Cambridge University Press)
  • Perlmutter, S., Aldering, G., Goldhaber, G., et al. 1999, ApJ, 517, 565 [NASA ADS] [CrossRef]
  • Perrotta, F., Matarrese, S., Pietroni, M., & Schimd, C. 2004, Phys. Rev. D, 69, 084004 [NASA ADS] [CrossRef]
  • Ratra, B., & Peebles, P. 1988, ApJ, 325, L17 [NASA ADS] [CrossRef]
  • Ratra, B., & Peebles, P. 2002, J. Rev. Mod. Phys., 75, 559 [NASA ADS] [MathSciNet]
  • Steinhardt, P. J., Wang, L., & Zlatev, I. 1999, Phys. Rev. D, 59, 123504 [NASA ADS] [CrossRef]
  • Steinhardt, P. 2003, Phil. Trans. Roy. Soc. Lond. A, 361, 2497 [NASA ADS]
  • Tonry, J., Schmidt, B. P., Barris, B., et al. 2003, ApJ, 594, 1 [NASA ADS]
  • Wang, L. M., & Steinhardt, P. J. 1998, ApJ, 508, 483 [NASA ADS] [CrossRef]
  • Weinberg, N., & Kamionkowski, M. 2003, MNRAS, 341, 251 [NASA ADS]
  • Weller, J., Battye, R., & Kneissl, R. 2002, , 88, 231301
  • Wetterich, C. 1988a, Nucl, Phys. B, 302, 645
  • Wetterich, C. 1988b, Nucl. Phys. B, 302, 668 [NASA ADS] [CrossRef]
  • Wetterich, C. 1995, A&A, 301, 321 [NASA ADS]
  • Wetterich, C. 2001, Phys. Lett. B, 522, 5 [NASA ADS] [CrossRef]
  • Wetterich, C. 2002, Phys. Rev. D, 65, 123512 [NASA ADS] [CrossRef] [MathSciNet]
Abstract (A&A 421 p.71)


What is OpenURL?

The OpenURL standard is a protocol for transmission of metadata describing the resource that you wish to access. An OpenURL link contains article metadata and directs it to the OpenURL server of your choice. The OpenURL server can provide access to the resource and also offer complementary services (specific search engine, export of references...). The OpenURL link can be generated by different means.
  • If your librarian has set up your subscription with an OpenURL resolver, OpenURL links appear automatically on the abstract pages.
  • You can define your own OpenURL resolver with your EDPS Account. In this case your choice will be given priority over that of your library.
  • You can use an add-on for your browser (Firefox or I.E.) to display OpenURL links on a page (see http://www.openly.com/openurlref/). You should disable this module if you wish to use the OpenURL server that you or your library have defined.