Λ is Coming: Parametrizing Freezing Fields

dc.contributor.authorLinder, Eric V.
dc.date.accessioned2017-08-24T10:38:44Z
dc.date.available2017-08-24T10:38:44Z
dc.date.issued2017-03-21
dc.description.abstractWe explore freezing dark energy, where the evolution of the field approaches that of a cosmological constant at late times. We propose two general, two parameter forms to describe the class of freezing field models, in analogy to ones for thawing fields, here based on the physics of the flow parameter or the calibrated w–w′ phase space. Observables such as distances and Hubble parameters are fit to within 0.1%, and the dark energy equation of state generally to within better than 1%, of the exact numerical solutions.ru_RU
dc.identifier.citationLinder, Eric V. (2017) Λ is Coming: Parametrizing Freezing Fields. International conference "ECL17: Exploring the Energetic Universe 2017", Nazarbayev University Energetic Cosmic Laboratoryru_RU
dc.identifier.urihttp://arxiv.org/abs/1701.01445v2
dc.identifier.urihttp://nur.nu.edu.kz/handle/123456789/2547
dc.language.isoenru_RU
dc.publisherInternational conference "ECL17: Exploring the Energetic Universe 2017", Nazarbayev University Energetic Cosmic Laboratoryru_RU
dc.rightsAttribution-NonCommercial-ShareAlike 3.0 United States*
dc.rights.urihttp://creativecommons.org/licenses/by-nc-sa/3.0/us/*
dc.subjectfreezing fieldsru_RU
dc.subjectdark energyru_RU
dc.subjectcosmologyru_RU
dc.subjectHubble parameterru_RU
dc.subjectResearch Subject Categories::NATURAL SCIENCES::Physics::Astronomy and astrophysics::Cosmology
dc.titleΛ is Coming: Parametrizing Freezing Fieldsru_RU
dc.typeArticleru_RU

Files

Original bundle
Now showing 1 - 1 of 1
Loading...
Thumbnail Image
Name:
1701.01445.pdf
Size:
147.06 KB
Format:
Adobe Portable Document Format
Description:
License bundle
Now showing 1 - 1 of 1
No Thumbnail Available
Name:
license.txt
Size:
6.37 KB
Format:
Item-specific license agreed upon to submission
Description: