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Non-canonical 3-form dark energy

Vitor da Fonseca
(
- U. Lisbon (main)
)
,
Bruno J. Barros
(
- U. Lisbon (main)
)
,
Tiago Barreiro
(
- U. Lisbon (main) and
- Lusofona U.
)
,
Nelson J. Nunes
(
- U. Lisbon (main)
)

Oct 15, 2024

12 pages

Published in:

Phys.Dark Univ. 47 (2025) 101827

Published: Jan 20, 2025

e-Print:

2410.11658 [gr-qc]

DOI:

10.1016/j.dark.2025.101827 (publication)

View in:

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Abstract: (Elsevier B.V.)

In this study, we meticulously construct a 3-form Lagrangian designed to mimic the dynamics of both dust matter in the past and dark energy driving the acceleration in the present era. A dynamical systems approach is used to investigate the underlying behavior of the cosmological background. By investigating the influence of the potential slope and initial conditions on the dynamical solutions, we identify distinct viable scenarios capable of replicating a De Sitter universe in the present epoch. An intriguing aspect of the model is the existence of solutions describing multiple inflationary phases in which the 3-form self-interacting potential decays rapidly.

Note:

12 pages, 6 figures, 2 tables. V2: matches published version

Dark energy
3-form
Dynamical system

References(59)

Figures(6)

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