15-18 septiembre 2026
Europe/Madrid timezone

Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide

16 sept. 2026 14:25
25m
Oral presentation Afternoon Session (Wednesday)

Ponente

Ozgur Akarsu (Istanbul Technical University (ITU))

Descripción

In general relativity, cosmic acceleration is a statement about geometry---the timelike defocusing of the comoving congruence---and the field equations source it with mass--energy combinations, not with any equation-of-state ratio. Evolving dark energy is now back at the center of cosmology, and several scenarios under active discussion---sign-switching $\Lambda_{\rm s}$CDM and AdS-to-dS transitions, which simultaneously ease the $H_0$ and $S_8$ tensions and restore $\sum m_\nu$ to physical values, as well as modified-gravity backgrounds recast in GR-like form---feature an effective dark-energy density that is negative in the past and crosses zero at some redshift $z_\dagger$. Our standard language quietly assumes this never happens: $w_{\rm de}<-1/3$ signals repulsion only while $\rho_{\rm de}>0$ and the inequality reverses on the negative branch; the phantom divide $w_{\rm de}=-1$ stops separating anything once the density changes sign; at $\rho_{\rm de}=0$ the ratio $w_{\rm de}$ does not exist, though nothing physical is singular there; and sign-preserving parametrizations such as $w_0$--$w_a$ cannot represent the crossing at all. In this talk, based on arXiv:2607.18008, we ask what defines dark energy when $w$ cannot, and answer with the two combinations the field equations actually use: the active gravitational mass density $\mathcal{M}=\rho+3p$, which drives Raychaudhuri defocusing, and the inertial mass density $\mathcal{I}=\rho+p$, whose zero---the null energy condition (NEC) boundary---replaces the phantom divide as the regular separator. Sharp results follow: any smooth sign switch is phantom-like and repulsive at the crossing, with the total NEC intact; the pole in $w_{\rm de}$ is purely kinematic, with universal residue $n(1+z_\dagger)/3$, so $w_{\rm de}=-1$ is never attained and the two sides of the divide connect only through the pole; repulsion begins strictly before the switch, at $z_{\rm rep}>z_\dagger$; an exact window in $\rho_{\rm de}'(z_\dagger)$ permits acceleration at the crossing itself; and the deceleration parameter admits exactly one or three sign-changing zeros. An analytic $\Lambda_{\rm s}$CDM profile, exponential infrared $f(T)$ gravity, and the minimal phantom brane realize the pattern. The practical moral for reconstructions: across $\rho_{\rm de}=0$ the regular targets are $(\rho_{\rm de},p_{\rm de},\mathcal{I}_{\rm de},\mathcal{M}_{\rm de})$---kinematic totals need no dark-sector split---and parametrizations should be allowed to change sign.

Autor primario

Ozgur Akarsu (Istanbul Technical University (ITU))

Coautores

Antonio De Felice (Kyoto University) Merve Uzun (Istanbul Technical University)

Materiales de la presentación

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