Clustering of dark energy

F. G. Alvarenga; J. C. Fabris; S. V. B. Gonçalves; G. Tadaiesky

doi:10.1103/PhysRevD.66.047302

Access by Xinjiang University

Clustering of dark energy

F. G. Alvarenga^*, J. C. Fabris^†, S. V. B. Gonçalves^‡, and G. Tadaiesky^§

Departamento de Física, Universidade Federal do Espírito Santo, 29060-900, Vitória, Espírito Santo, Brazil

^*Email address: flavio@cce.ufes.br
^†Email address: fabris@cce.ufes.br
^‡Email address: sergio@cce.ufes.br
^§Email address: gtadaiesky@cce.ufes.br

PDF

Phys. Rev. D 66, 047302 – Published 14 August, 2002

DOI: https://doi.org/10.1103/PhysRevD.66.047302

Abstract

A cosmological model with pressureless matter and a fluid of negative pressure is studied. At the perturbative level, fluctuations of both fluids are considered. It is shown that, at least at very large scales, the fluid of negative pressure, which represents the dark energy content of the universe, clusters like the dust fluid. Numerical integration reveals that this behavior may also occur at scales smaller than the Hubble radius.

References (18)

S.M. Kent and J.E. Gunn, Astron. J. 87, 7 (1982).
C.H. Lineweaver, “Cosmological parameters,” astro-ph/ 0112381.
R.R. Caldwell, R. Dave, and P.J. Steinhardt, Phys. Rev. Lett. 80, 1582 (1998).
J.C. Fabris and J. Martin, Phys. Rev. D 55, 5205 (1997).
E. Lokas, Acta Phys. Pol. B 32, 3643 (2001).
S. Weinberg, Gravitation and Cosmology (Wiley, New York, 1972).
P.J.E. Peebles, Principles of Physical Cosmology (Princeton University Press, Princeton, 1993).
E.W. Kolb and M.S. Turner, The Early Universe (Addison-Wesley, Redwood, 1990).
J.C. Fabris, S.V.B. Gonçalves, and N. Tomimura, Class. Quantum Grav. 17, 2983 (2000).
L.P. Grishchuk, Phys. Rev. D 50, 7154 (1994).
C. Wetterich, Phys. Lett. B 522, 5 (2001).
A. Starobinsky, JETP Lett. 68, 757 (1998).
D. Podolsky, Astron. Lett. 28, 434 (2002).
J.C. Fabris, S.V.B. Gonçalves, and P.E. de Souza, Gen. Relativ. Gravit. 34, 53 (2002).
A. Kamenshchik, U. Moschella, and V. Pasquier, Phys. Lett. B 511, 265 (2001).
J.C. Fabris, S.V.B. Gonçalves, and P.E. de Souza, “Power spectrum in a universe dominated by the Chaplygin gas,” astro-ph/0203441.
N. Bilic, G.B. Tupper, and R.D. Viollier, Phys. Lett. B 535, 17 (2002).
F. Perrota and C. Baccigalupi, Phys. Rev. D 65, 123505 (2002).

[c1] S.M. Kent and J.E. Gunn, Astron. J. 87, 7 (1982).

[c2] C.H. Lineweaver, “Cosmological parameters,” astro-ph/ 0112381.

[c3] R.R. Caldwell, R. Dave, and P.J. Steinhardt, Phys. Rev. Lett. 80, 1582 (1998).

[c4] J.C. Fabris and J. Martin, Phys. Rev. D 55, 5205 (1997).

[c5] E. Lokas, Acta Phys. Pol. B 32, 3643 (2001).

[c6] S. Weinberg, Gravitation and Cosmology (Wiley, New York, 1972).

[c7] P.J.E. Peebles, Principles of Physical Cosmology (Princeton University Press, Princeton, 1993).

[c8] E.W. Kolb and M.S. Turner, The Early Universe (Addison-Wesley, Redwood, 1990).

[c9] J.C. Fabris, S.V.B. Gonçalves, and N. Tomimura, Class. Quantum Grav. 17, 2983 (2000).

[c10] L.P. Grishchuk, Phys. Rev. D 50, 7154 (1994).

[c11] C. Wetterich, Phys. Lett. B 522, 5 (2001).

[c12] A. Starobinsky, JETP Lett. 68, 757 (1998).

[c13] D. Podolsky, Astron. Lett. 28, 434 (2002).

[c14] J.C. Fabris, S.V.B. Gonçalves, and P.E. de Souza, Gen. Relativ. Gravit. 34, 53 (2002).

[c15] A. Kamenshchik, U. Moschella, and V. Pasquier, Phys. Lett. B 511, 265 (2001).

[c16] J.C. Fabris, S.V.B. Gonçalves, and P.E. de Souza, “Power spectrum in a universe dominated by the Chaplygin gas,” astro-ph/0203441.

[c17] N. Bilic, G.B. Tupper, and R.D. Viollier, Phys. Lett. B 535, 17 (2002).

[c18] F. Perrota and C. Baccigalupi, Phys. Rev. D 65, 123505 (2002).

Physical Review D

Export citation

Export citation

Clustering of dark energy

Abstract

References (18)

Outline

Information

Filter

Filter

Article Lookup

Enter a citation