Strings in Cosmological and Black Hole Backgrounds: Ring Solutions
H.J. de Vega, I.L. Egusquiza

TL;DR
This paper solves string equations for ring-shaped configurations in cosmological and black hole backgrounds, revealing their asymptotic behaviors, oscillatory regimes, and interactions with black hole horizons, including transmutation phenomena.
Contribution
It provides new exact solutions and detailed analysis of ring-shaped strings in cosmological and black hole spacetimes, including their asymptotic forms and horizon interactions.
Findings
Strings grow or shrink depending on the cosmological scale factor.
Oscillatory regimes with constant size and energy are identified.
Rings can be absorbed or transmute when approaching black hole horizons.
Abstract
The string equations of motion and constraints are solved for a ring shaped Ansatz in cosmological and black hole spacetimes. In FRW universes with arbitrary power behavior [], the asymptotic form of the solution is found for both and and we plot the numerical solution for all times. Right after the big bang (), the string energy decreasess as and the string size grows as for and as for and . Very soon [ ] , the ring reaches its oscillatory regime with frequency equal to the winding and constant size and energy. This picture holds for all values of including string vacua (for which, asymptotically, ). In addition, an exact non-oscillatory ring solution is found. For black hole spacetimes (Schwarzschild, Reissner-Nordstr\oo…
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