Vector disformal transformation of cosmological perturbations

Abstract : We study disformal transformations of cosmological perturbations by vector fields in theories invariant under U(1) gauge transformations. Three types of vector disformal transformations are considered: (i) disformal transformations by a single timelike vector; (ii) disformal transformations by a single spacelike vector; and (iii) disformal transformations by three spacelike vectors. We show that transformations of type (i) do not change either curvature perturbation or gravitational waves; that those of type (ii) do not change curvature perturbation but change gravitational waves; and that those of type (iii) change both curvature perturbation and gravitational waves. Therefore, coupling matter fields to the metric after disformal transformations of type (ii) or (iii) in principle have observable consequences. While the recent multi-messenger observation of binary neutron stars has singled out a proper disformal frame at the present epoch with a high precision, the result of the present paper may thus help distinguishing disformal frames in the early universe.
Liste complète des métadonnées

https://hal.archives-ouvertes.fr/hal-01757861
Contributeur : Inspire Hep <>
Soumis le : mercredi 4 avril 2018 - 09:52:47
Dernière modification le : mardi 19 mars 2019 - 22:36:52

Lien texte intégral

Identifiants

Collections

Citation

Vassilis Papadopoulos, Moslem Zarei, Hassan Firouzjahi, Shinji Mukohyama. Vector disformal transformation of cosmological perturbations. Phys.Rev.D, 2018, 97 (6), pp.063521. 〈10.1103/PhysRevD.97.063521〉. 〈hal-01757861〉

Partager

Métriques

Consultations de la notice

51