Cargando…
Rapidly descending dark energy and the end of cosmic expansion
If dark energy is a form of quintessence driven by a scalar field [Formula: see text] evolving down a monotonically decreasing potential [Formula: see text] that passes sufficiently below zero, the universe is destined to undergo a series of smooth transitions. The currently observed accelerated exp...
Autores principales: | Andrei, Cosmin, Ijjas, Anna, Steinhardt, Paul J. |
---|---|
Formato: | Online Artículo Texto |
Lenguaje: | English |
Publicado: |
National Academy of Sciences
2022
|
Materias: | |
Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9169868/ https://www.ncbi.nlm.nih.gov/pubmed/35380902 http://dx.doi.org/10.1073/pnas.2200539119 |
Ejemplares similares
-
Introduction to cosmic inflation and dark energy
por: Dimopoulos, Konstantinos
Publicado: (2021) -
Cosmic coincidences: dark matter, mankind, and anthropic cosmology
por: Gribbin, John R, et al.
Publicado: (1989) -
Antimatter dark matter and cosmic rays with AMS
por: Vialle, J P
Publicado: (2001) -
International Workshop on Early Cosmic Structures and the End of the Dark Ages
Publicado: (2002) -
Constraining Dark Energy through the Stability of Cosmic Structures
por: Pavlidou, V., et al.
Publicado: (2014)