Matter creation and cosmic acceleration

Rudnei O. Ramos, Marcelo Vargas dos Santos, and Ioav Waga
Phys. Rev. D 89, 083524 – Published 9 April 2014

Abstract

We investigate the creation of cold dark matter (CCDM) cosmology as an alternative to explain the cosmic acceleration. Particular attention is given to the evolution of density perturbations and constraints coming from recent observations. By assuming negligible effective sound speed we compare CCDM predictions with redshift-space-distortion based f(z)σ8(z) measurements. We identify a subtle issue associated with which contribution in the density contrast should be used in this test and then show that the CCDM results are the same as those obtained with ΛCDM. These results are then contrasted with the ones obtained at the background level. For the background tests we have used type Ia supernovae data (Union 2.1 compilation) in combination with baryonic acoustic oscillations and cosmic microwave background observations and also measurements of the Hubble parameter at different redshifts. As a consequence of the studies we have performed at both the background and perturbation levels, we explicitly show that CCDM is observationally degenerate with respect to ΛCDM (dark degeneracy). The need to overcome the lack of a fundamental microscopic basis for the CCDM is the major challenge for this kind of model.

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  • Received 3 March 2014

DOI:https://doi.org/10.1103/PhysRevD.89.083524

© 2014 American Physical Society

Authors & Affiliations

Rudnei O. Ramos1,*, Marcelo Vargas dos Santos2,†, and Ioav Waga2,‡

  • 1Departamento de Física Teórica, Universidade do Estado do Rio de Janeiro, 20550-013 Rio de Janeiro, Rio de Janeiro, Brazil
  • 2Instituto de Física, Universidade Federal do Rio de Janeiro, C.P. 68528, 21941-972 Rio de Janeiro, Rio de Janeiro, Brazil

  • *rudnei@uerj.br
  • vargas@if.ufrj.br
  • ioav@if.ufrj.br

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Issue

Vol. 89, Iss. 8 — 15 April 2014

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