Revisiting Flat Rotation Curves in Chern-Simons Modified Gravity

Abstract

We revisit slow rotating black hole (BH) solutions in Chern-Simons modified gravity (CSMG) by considering perturbative solution about Schwarzschild BH. In particular, the case when nondynamical CSMG with noncanonical CS scalar is considered. We provide a new solution different from the previously obtained one \cite{Konno:2007ze} which we refer to as KMT model. The present solution accounts for frame dragging effect which includes not only radial dependence as in the KMT. Nevertheless, it reduces to KMT as a particular case. We show that the tidal gravitational force (Kretschmann invariant) associated to the present solution contains a term of order $1/r^3$ additional to Schwarzschild but absent from directional divergence, unlike KMT model which diverges along the axis of symmetry. We derive the corresponding circular velocity of a massive test particle in which the KMT velocity is recovered in addition to an extra term $\propto r$. We investigate possible constraints on KMT and the present solutions from the observed rotation curve of UGC11455 galaxy as an example. We show that perturbation solutions cannot physically explain the flattening of galactic rotation curves.

13 pages, 2 figures, match the version that will appear in Phys. Lett. B

References in corpus (16)

• GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
• First M87 Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole
• The Confrontation between General Relativity and Experiment
• f(R,T) gravity
• GW170814: A Three-Detector Observation of Gravitational Waves from a Binary Black Hole Coalescence
• Extra force in $f(R)$ modified theories of gravity
• SPARC: Mass Models for 175 Disk Galaxies with Spitzer Photometry and Accurate Rotation Curves
• Timing Measurements of the Relativistic Binary Pulsar PSR B1913+16
• One Law To Rule Them All: The Radial Acceleration Relation of Galaxies
• Dynamical Chern-Simons Modified Gravity I: Spinning Black Holes in the Slow-Rotation Approximation
• Generalized curvature-matter couplings in modified gravity
• How do Black Holes Spin in Chern-Simons Modified Gravity?
• Rotational Velocity Curves in the Milky Way as a Test of Modified Gravity
• Does a black hole rotate in Chern-Simons modified gravity?
• Flat rotation curves in Chern-Simons modified gravity
• Modified Gravitational Theory and Galaxy Rotation Curves