English

Optical equations for null strings

General Relativity and Quantum Cosmology 2021-06-16 v1 High Energy Physics - Theory

Abstract

An optical equation for null strings is derived. The equation is similar to Sachs' optical equations for null geodesic congruences. The string optical equation is given in terms of a single complex scalar function ZZ, which is a combination of spin coefficients at the string trajectory. Real and imaginary parts of ZZ determine expansion and rotation of strings. Trajectories of strings can be represented by diagrams in a complex ZZ-plane. Such diagrams allow one to draw some universal features of null strings in different backgrounds. For example, in asymptotically flat space-times ZZ vanishes as future null infinity is approached, that is, gradually shapes of strings are "freezing out". Outgoing gravitational radiation and flows of matter leave ripples on the strings. These effects are encoded in subleading terms of ZZ. String diagrams are demonstrated for rotating and expanding strings in a flat space-time and in cosmological models.

Keywords

Cite

@article{arxiv.2104.04982,
  title  = {Optical equations for null strings},
  author = {Dmitri Fursaev},
  journal= {arXiv preprint arXiv:2104.04982},
  year   = {2021}
}

Comments

21 pages, 3 figures

R2 v1 2026-06-24T01:03:04.768Z