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Research output: Contribution to Journal/Magazine › Journal article › peer-review
Research output: Contribution to Journal/Magazine › Journal article › peer-review
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TY - JOUR
T1 - Quintessence in the Weyl-Gauss-Bonnet model
AU - Terente Diaz, Jose
AU - Dimopoulos, Konstantinos
AU - Karciauskas, Mindaugas
AU - Racioppi, Antonio
PY - 2024/2/23
Y1 - 2024/2/23
N2 - Quintessence models have been widely examined in the context of scalar-Gauss-Bonnet gravity, a subclass of Horndeski’s theory, and were proposed as viable candidates for Dark Energy. However, the relatively recent observational constraints on the speed of gravitational waves c_GW have resulted in many of those models being ruled out because they predict c_GW ≠ c generally. While these were formulated in the metric formalism of gravity, we put forward a new quintessence model with the scalar-Gauss-Bonnet action but in Weyl geometry, where the connection is not metric compatible. We find the fixed points of the dynamical system under some assumptions and determine their stability via linear analysis. The past evolution of the Universe can be reproduced correctly, but the late Universe constraints on c_GW are grossly violated. Moreover, at these later stages tensor modes suffer from the gradient instabilities. We also consider the implications of imposing an additional constraint c_GW = c, but this does not lead to evolution that is consistent with cosmological observations.
AB - Quintessence models have been widely examined in the context of scalar-Gauss-Bonnet gravity, a subclass of Horndeski’s theory, and were proposed as viable candidates for Dark Energy. However, the relatively recent observational constraints on the speed of gravitational waves c_GW have resulted in many of those models being ruled out because they predict c_GW ≠ c generally. While these were formulated in the metric formalism of gravity, we put forward a new quintessence model with the scalar-Gauss-Bonnet action but in Weyl geometry, where the connection is not metric compatible. We find the fixed points of the dynamical system under some assumptions and determine their stability via linear analysis. The past evolution of the Universe can be reproduced correctly, but the late Universe constraints on c_GW are grossly violated. Moreover, at these later stages tensor modes suffer from the gradient instabilities. We also consider the implications of imposing an additional constraint c_GW = c, but this does not lead to evolution that is consistent with cosmological observations.
U2 - 10.1088/1475-7516/2024/02/040
DO - 10.1088/1475-7516/2024/02/040
M3 - Journal article
VL - 2024
JO - Journal of Cosmology and Astroparticle Physics
JF - Journal of Cosmology and Astroparticle Physics
SN - 1475-7516
IS - 2
M1 - 040
ER -