TY  - INPR
A1  - Benisty, David
A1  - Vasak, David
A1  - Struckmeier, Jürgen
A1  - Stöcker, Horst
T1  - Bounding Dark Energy from the SPARC rotation curves: Data driven probe for galaxy virialization
T2  - arXiv
N2  - Dark Energy (DE) acts as a repulsive force that opposes gravitational attraction. Assuming galaxies maintain a steady state over extended periods, the estimated upper bound on DE studies its resistance to the attractive gravitational force from dark matter. Using the SPARC dataset, we fit the Navarro-Frenk-White (NFW) and Hernquist models to identify the most suitable galaxies for these models. Introducing the presence of DE in these galaxies helps establish the upper limit on its repulsive force. This upper bound on DE sits around ρ(<Λ)∼10−25~kg/m3, only two orders of magnitude higher than the one measured by Planck. We discuss the conditions for detecting DE in different systems and show the consistency of the upper bound from galaxies to other systems. The upper bound is of the same order of magnitude as ρ200=200ρc for both dark matter profiles. We also address the implications for future measurements on that upper bound and the condition for detecting the impact of Λ on galactic scales.
Y1  - 2024
UR  - http://publikationen.ub.uni-frankfurt.de/frontdoor/index/index/docId/86290
UR  - https://nbn-resolving.org/urn:nbn:de:hebis:30:3-862903
UR  - https://arxiv.org/abs/2405.16650v1
IS  - 2405.16650v1
PB  - arXiv
ER  -