arXiv · astro-ph/0605388
Inflation is the generic feature of phantom field-not the big-rip
Abstract
A class of solutions for phantom field corresponding to a generalized k-essence lagrangian has been presented, employing a simple method which provides the scope to explore many such. All the solutions having dynamical state parameter are found to touch the magic line w = -1, asymptotically. The solutions with constant equation of state can represent phantom, quitessence or an ordinary scalar field cosmologies depending on the choice of a couple of parameters of the theory. For w approximately equal to -1, quintessence and phantom models are indistinguishable through the Hubble parameter. Finally, inflation rather than big-rip has been found to be the generic feature of phantom cosmology.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
Abhik Kumar Sanyal. 2006-05-16. Inflation is the generic feature of phantom field-not the big-rip. https://doi.org/10.1142/s0217751x07035173
Cite the original work for its findings. Save a collection to share your selection of sources.