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Auteurs principaux: Caldwell, Robert R., Linder, Eric V.
Format: Preprint
Publié: 2025
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Accès en ligne:https://arxiv.org/abs/2511.07526
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author Caldwell, Robert R.
Linder, Eric V.
author_facet Caldwell, Robert R.
Linder, Eric V.
contents We clarify the role of the oft-misunderstood Null Energy Condition (NEC) in the context of the current cosmological data. In particular, the NEC implies the sum of the total energy density and pressure satisfies $ρ_{tot}+P_{tot} \ge 0$; the energy conditions do not apply separately to individual components of the cosmological fluid. Consequently, we show that under the current best-fit cosmological model no violation of the NEC takes place, past or future. Further, growth in the energy density of an individual component cannot be used to signal violation of the NEC. We illustrate these points with a worked example whereby misestimation of the matter density leads to a phase during which $ρ_{de} + P_{de} < 0$ for the effective dark energy, followed by a phantom crossing and subsequent $ρ_{de} + P_{de} > 0$. At no time is the NEC violated. We also introduce ``elephant'' and ``chimera'' classes of physics for crossing $w_{de}=-1$.
format Preprint
id arxiv_https___arxiv_org_abs_2511_07526
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Null Impact of the Null Energy Condition in Current Cosmology
Caldwell, Robert R.
Linder, Eric V.
Cosmology and Nongalactic Astrophysics
We clarify the role of the oft-misunderstood Null Energy Condition (NEC) in the context of the current cosmological data. In particular, the NEC implies the sum of the total energy density and pressure satisfies $ρ_{tot}+P_{tot} \ge 0$; the energy conditions do not apply separately to individual components of the cosmological fluid. Consequently, we show that under the current best-fit cosmological model no violation of the NEC takes place, past or future. Further, growth in the energy density of an individual component cannot be used to signal violation of the NEC. We illustrate these points with a worked example whereby misestimation of the matter density leads to a phase during which $ρ_{de} + P_{de} < 0$ for the effective dark energy, followed by a phantom crossing and subsequent $ρ_{de} + P_{de} > 0$. At no time is the NEC violated. We also introduce ``elephant'' and ``chimera'' classes of physics for crossing $w_{de}=-1$.
title Null Impact of the Null Energy Condition in Current Cosmology
topic Cosmology and Nongalactic Astrophysics
url https://arxiv.org/abs/2511.07526