Mass and force relations for extremal Einstein-Maxwell-dilaton-axion black holes
Creators
- 1. Department of Physics, Lehigh University, Bethlehem, Pennsylvania 18018, USA
- 2. Department of Physics and Astronomy, University of Pennsylvania, Philadelphia, Pennsylvania 19104, USA
- 3. George P. & Cynthia Woods Mitchell Institute for Fundamental Physics and Astronomy, Texas A&M University, College Station, Texas 77843, USA
- 4. Feza Gursey Center for Physics and Mathematics, Bogazici University, Kandilli 34684, Istanbul, Türkiye
Description
We investigate various properties of extremal dyonic static black holes in Einstein-Maxwell-Dilaton-Axion theory. We obtain a simple first-order ordinary differential equation for the black hole mass in terms of its electric and magnetic charges, which we can solve explicitly for certain special values of the scalar couplings. For one such case we also construct new dyonic black hole solutions, making use of the presence of an enhanced $ SL(2,\mathbb{R})$ symmetry. Finally, we investigate the structure of long range forces and binding energies between nonequivalent extremal black holes. For certain special cases, we can identify regions of parameter space where the force is always attractive or repulsive. Unlike in the case without an axion, the force and binding energies between distinct black holes are not always correlated with each other. Our work is motivated in part by the question of whether long range forces between nonidentical states can potentially encode information about UV constraints on low-energy physics.
Files
PhysRevD.111.066008.pdf
Files
(269.8 kB)
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