Abstract
We investigate generalized chaplygin gas for warm inflationary scenario in the context of locally rotationally symmetric Bianchi type I universe model. We assume two different cases of dissipative coefficient, i.e., constant as well as function of scalar field. We construct dynamical equations as well as a relationship between scalar and radiation energy densities under slow-roll approximation. We also derive slow-roll parameters, scalar and tensor power spectra, scalar spectral index, tensor to scalar ratio for analyzing inflationary background during high dissipative regime. We also use the WMAP7 data for the discussion of our parameters.
Sign-in/Register to access full text options 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
