Constraints on Braneworld Gravity Models from a Kinematic Limit on the Age of the Black Hole XTE J1118+480
arXiv:astro-ph/0612611 · doi:10.1103/PhysRevLett.98.181101
Abstract
In braneworld gravity models with a finite AdS curvature in the extra dimension, the AdS/CFT correspondence leads to a prediction for the lifetime of astrophysical black holes that is significantly smaller than the Hubble time, for asymptotic curvatures that are consistent with current experiments. Using the recent measurements of the position, three-dimensional spatial velocity, and mass of the black hole XTE J1118+480, I calculate a lower limit on its kinematic age of 11 Myr (95% confidence). This translates into an upper limit for the asymptotic AdS curvature in the extra dimensions of 0.08 mm, which significantly improves the limit obtained by table-top experiments of sub-mm gravity.
4 pages, to appear in the Physical Review Letters
References in corpus (16)
- A Large Mass Hierarchy from a Small Extra Dimension
- An Alternative to Compactification
- The Hierarchy Problem and New Dimensions at a Millimeter
- New Dimensions at a Millimeter to a Fermi and Superstrings at a TeV
- Sub-millimeter tests of the gravitational inverse-square law: A search for "large" extra dimensions
- Black Holes in Theories with Large Extra Dimensions: a Review
- The distances to Galactic low-mass X-ray binaries: consequences for black hole luminosities and kicks
- Classical black hole evaporation in Randall-Sundrum infinite braneworld
- A high-velocity black hole on a Galactic-halo orbit in the solar neighborhood
- A Black Hole of > 6 Solar Masses in the X-ray Nova XTE J1118+480
- Luminous and Dark Matter in the Milky Way
- The Halo Black-Hole X-ray Transient XTE J1118+480
- Black Hole Astrophysics in AdS Braneworlds
- Has the black hole in XTE J1118+480 experienced an asymmetric natal kick?
- On the existence and dynamics of braneworld black holes
- XTE J1118+480: A Metal-Rich Black Hole Binary in the Galactic Halo
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