Article ISI
PHYSICS OF THE DARK UNIVERSE  (2020)

The spin tensor of dark matter and the Hubble parameter tension

Lepe, Samuel

Abstract

Allowing for a nonvanishing spin tensor for cold dark matter (omega(DM) = 0) has the consequence of giving rise to an effective FLRW dynamics with a small negative barotropic constant for an effective dark matter density (-1/3 omega(eff) = 0). This turns out to solve the Hubble parameter tension in a straightforward way. (C) 2020 Elsevier B.V. All rights reserved.

Más información

Título según WOS: The spin tensor of dark matter and the Hubble parameter tension
Título de la Revista: PHYSICS OF THE DARK UNIVERSE
Volumen: 30
Editorial: Elsevier
Fecha de publicación: 2020
DOI:

10.1016/j.dark.2020.100662
Notas: ISI