Observational constraints on the extended Chaplygin gas inflation

Author:

Kahya E. O.,Pourhassan B.

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference76 articles.

1. Ade, P.A.R., et al. (Planck Collaboration): Planck 2013 results. XV. CMB power spectra and likelihood (2013). arXiv:1303.5075 [astro-ph.CO]

2. Ade, P.A.R., et al. (BICEP2 Collaboration): BICEP2 I: Detection of B-mode Polarization at Degree Angular Scales (2014). arXiv:1403.3985 [astro.ph.CO]

3. Amani, A.R., Pourhassan, B.: Viscous generalized Chaplygin gas with arbitrary α. Int. J. Theor. Phys. 52, 1309 (2013)

4. Amani, A.R., Escamilla-Rivera, C., Faghani, H.R.: Interacting closed string tachyon with modified Chaplygin gas and its stability. Phys. Rev. D 88, 124008 (2013)

5. Ananda, K.N., Bruni, M.: Cosmo-dynamics and dark energy with non-linear equation of state: a quadratic model. Phys. Rev. D 74, 023523 (2006)

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