skip to main content
OSTI.GOV title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: Quintessential inflation on the brane and the relic gravity wave background

Journal Article · · Physical Review. D, Particles Fields
;  [1]
  1. Inter-University Centre for Astronomy and Astrophysics (IUCAA), Post Bag 4, Ganeshkhind, Pune 411 007 (India)

Quintessential inflation describes a scenario in which both inflation and dark energy (quintessence) are described by the same scalar field. In conventional braneworld models of quintessential inflation gravitational particle-production is used to reheat the universe. This reheating mechanism is very inefficient and results in an excessive production of gravity waves which violate nucleosynthesis constraints and invalidate the model. We describe a new method of realizing quintessential inflation on the brane in which inflation is followed by 'instant preheating' (Felder, Kofman and Linde 1999). The larger reheating temperature in this model results in a smaller amplitude of relic gravity waves which is consistent with nucleosynthesis bounds. The relic gravity wave background has a 'blue' spectrum at high frequencies and is a generic byproduct of successful quintessential inflation on the brane.

OSTI ID:
20705447
Journal Information:
Physical Review. D, Particles Fields, Vol. 70, Issue 8; Other Information: DOI: 10.1103/PhysRevD.70.083513; (c) 2004 The American Physical Society; Country of input: International Atomic Energy Agency (IAEA); ISSN 0556-2821
Country of Publication:
United States
Language:
English

Similar Records

Brane assisted quintessential inflation with transient acceleration
Journal Article · Sun Jun 15 00:00:00 EDT 2008 · Physical Review. D, Particles Fields · OSTI ID:20705447

Quintessential inflation with α-attractors
Journal Article · Thu Jun 01 00:00:00 EDT 2017 · Journal of Cosmology and Astroparticle Physics · OSTI ID:20705447

On the possibility of braneworld quintessential inflation
Journal Article · Thu Apr 15 00:00:00 EDT 2010 · Physical Review. D, Particles Fields · OSTI ID:20705447