COSMOLOGICAL CONSTRAINTS FOR THE COSMIC DEFECT THEORY

Author:

RADICELLA NINFA1,SERENO MAURO23,TARTAGLIA ANGELO23

Affiliation:

1. Departament de Física, Universitat Autònoma de Barcelona, Spain

2. Dipartimento di Fisica, Politecnico di Torino, Corso Duca degli Abruzzi 24, Torino, 10129, Italy

3. INFN, Sezione di Torino, Via Pietro Giuria 1, Torino, 10125, Italy

Abstract

The cosmic defect theory has been confronted with four observational constraints: primordial nuclear species abundances emerging from the big bang nucleosynthesis; large scale structure formation in the Universe; cosmic microwave background acoustic scale; luminosity distances of type Ia supernovae. The test has been based on a statistical analysis of the a posteriori probabilities for three parameters of the theory. The result has been quite satisfactory and such that the performance of the theory is not distinguishable from that of the ΛCDM theory. The use of the optimal values of the parameters for the calculation of the Hubble constant and the age of the Universe confirms the compatibility of the cosmic defect approach with observations.

Publisher

World Scientific Pub Co Pte Lt

Subject

Space and Planetary Science,Astronomy and Astrophysics,Mathematical Physics

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